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Page 1: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 2: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 3: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 4: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 5: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 6: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 7: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 8: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Today’s Outline - January 20, 2016

• Multiple degenerate states

• Fine structure

• Relativistic correction

• Spin-orbit coupling

Homework Assignment #02:Chapter 5:27,30; Chapter 6:1,4,6,29due Wednesday, January 27, 2016

Homework Assignment #03:Chapter 6:9,17,21,24,25,32due Wednesday, February 3, 2016

Office hours:Monday & Wednesday, 13:50–15:05

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 1 / 14

Page 9: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

⟩H0ψ0

i = E 0ψ0i ,

⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 10: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1

(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

⟩H0ψ0

i = E 0ψ0i ,

⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 11: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

⟩H0ψ0

i = E 0ψ0i ,

⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 12: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

⟩H0ψ0

i = E 0ψ0i ,

⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 13: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

H0ψ0i = E 0ψ0

i ,⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 14: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate

and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

H0ψ0i = E 0ψ0

i ,⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 15: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate

and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

⟩H0ψ0

i = E 0ψ0i ,

⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 16: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

⟩H0ψ0

i = E 0ψ0i ,

⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 17: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Higher order degeneracy

When there are more than two de-generate states, a matrix formula-tion is more useful

The E 1 are the eigenvalues of theW -matrix and the “good” linearcombinations of the unperturbedstates are the eigenvectors of Wij

This can be proven as follows, as-sume that the set of unperturbedeigenfunctions ψ0

i are n-fold degen-erate and that ψ0 is a general lin-ear combination

αWaa + βWab = αE 1

αWba + βWbb = βE 1(Waa Wab

Wba Wbb

)(αβ

)= E 1

(αβ

)

Wij =⟨ψ0i

∣∣H ′∣∣ψ0j

⟩H0ψ0

i = E 0ψ0i ,

⟨ψ0i

∣∣ψ0j

⟩= δij

ψ0 =n∑

i=1

αiψ0i

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 2 / 14

Page 18: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction and eigenvalues

ψ = ψ0 + ψ1 + · · · E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 19: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction and eigenvalues

ψ = ψ0 + ψ1 + · · · E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 20: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j

= E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction and eigenvalues

ψ = ψ0 + ψ1 + · · · E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 21: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j

= E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction and eigenvalues

ψ = ψ0 + ψ1 + · · · E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 22: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction and eigenvalues

ψ = ψ0 + ψ1 + · · · E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 23: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction

and eigenvalues

ψ = ψ0 + ψ1 + · · · E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 24: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction

and eigenvalues

ψ = ψ0 + ψ1 + · · ·

E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 25: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction and eigenvalues

ψ = ψ0 + ψ1 + · · ·

E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 26: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10

In the text it is asserted that the first-order corrections to an n-folddegenerate energy are the eigenvalues of the W matrix, and that this isthe “natural” generalization fo the n = 2 case. Prove this by starting with

ψ0 =n∑

j=1

αjψ0j .

First we note that since each of the n degenerate solutions, ψ0j of H0 has

eigenvalue E 0 and therefore

H0ψ0 =n∑

j=1

αjH0ψ0

j = E 0n∑

j=1

αjψ0j = E 0ψ0

we want to solve for the corrections in the presence of a perturbingHamiltonian, H ′, by expanding the presumed eigenfunction and eigenvalues

ψ = ψ0 + ψ1 + · · · E = E 0 + E 1 + · · ·

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 3 / 14

Page 27: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

Page 28: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ

−→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

Page 29: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

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Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣

������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

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Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= E 0

⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

n∑j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

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Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

n∑j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

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Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

Page 34: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

Page 35: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

Page 36: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Problem 6.10 (cont.)

Gather all the first order combinations of the eigenvalue equation

Hψ = Eψ −→ H0ψ1 + H ′ψ0 = E 0ψ1 + E 1ψ0

take the inner product with⟨ψ0i

∣∣������⟨ψ0i |H0ψ1

⟩+⟨ψ0i |H ′ψ0

⟩= ������

E 0⟨ψ0i |ψ1

⟩+ E 1

⟨ψ0i |ψ0

⟩n∑

j=1

αj

⟨ψ0i |H ′ψ0

j

⟩= E 1

n∑j=1

αj

⟨ψ0i |ψ0

j

⟩= E 1αi

n∑j=1

αjWij = E 1αi , Wij ≡⟨ψ0i |H ′|ψ0

j

⟩this defines n equations in n unknowns, the αi ’s, which together give annth order equation in E 1 whose n solutions are the elements of thediagonalized W -matrix

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 4 / 14

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Problem 6.10 (cont.)

