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Page 1: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Luigi Paolasini [email protected]

Page 2: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Lecture 1 14 JANUARY 2014: “Why spins spin?”

Lecture 2 28 JANUARY 2014: “Lonely atoms”

Lecture 3 11 FEBRUARY 2014: “Local perturbations”

Lecture 4 25 FEBRUARY 2014: “Magnetic interactions”

Lecture 5 11 MARCH 2014: “Magnetic structures”

Lecture 6 25 MARCH 2014: “Magnetic excitations”

Lecture 7 8 APRIL 2014: “The dark side of magnetism: magnetic metals”

Lecture 8 22 APRIL 2014: “Neutron magnetic scattering”

Lecture 9 6 MAY 2014: “X-ray magnetic scattering”

Lecture 10 27 MAY 2014: “Other x-ray techniques for magnetism

Page 3: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

LECTURE 1: “WHY SPINS SPIN?”

Historical view. Classical and quantum mechanics. Self-rotating electron model. Spin algebra and coupling of two spins.

Reference books:

-  Stephen Blundell: “Magnetism in Condensed Matter”, Oxford Master series in Condensed Matter Physics.

-  Sin-itiro Tomonaga: “The story of spin”, University of Chicago press.

Page 4: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Magnetism from the beginning

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Page 5: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

The magnetic moment

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

The fundamental object in Magnetism is the elementary magnetic moment dμ (or magnetic dipole), which can be defined in classical electromagnetism as:

“ an electric current I circulating in a vanishingly small and oriented loop dS”

dS

The magnetic moment μassociated to a finite loop size is obtained by integrating the infinitesimal current loops.

NOTICE: the currents in the infinitesimal adiacent loops cancel each other, leaving only the periferical current I.

Page 6: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

The angular momentum

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

The magnetic moments are generated by rotating charged particles (such as the atomic electrons). The angular momentum L is due to the rotation of these massive particles, and is always connected with the magnetic moment: !

γ = gyromagnetic ratio

EINSTEIN-de HAAS-Effect (1915) Ampère's conjecture in 1820: ”Magnetism is caused by circulation of electric charges” A suspended ferromagnetic rod rotates when a magnetic field is applied. This is due to the conservation of angular momentum and the rotation is opposite to the magnetization direction.

Page 7: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Definition of Bohr Magneton μB Hydrogen atom:

- electron charge -e - mass me - circular orbit at distance r

Electron current: I = −e/ τ Orbital period: τ = 2π r/v Angular momentum of electron: L = mevr = !

Angular momentum is oppositely direct with respect to the magnetic dipole moment because the negative electron charge.

Because µ=γ L =γ ! => γ = -e/2me and ωL= eB/2me

(= )

Page 8: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Magnetic moment precession

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

The energy of a magnetic dipole in a static magnetic field is

A torque act perpendicularly to µ and B

Equation of motion:

The moment µ precess around the magnetic field with constant modulus |µ| at Larmor’s precession frequency

and is equal to the rate of change of L, G = dL/dt

… like a spinning top or a gyroscope!

Page 9: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Magnetization and magnetic field

“Macroscopic” magnetization M= µ/v: magnetic moment per unit volume

Magnetic vector fields B or H (B is called also magnetic induction)

B is measured in Tesla, H in A/m

In the free space (vacuum): M=0 B= µ0 H where µ0= 4π 10-7 Hm-1 is the vacuum permeability

In the solids: M≠0 B= µ0 (H + M) B could different from H in direction and magnitude.

In the linear materials: M= χ H where χ is the magnetic susceptibility

B= µ0 (1+χ)H = µ0µr H where µr= (1+χ) is the relative permeability

Page 10: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Magnetization of a system of electrons

Magnetization of a system of electrons: magnetic moment per unit volume that is induced by a magnetic field B is proportional to the rate of change of energy of the system.

The classical mechanics cannot explain the existence of magnetic materials!!

.

Bohr-van Leeuwen theorem: “In a classical system there is no thermal equilibrium magnetization”

Lorentz force F=-e v x B: The magnetic field produces forces perpendicular to the particle velocity. No work is done!

