today’s outline - november 05, 2012 - iitphys.iit.edu/~segre/phys405/12f/lecture_20.pdf · 2012....
TRANSCRIPT
Today’s Outline - November 05, 2012
• Problem 4.52
• Electrons in a magnetic field
• Adding angular momentum
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 1 / 10
Today’s Outline - November 05, 2012
• Problem 4.52
• Electrons in a magnetic field
• Adding angular momentum
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 1 / 10
Today’s Outline - November 05, 2012
• Problem 4.52
• Electrons in a magnetic field
• Adding angular momentum
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 1 / 10
Today’s Outline - November 05, 2012
• Problem 4.52
• Electrons in a magnetic field
• Adding angular momentum
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 1 / 10
Problem 4.52
Find the matrix representing Sx for a particle of spin 3/2 (using, as always,the basis of eigenstates of Sz . Solve the characteristic equation todetermine the eigenvalues of Sx .
First we write down the eigenstates of Sz in the S = 3/2 system.
| 32
32〉 =
1000
| 32
12〉 =
0100
| 32
−12〉 =
0010
| 32
−32〉 =
0001
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 2 / 10
Problem 4.52
Find the matrix representing Sx for a particle of spin 3/2 (using, as always,the basis of eigenstates of Sz . Solve the characteristic equation todetermine the eigenvalues of Sx .
First we write down the eigenstates of Sz in the S = 3/2 system.
| 32
32〉 =
1000
| 32
12〉 =
0100
| 32
−12〉 =
0010
| 32
−32〉 =
0001
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 2 / 10
Problem 4.52
Find the matrix representing Sx for a particle of spin 3/2 (using, as always,the basis of eigenstates of Sz . Solve the characteristic equation todetermine the eigenvalues of Sx .
First we write down the eigenstates of Sz in the S = 3/2 system.
| 32
32〉 =
1000
| 32
12〉 =
0100
| 32
−12〉 =
0010
| 32
−32〉 =
0001
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 2 / 10
Problem 4.52
Find the matrix representing Sx for a particle of spin 3/2 (using, as always,the basis of eigenstates of Sz . Solve the characteristic equation todetermine the eigenvalues of Sx .
First we write down the eigenstates of Sz in the S = 3/2 system.
| 32
32〉 =
1000
| 32
12〉 =
0100
| 32
−12〉 =
0010
| 32
−32〉 =
0001
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 2 / 10
Problem 4.52
Find the matrix representing Sx for a particle of spin 3/2 (using, as always,the basis of eigenstates of Sz . Solve the characteristic equation todetermine the eigenvalues of Sx .
First we write down the eigenstates of Sz in the S = 3/2 system.
| 32
32〉 =
1000
| 32
12〉 =
0100
| 32
−12〉 =
0010
| 32
−32〉 =
0001
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 2 / 10
Problem 4.52
Find the matrix representing Sx for a particle of spin 3/2 (using, as always,the basis of eigenstates of Sz . Solve the characteristic equation todetermine the eigenvalues of Sx .
First we write down the eigenstates of Sz in the S = 3/2 system.
| 32
32〉 =
1000
| 32
12〉 =
0100
| 32
−12〉 =
0010
| 32
−32〉 =
0001
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 2 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0 00 0 2 0
0 0 0√
30 0 0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0 00 0 2 0
0 0 0√
30 0 0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0 00 0 2 0
0 0 0√
30 0 0 0
S+| 32 32〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0 00 0 2 0
0 0 0√
30 0 0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0
√3 0 0
0
0 2 0
0
0 0√
3
0
0 0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0
√3 0 0
0
0 2 0
0
0 0√
3
0
0 0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉
=√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0
√3 0 0
0
0 2 0
0
0 0√
3
0
0 0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3
0 0
0 0
2 0
0 0
0√
3
0 0
0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3
0 0
0 0
2 0
0 0
0√
3
0 0
0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉
= 2~ | 32
12〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3
0 0
0 0
2 0
0 0
0√
3
0 0
0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0
0
0 0 2
0
0 0 0
√3
0 0 0
0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0
0
0 0 2
0
0 0 0
√3
0 0 0
0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉
=√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0
0
0 0 2
0
0 0 0
√3
0 0 0
0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
The raising and lowering operators are
S±|sm〉 = ~√
s(s + 1)−m(m ± 1) |s(m ± 1)〉
we build the matrix for S+ by applying the raising operator to each of theeigenstates
S+ = ~
0√
3 0 00 0 2 0
0 0 0√
30 0 0 0
S+| 32 3
2〉 = 0
S+| 32 12〉 =
√32( 5
2)− 12( 3
2)~ | 32 32〉 =√