To see this more clearly, rewrite the defining equations in matrix form

W11 W12 W13 · · · W1n

W21 W22 W23 · · · W2n

W31 W32 W33 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn

α1

α2

α3...αn

= E 1

α1

α2

α3...αn

which is solved by a determinant

det

∣∣∣∣∣∣∣∣∣∣∣

W11 − E 1 W12 W13 · · · W1n

W21 W22 − E 1 W23 · · · W2n

W31 W32 W33 − E 1 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn − E 1

∣∣∣∣∣∣∣∣∣∣∣= 0

giving an nth order equation in E 1

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 5 / 14

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Problem 6.10 (cont.)

To see this more clearly, rewrite the defining equations in matrix formW11 W12 W13 · · · W1n

W21 W22 W23 · · · W2n

W31 W32 W33 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn

α1

α2

α3...αn

= E 1

α1

α2

α3...αn

which is solved by a determinant

det

∣∣∣∣∣∣∣∣∣∣∣

W11 − E 1 W12 W13 · · · W1n

W21 W22 − E 1 W23 · · · W2n

W31 W32 W33 − E 1 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn − E 1

∣∣∣∣∣∣∣∣∣∣∣= 0

giving an nth order equation in E 1

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 5 / 14

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Problem 6.10 (cont.)

To see this more clearly, rewrite the defining equations in matrix formW11 W12 W13 · · · W1n

W21 W22 W23 · · · W2n

W31 W32 W33 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn

α1

α2

α3...αn

= E 1

α1

α2

α3...αn

which is solved by a determinant

det

∣∣∣∣∣∣∣∣∣∣∣

W11 − E 1 W12 W13 · · · W1n

W21 W22 − E 1 W23 · · · W2n

W31 W32 W33 − E 1 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn − E 1

∣∣∣∣∣∣∣∣∣∣∣= 0

giving an nth order equation in E 1

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 5 / 14

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Problem 6.10 (cont.)

To see this more clearly, rewrite the defining equations in matrix formW11 W12 W13 · · · W1n

W21 W22 W23 · · · W2n

W31 W32 W33 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn

α1

α2

α3...αn

= E 1

α1

α2

α3...αn

which is solved by a determinant

det

∣∣∣∣∣∣∣∣∣∣∣

W11 − E 1 W12 W13 · · · W1n

W21 W22 − E 1 W23 · · · W2n

W31 W32 W33 − E 1 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn − E 1

∣∣∣∣∣∣∣∣∣∣∣= 0

giving an nth order equation in E 1

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 5 / 14

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Problem 6.10 (cont.)

To see this more clearly, rewrite the defining equations in matrix formW11 W12 W13 · · · W1n

W21 W22 W23 · · · W2n

W31 W32 W33 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn

α1

α2

α3...αn

= E 1

α1

α2

α3...αn

which is solved by a determinant

det

∣∣∣∣∣∣∣∣∣∣∣

W11 − E 1 W12 W13 · · · W1n

W21 W22 − E 1 W23 · · · W2n

W31 W32 W33 − E 1 · · · W3n...

......

. . ....

Wn1 Wn2 Wn3 · · · Wnn − E 1

∣∣∣∣∣∣∣∣∣∣∣= 0

giving an nth order equation in E 1

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 5 / 14

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Example 6.2

Consider the three-dimensional infinite cubical well

V 0(x , y , z) =

{0, 0 < x , y , z < a

∞, otherwise

The stationary states are

ψ0nxnynz (x , y , z) =

(2

a

)3/2

sin(nxπ

ax)

sin(nyπ

ay)

sin(nzπ

az)

where nx , ny , and nz are positive integers. The corresponding allowedenergies are

E 0nxnynz =

π2~2

2ma2(n2x + n2y + n2z)

The first excited state is triply degenerate

ψa ≡ ψ112, ψb ≡ ψ121, ψc ≡ ψ211, E 01 ≡ 3

π2~2

ma2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 6 / 14

Page 43: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Consider the three-dimensional infinite cubical well

V 0(x , y , z) =

{0, 0 < x , y , z < a

∞, otherwise

The stationary states are

ψ0nxnynz (x , y , z) =

(2

a

)3/2

sin(nxπ

ax)

sin(nyπ

ay)

sin(nzπ

az)

where nx , ny , and nz are positive integers.