As a consequence, the energy of the system does not depends on the applied magnetic field B

The magnetization must be zero in a classical system!

Page 11: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Quantum mechanics

and quantum numbers

Page 12: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Hydrogen spectrum

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

1913 Niels Bohr: “Theory for the spectrum of hydrogen atom, based on quantum theory that energy is transferred only in certain well defined quantities”

N. Bohr

n = principal quantum number (integral positive) size of electron orbit

k = subordinate quantum number (integral positive) shape of the orbit (S, P, D … for k=1,2,3 …) denotes also the orbital angular momentum (unit ħ)

m = magnetic quantum number (integral) components of the angular momentum vector k along the magnetic field (Zeeman split)

PS: k and m introduced by Sommerfield in 1916

Rules: “space quantization of angular momentum”

n ≥ k

-k ≤ m ≤k (2k+1 values)

!

k-1

k+1

" k

!

m-1

m+1

" # m m

Page 13: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

R=multiplicity/2

Inner quantum numbers

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

A. Landé W. Pauli A. Sommerfeld

To classify the variety of the levels in a multiplet term Sommerfeld introduced in 1920 the inner quantum number j. Now m specify the sublevels which are split for a level defined by n,k,j by a magnetic field, and -j ≤ m ≤j

“Find the origin of the spectral multiplicity in the Zeeman effect”

!

k-1

k+1

" k

!

j-1

j+1

" # j j

!

m-1

m+1

" # m m

Because experimentally transitions occur only between the terms with the same multiplicity of differing by 2, Landé introduced a supplementary quantum number R:

R=1/2 singlets R=1 doublets R=3/2 triplets

Page 14: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Spectral terms of alkali atoms

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

E (cm-1)

Na

Sodium have two closely spaced levels

Doublets: multiplicity=2

Inner quantum numbers for alkali doublet terms

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Spectral terms of alkaline earths

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Singlets: multiplicity=1

Triplets: multiplicity=3

Mg

Page 16: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Lande, Sommerfeld and Pauli Ersatzmodell

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

“A radiant electron moves in an electric field created by the core electrons and the atomic nucleus. In general, the core electrons are not spherical symmetric but have an angular momentum, which originates an internal Zeeman splitting. ”

Landé Ersatzmodell: The core is have an orbital momentum R and then a magnetic moment µR=-g0R. The total angular momentum of the system is J=K+R, where K=-µK is the angular momentum of radiant electron associated to it :

K=k-1/2 |R-K|+1/2 ≤ J≤ |R+K|-1/2 -J+1/2 ≤ m ≤ J-1/2

Sommerfeld Ersatzmodell: The core angular momentum is j0=(multiplicity-1)/2 and the total angular momentum j=ja+j0, where ja=k-1:

ja=k-1 (=l) |j0-ja|≤ j≤ |j0+ja| -j ≤ m ≤ j

Pauli Ersatzmodell: The core angular momentum is r=(multiplicity+1)/2 and the total angular momentum JP=r+k, where ja=k-1:

k=k |k-r|+1≤JP≤ |k+r|-1 -JP+1 ≤ m ≤ JP-1

Page 17: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Model limitations.

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

The Landé model succeeded in deriving the rule for the multiplet splitting, confirming a large amounth of experimental results … apart for very light atoms like He and Li!!

ΔWmag= cost. . (J-1/2)

Another inconsistency was found in the calculation of the values of ΔWmag in alkali doublets using the core-electron magnetic forces.

The idea that the origin of the multiplicity is not due to the electron core but the electron itself became to appears in 1924. Pauli says: “The very fact that the two electrons in He have to play entirely different roles –one for electron core and the other the radiant electron- is the failure of the model”. “The doublet structure of alkalis spectra and the breakdown of Larmor theorem is caused by the strange two-valuedness of quantum-theoretical properties of the radiant electron which cannot be described classically.”