3~ | 32
32〉
S+| 32 −12〉 =
√32( 5
2)+ 12( 1
2)~ | 32 12〉 = 2~ | 3
212〉
S+| 32 −32〉 =
√32( 5
2)+ 32(− 1
2)~ | 32 −12〉 =√
3~ | 32
−12〉
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 3 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0 0 0√3 0 0 0
0 2 0 0
0 0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0 0 0√3 0 0 0
0 2 0 0
0 0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0 0 0√3 0 0 0
0 2 0 0
0 0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉
=√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0 0 0√3 0 0 0
0 2 0 0
0 0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0
0 0 0
√3
0 0 0
0
2 0 0
0
0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0
0 0 0
√3
0 0 0
0
2 0 0
0
0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉
= 2~ | 32
−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0
0 0 0
√3
0 0 0
0
2 0 0
0
0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0
0 0
√3 0
0 0
0 2
0 0
0 0
√3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0
0 0
√3 0
0 0
0 2
0 0
0 0
√3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉
=√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0
0 0
√3 0
0 0
0 2
0 0
0 0
√3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0 0
0
√3 0 0
0
0 2 0
0
0 0√
3
0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0 0
0
√3 0 0
0
0 2 0
0
0 0√
3
0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Similarly, we build the matrix for S− by applying the lowering operator toeach of the eigenstates
S− = ~
0 0 0 0√3 0 0 0
0 2 0 0
0 0√
3 0
S−| 32 32〉 =
√32( 5
2)− 32( 1
2)~ | 32 12〉 =√
3~ | 32
12〉
S−| 32 12〉 =
√32( 5
2)− 12(− 1
2)~ | 32 −12〉 = 2~ | 3
2−12〉
S−| 32 −12〉 =
√32( 5
2)+ 12(− 3
2)~ | 32 −32〉 =√
3~ | 32
−32〉
S−| 32 −32〉 = 0
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 4 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−)
=~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣− λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣− λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣− λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣− λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣
= −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣− λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣
−√
3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣
= −λ[−λ(λ2 − 3)− 2(−2λ)]−√
3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9]
= λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9
= (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1)
= (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Problem 4.52 (cont.)
Sx =1
2(S+ + S−) =
~2
0√
3 0 0√3 0 2 0
0 2 0√
3
0 0√
3 0
The characteristic equation for eigenvalues is
0 =
∣∣∣∣∣∣∣∣−λ
√3 0 0√
3 −λ 2 0
0 2 −λ√
3
0 0√
3 −λ
∣∣∣∣∣∣∣∣ = −λ
∣∣∣∣∣∣−λ 2 0
2 −λ√
3
0√
3 −λ
∣∣∣∣∣∣−√3
∣∣∣∣∣∣√
3 2 0
0 −λ√
3
0√
3 −λ
∣∣∣∣∣∣= −λ[−λ(λ2 − 3)− 2(−2λ)]−
√3[√
3(λ2 − 3)]
= −λ[−λ3 + 7λ]− [3λ2 − 9] = λ4 − 10λ2 + 9
0 = λ4 − 10λ2 + 9 = (λ2 − 9)(λ2 − 1) = (λ+ 3)(λ− 3)(λ+ 1)(λ− 1)
the eigenvalues of Sx are : 32~, 1
2~,− 1
2~,− 3
2~
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 5 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Electron in a magnetic field
Orbital angular momentum implies a circulating charge which leads to amagnetic moment
because spin behaves in all ways like orbital angular momentum, it mustalso be associated with a magnetic dipole moment
~µ = γ~S
in the presence of a magnetic field,the dipole feels a torque
and has total energy
the Hamiltonian for a particle withspin in the presence of a magneticfield, is thus
γ is the gyromagnetic ratio
~τ = ~µ× ~B
H = −~µ · ~B
H = −γ~B · ~S
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 6 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz
= −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
)
{χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
)
{χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation
can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation
can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~
=
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Dipole at rest in a magnetic field
consider a particle of spin 1/2 atrest in the presence of a magneticfield in the z-direction
the Hamiltonian is
and its eigenstates are those of Szwith eigenvalues E±
the time dependent Schrodingerequation can be solved in terms ofthe stationary states
~B = B0z
H = −γB0Sz = −γB0~2
(1 00 −1
){χ+, E+ = −γB0~
2
χ−, E− = +γB0~2
i~∂χ
∂t= Hχ
χ(t) = aχ+e−E+t/~ + bχ−e
−E−t/~ =
(ae iγB0t/2
be−iγB0t/2
)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 7 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)
a = cos(α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)