The corresponding allowedenergies are

E 0nxnynz =

π2~2

2ma2(n2x + n2y + n2z)

The first excited state is triply degenerate

ψa ≡ ψ112, ψb ≡ ψ121, ψc ≡ ψ211, E 01 ≡ 3

π2~2

ma2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 6 / 14

Page 44: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Consider the three-dimensional infinite cubical well

V 0(x , y , z) =

{0, 0 < x , y , z < a

∞, otherwise

The stationary states are

ψ0nxnynz (x , y , z) =

(2

a

)3/2

sin(nxπ

ax)

sin(nyπ

ay)

sin(nzπ

az)

where nx , ny , and nz are positive integers. The corresponding allowedenergies are

E 0nxnynz =

π2~2

2ma2(n2x + n2y + n2z)

The first excited state is triply degenerate

ψa ≡ ψ112, ψb ≡ ψ121, ψc ≡ ψ211, E 01 ≡ 3

π2~2

ma2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 6 / 14

Page 45: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Consider the three-dimensional infinite cubical well

V 0(x , y , z) =

{0, 0 < x , y , z < a

∞, otherwise

The stationary states are

ψ0nxnynz (x , y , z) =

(2

a

)3/2

sin(nxπ

ax)

sin(nyπ

ay)

sin(nzπ

az)

where nx , ny , and nz are positive integers. The corresponding allowedenergies are

E 0nxnynz =

π2~2

2ma2(n2x + n2y + n2z)

The first excited state is triply degenerate

ψa ≡ ψ112, ψb ≡ ψ121, ψc ≡ ψ211, E 01 ≡ 3

π2~2

ma2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 6 / 14

Page 46: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

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Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 48: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

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Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

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Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

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Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 52: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 53: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2

[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 54: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 55: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 56: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2

(a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 57: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)

=V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 58: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Suppose we apply a perturbation

H ′ =

{V0, 0 < x < a/2 and 0 < y < a/2

0, otherwise

We need to calculate the matrix elements of the the 3× 3, W -matrix

Waa =⟨ψ112|H ′|ψ112

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(πay)dy

∫ a

0sin2

(2π

az

)dz

=

(2

a

)3

V0

{[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

}2[z

2− a

8πsin

(4π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)2 (a2

)=

V0

4

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 7 / 14

Page 59: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 60: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 61: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 62: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 63: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 64: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 65: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 66: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

)

(a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 67: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

)

(a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 68: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)

=V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 69: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4

= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 70: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 71: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 72: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 73: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

∫ a

0sin

(2π

az

)sin(πaz)dz

]

= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 74: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The next diagonal element is slightly different

Wbb =⟨ψ121|H ′|ψ121

⟩=

(2

a

)3

V0

∫ a/2

0sin2

(πax)dx

∫ a/2

0sin2

(2π

ay

)dy

∫ a

0sin2

(πaz)dz

=

(2

a

)3

V0

[x

2− a

4πsin

(2π

ax

)∣∣∣∣a/20

[y

2− a

8πsin

(4π

ay

)∣∣∣∣a/20

×[z

2− a

4πsin

(2π

az

)∣∣∣∣a0

=

(2

a

)3

V0

(a4

) (a4

) (a2

)=

V0

4= Wcc

now compute the off-diagonal elements of the matrix

Wab =⟨ψ112|H ′|ψ121

⟩=

(2

a

)3V0

[∫ a/2

0sin2

(πax)dx

×∫ a/2

0sin(πay)

sin

(2π

ay

)dy

�������������∫ a

0sin

(2π

az

)sin(πaz)dz

]= 0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 8 / 14

Page 75: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)

2

∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 76: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)

2

∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 77: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)

2

∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 78: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)

2

∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 79: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)

( aπ

)

2

∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 80: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)

( aπ

)2∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 81: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)2∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 82: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)2∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2

=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 83: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)2∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 84: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)2∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2

=V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 85: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)2∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2

=V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 86: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The same integrals hold for Wac , thus Wab = Wac = 0, and all thatremains is Wbc

Wbc =⟨ψ121|H ′|ψ211

⟩=

(2

a

)3V0

[∫ a/2

0sin(πax)

sin

(2π

ax

)dx

×∫ a/2

0sin

(2π

ay

)sin(πay)dy

∫ a

0sin2

(πaz)dz

]

=

(2

a

)3V0

(a2

)( aπ

)2∫ π/2

0sin(θ) sin(2θ) dθ

∫ π/2

0sin(2φ) sin(φ) dφ

=

(4V0

π2

){∫ π/2

02 sin2(θ) cos(θ) dθ

}2=

(4V0

π2

){2

[sin3(θ)

3

∣∣∣∣π/20

}2

=16V0

9π2=

V0

4· 64

9π2=

V0

4κ κ ≡

(8

)2≈ 0.7205

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 9 / 14

Page 87: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 88: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

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Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 90: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣

= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 91: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 92: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 93: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 94: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 95: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

The W -matrix thus becomes

the matrix can be diagonalizedin the usual way

the solutions are:

w3 = 1 + κ ≈ 1.7205,

w1 = 1,

w2 = 1− κ ≈ 0.2795

E1(λ) =

E 01 + λ(1 + κ)V0/4

E 01 + λV0/4

E 01 + λ(1− κ)V0/4

W =V0

4

1 0 00 1 κ0 κ 1

0 = det

∣∣∣∣∣∣1− w 0 0

0 1− w κ0 κ 1− w

∣∣∣∣∣∣= (1− w)[(1− w)2 − κ2]