Splitting ratio in triplet terms

Page 18: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

Self rotating electron model

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

R. Kronig Uhnlenbeck and Goudsmith

Proposed originally by R. Kronig in 1925 but never published! “An electron rotating about its own axis and with an angular momentum of self-rotation of ½ and a g-factor g0=2”

The interaction between the magnetic moments generated by the self-rotation and the orbital motion could be derived through relativity … … and then calculate the interval between the multiplet terms.

Because g0=2, these demonstration fail completely by a factor 2 and Pauli strongly reject this theory! Problems arise also for the necessity to have a fast rotation of the electron to have an orbital moment of ½ (surface speed 10 time c!). … 6 months later Uhnlenbeck and Goudsmith publish in Naturwissenschaften this “wrong” theory.

Landé empirical expression Kronig model and relativistic calculation

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L. Paolasini - LECTURES ON MAGNETISM- LECT.1

The Thomas ½ factor

Llewellyn H. Thomas

1926: Thomas introduce a correction to the spin-orbit interaction which take into account the relativistic “time dilatation” between electron and nucleus of an atom.

The electron rest frame is not inertial, but is accelerated, and it rotates with respect to the laboratory system. As a result, the Larmor precession of µe of the electron in the magnetic field generate by its relativistic motion is not the same as seem in the laboratory system.

When this correction is taken into account, the calculation of level intervals became in accord with experiment and given by:

… this expression is half of that calculated by the Kronig and Uhnlenbeck/Goudsmith

Page 20: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

1926: a special year for quantum theories

Heisenberg Matrix mechanics

Schrödinger Wave mechanics

Dirac Transformation theory

Pauli Spin theory

?

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L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Pauli spin theory

Definition of the spin angular momentum S

Pauli decided to use the component sz= ±½ as running variable for the spin degree of freedom and not the canonical momentum conjugate φ associated to the azimuthal rotation.

Electron wavefunction Probability density to find the electron at x with spin up

Probability density to find the electron at x with spin down

… we need to write the Hamiltonian H which involve the external H1 and the internal H2 magnetic fields

Page 22: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Operators

Schrödinger operators:

… and than the orbital angular momentum operators l

momentum

position

=> =>

Which spin operator? Pauli take the similarities with the angular momentum matrices (mx, my, mz) used in matrix mechanics:

Commutation relations

Eigenvalues

Page 23: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Pauli matrices

Pauli propose to use the matrices (sx, sy, sz) direcly in the Schrödinger equation:

Pauli matrices

Properties:

This correspond to considering the spin state vector as a column vector described by the two component wavefunction ψ(x,sz):

=>

Page 24: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Limitation of Pauli equation

1)  The Pauli equation contains the non-relativistic Hamiltonian H0, and so is non-relativistic! As a result cannot be used to calculate the doublet terms and the anomalous Zeeman effect!

2)  Pauli introduces arbitrarily the spin ½ and g0=2 in the H1, and also the Thomas factor (g0-1) in H2, and judge his theory a tentative.

3)  The choice of Pauli algebra have an enormous implication in the coupling of two spin:

Theorem. “When there are two particles of spin ½, the wave function for which the sum of two spins equal 1 does not change its value when the spin variable of the electrons are exchanged (symmetric). The wave function for which the sum of the two spin becomes 0 change sign when the spin variables are interchanged (antisymmetric)”

Page 25: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Two electron states I

Let we consider two electrons with spin matrices:

The square of the magnitude of the total spin |s1+s2|2 is:

and because:

=>

Let we assume that the wave function describing the two spin states is a column vector (we omit the variables coordinate x1 and x2) and we

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L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Two electron states II

Then we obtain: … because:

and:

and

… because:

Page 27: Luigi Paolasini paolasini@esrf lecture1.pdfL. Paolasini - LECTURES ON MAGNETISM- LECT.1 A. Sommerfeld A. Landé W. Pauli To classify the variety of the levels in a multiplet term Sommerfeld

L. Paolasini - LECTURES ON MAGNETISM- LECT.1

Two electron states III

TOTAL SPIN 1

TOTAL SPIN 0

=>

=> Symmetric wave function

=>

=> Anti-Symmetric wave function