a = cos(α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)
the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)
=~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)
=~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)
=~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
Time-dependent expectation value
The constants a and b can be de-termined from the initial conditions
giving |a|2 + |b|2 = 1 and suggest-ing the relationship
the time-dependent solution is thus
χ(0) =
(ab
)a = cos(
α
2), b = sin(
α
2)
χ(t) =
(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)the expectation value of S as a function of time can now be calculated
〈Sx〉 = χ†(t)Sxχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 11 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(sin(α2 )e−iγB0t/2
cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(e−iγB0t + e iγB0t
)=
~2
sinα cos(γB0t)
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 8 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)
=~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)
=~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)
= −~2
sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)
=~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)
=~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)
=~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
More expectation values
〈Sy 〉 = χ†(t)Syχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(0 −ii 0
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)(−i sin(α2 )e−iγB0t/2
i cos(α2 )e iγB0t/2
)=
~2
cos(α/2) sin(α/2)(−ie−iγB0t + ie iγB0t
)= −~
2sinα sin(γB0t)
〈Sz〉 = χ†(t)Szχ(t)
=(
cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2) ~
2
(1 00 −1
)(cos(α2 )e iγB0t/2
sin(α2 )e−iγB0t/2
)=
~2
(cos(α2 )e−iγB0t/2 sin(α2 )e+iγB0t/2
)( cos(α2 )e iγB0t/2
− sin(α2 )e−iγB0t/2
)=
~2
(cos2(α/2)− sin2(α/2)
)=
~2
cosα
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 9 / 10
Larmor precession
The expectation values for the compo-nents of S are thus
〈Sx〉 =~2
sinα cos(γB0t)
〈Sy 〉 = −~2
sinα sin(γB0t)
〈Sz〉 =~2
cosα
S precesses about the z-axis, at a fixedangle α so 〈Sz〉 is constant and the othertwo are constantly changing
the precession frequency ω = γB0 iscalled the Larmor frequency
z
y
x
S
ω
α
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 10 / 10
Larmor precession
The expectation values for the compo-nents of S are thus
〈Sx〉 =~2
sinα cos(γB0t)
〈Sy 〉 = −~2
sinα sin(γB0t)
〈Sz〉 =~2
cosα
S precesses about the z-axis, at a fixedangle α so 〈Sz〉 is constant and the othertwo are constantly changing
the precession frequency ω = γB0 iscalled the Larmor frequency
z
y
x
S
ω
α
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 10 / 10
Larmor precession
The expectation values for the compo-nents of S are thus
〈Sx〉 =~2
sinα cos(γB0t)
〈Sy 〉 = −~2
sinα sin(γB0t)
〈Sz〉 =~2
cosα
S precesses about the z-axis, at a fixedangle α so 〈Sz〉 is constant and the othertwo are constantly changing
the precession frequency ω = γB0 iscalled the Larmor frequency
z
y
x
S
ω
α
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 10 / 10
Larmor precession
The expectation values for the compo-nents of S are thus
〈Sx〉 =~2
sinα cos(γB0t)
〈Sy 〉 = −~2
sinα sin(γB0t)
〈Sz〉 =~2
cosα
S precesses about the z-axis, at a fixedangle α so 〈Sz〉 is constant and the othertwo are constantly changing
the precession frequency ω = γB0 iscalled the Larmor frequency
z
y
x
S
ω
α
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 10 / 10
Larmor precession
The expectation values for the compo-nents of S are thus
〈Sx〉 =~2
sinα cos(γB0t)
〈Sy 〉 = −~2
sinα sin(γB0t)
〈Sz〉 =~2
cosα
S precesses about the z-axis, at a fixedangle α so 〈Sz〉 is constant and the othertwo are constantly changing
the precession frequency ω = γB0 iscalled the Larmor frequency
z
y
x
S
ω
α
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 10 / 10
Larmor precession
The expectation values for the compo-nents of S are thus
〈Sx〉 =~2
sinα cos(γB0t)
〈Sy 〉 = −~2
sinα sin(γB0t)
〈Sz〉 =~2
cosα
S precesses about the z-axis, at a fixedangle α so 〈Sz〉 is constant and the othertwo are constantly changing
the precession frequency ω = γB0 iscalled the Larmor frequency
z
y
x
S
ω
α
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 10 / 10
Larmor precession
The expectation values for the compo-nents of S are thus
〈Sx〉 =~2
sinα cos(γB0t)
〈Sy 〉 = −~2
sinα sin(γB0t)
〈Sz〉 =~2
cosα
S precesses about the z-axis, at a fixedangle α so 〈Sz〉 is constant and the othertwo are constantly changing
the precession frequency ω = γB0 iscalled the Larmor frequency
z
y
x
S
ω
α
C. Segre (IIT) PHYS 405 - Fall 2012 November 05, 2012 10 / 10