= (1− w)(1− w − κ)(1− w + κ)

λ1

E1

κ

V

4

0

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 10 / 14

Page 96: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 97: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 98: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 99: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 100: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 101: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 102: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 103: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 104: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 105: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 106: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 107: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 108: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Example 6.2

Now we can determine the“good” linear combinations

ψ0 = αψ112 + βψ121 + γψ211

expanding into three equations

when w = 1 the only solution isα = 1, β = γ = 0

the other two eigenvalues give asolution where α = 0 and β =±γ

the three “good” states arethus

what operator would fullfill thetheorem?

1 0 00 1 κ0 κ 1

αβγ

= w

αβγ

wα = α

wβ = β + κγ

wγ = κβ + γ

ψ0 =

1√2

(ψ121 + ψ211)

ψ112

1√2

(ψ121 − ψ211)

PxyQz f (x , y , z) = f (y , x , a− z)

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 11 / 14

Page 109: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 110: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp

≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 111: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 112: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 113: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 114: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 115: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 116: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 117: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 118: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 119: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Hydrogen fine structure

The Hamiltonian that can besolved exactly for the hydrogenatom is merely an approxima-tion. The first is the correctionfor the motion of the proton.

The other important correctionscan be scaled according to thefine structure constant:

The largest correction is the finestructure and this consists oftwo terms: the relativistic cor-rection and the spin-orbit cor-rection.

me → µ =memp

me + mp≈ 1836

1837me ≈ me

α =e2

4πε0~c' 1

137.04

Some of the relevant energy scales are:

Bohr energy: α2mc2

Fine structure: α4mc2

Lamb shift: α5mc2

Hyperfine splitting: (m/mp)α4mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 12 / 14

Page 120: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 121: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2

=p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 122: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m

= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 123: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m

= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 124: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 125: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 126: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 127: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 128: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 129: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv

=mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 130: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 131: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4

= γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 132: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4

= γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 133: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 134: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])

= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 135: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 136: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2

−→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 137: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

Relativistic correction

The first term in the Hamiltonianrepresents the kinetic energy

if we substitute p = (~/i)∇, thefamiliar operator form emerges

this is not good enough for relativis-tic electrons, instead we must sub-tract the rest energy from the totalenergy

and the relativistic momentum

T =1

2mv2 =

p2

2m= − ~2

2m∇2

T = γmc2 −mc2

=mc2√

1− (v/c)2−mc2

p = γmv =mv√

1− (v/c)2

p2c2 + m2c4 = γ2m2v2c2 + m2c4 = γ2m2v2c2 + γ2m2c41

γ2

= γ2(m2v2c2 + m2c4

[1− (v/c)2

])= γ2m2c4

=(T + mc2

)2 −→ T =√p2c2 + m2c4 −mc2

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 13 / 14

Page 138: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc

so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[

1 +1

2

( p

mc

)2− 1

8

( p

mc

)4· · ·

− 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 139: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[

1 +1

2

( p

mc

)2− 1

8

( p

mc

)4· · ·

− 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 140: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]

= mc2[

1 +1

2

( p

mc

)2− 1

8

( p

mc

)4· · ·

− 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 141: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[

1 +1

2

( p

mc

)2− 1

8

( p

mc

)4· · ·

− 1

]

=p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 142: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1

+1

2

( p

mc

)2− 1

8

( p

mc

)4· · ·

− 1

]

=p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 143: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2

− 1

8

( p

mc

)4· · ·

− 1

]

=p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 144: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]

=p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 145: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 146: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 147: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 148: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 149: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 150: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩

C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14

Page 151: Today’s Outline - January 20, 2016csrri.iit.edu/~segre/phys406/16S/lecture_03.pdfToday’s Outline - January 20, 2016 Multiple degenerate states Fine structure Relativistic correction

First order relativistic correction

This expression must reduce to theclassical value when p � mc so ex-panding in powers of (p/mc)

T =√p2c2 + m2c4 −mc2

T = mc2

[√1 +

( p

mc

)2− 1

]= mc2

[1 +

1

2

( p

mc

)2− 1

8

( p

mc

)4· · · − 1

]=

p2

2m− p4

8m3c2+ · · ·

The second term is the first orderrelativistic correction

and the correction to the energy isthus

H ′r = − p4

8m3c2

E(1)r =

⟨H ′r

⟩= − 1

8m3c2〈ψ| p4ψ

⟩= − 1

8m3c2⟨p2ψ

∣∣ p2ψ⟩C. Segre (IIT) PHYS 406 - Spring 2016 January 20, 2016 14 / 14