Bohr–Van Leeuwen theorem explained

The Bohr–Van Leeuwen theorem states that when statistical mechanics and classical mechanics are applied consistently, the thermal average of the magnetization is always zero.[1] This makes magnetism in solids solely a quantum mechanical effect and means that classical physics cannot account for paramagnetism, diamagnetism and ferromagnetism. Inability of classical physics to explain triboelectricity also stems from the Bohr–Van Leeuwen theorem.[2]

History

What is today known as the Bohr–Van Leeuwen theorem was discovered by Niels Bohr in 1911 in his doctoral dissertation[3] and was later rediscovered by Hendrika Johanna van Leeuwen in her doctoral thesis in 1919.[4] In 1932, J. H. Van Vleck formalized and expanded upon Bohr's initial theorem in a book he wrote on electric and magnetic susceptibilities.[5]

The significance of this discovery is that classical physics does not allow for such things as paramagnetism, diamagnetism and ferromagnetism and thus quantum physics is needed to explain the magnetic events.[6] This result, "perhaps the most deflationary publication of all time,"[7] may have contributed to Bohr's development of a quasi-classical theory of the hydrogen atom in 1913.

Proof

An intuitive proof

The Bohr–Van Leeuwen theorem applies to an isolated system that cannot rotate. If the isolated system is allowed to rotate in response to an externally applied magnetic field, then this theorem does not apply.[8] If, in addition, there is only one state of thermal equilibrium in a given temperature and field, and the system is allowed time to return to equilibrium after a field is applied, then there will be no magnetization.

The probability that the system will be in a given state of motion is predicted by Maxwell–Boltzmann statistics to be proportional to

\exp(-U/kBT)

, where

U

is the energy of the system,

kB

is the Boltzmann constant, and

T

is the absolute temperature. This energy is equal to the sum of the kinetic energy (

mv2/2

for a particle with mass

m

and speed

v

) and the potential energy.[8]

q

and velocity

v

is

F=q\left(E+v x B\right),

where

E

is the electric field and

B

is the magnetic flux density. The rate of work done is

Fv=qEv

and does not depend on

B

. Therefore, the energy does not depend on the magnetic field, so the distribution of motions does not depend on the magnetic field.[8]

In zero field, there will be no net motion of charged particles because the system is not able to rotate. There will therefore be an average magnetic moment of zero. Since the distribution of motions does not depend on the magnetic field, the moment in thermal equilibrium remains zero in any magnetic field.[8]

A more formal proof

So as to lower the complexity of the proof, a system with

N

electrons will be used.

This is appropriate, since most of the magnetism in a solid is carried by electrons, and the proof is easily generalized to more than one type of charged particle.

Each electron has a negative charge

e

and mass

me

.

If its position is

r

and velocity is

v

, it produces a current

j=ev

and a magnetic moment[6]

\mu=

1
2c

r x j=

e
2c

r x v.

The above equation shows that the magnetic moment is a linear function of the velocity coordinates, so the total magnetic moment in a given direction must be a linear function of the form

\mu=

Na
\sum
ir

i,

where the dot represents a time derivative and

ai

are vector coefficients depending on the position coordinates

\{ri,i=1\ldotsN\}

.[6]

Maxwell–Boltzmann statistics gives the probability that the nth particle has momentum

pn

and coordinate

rn

as

dP\propto\exp{\left[-

l{H
(p

1,\ldots,pN;r1,\ldots,rN)}{kBT}\right]}dp1,\ldots,dpNdr1,\ldots,drN,

where

l{H}

is the Hamiltonian, the total energy of the system.[6]

The thermal average of any function

f(p1,\ldots,pN;r1,\ldots,rN)

of these generalized coordinates is then

\langlef\rangle=

\intfdP
\intdP

.

In the presence of a magnetic field,

l{H}=

1
2me
N
\sum
i=1

\left(pi-

e
c

Ai\right)2+e\phi(q),

where

Ai

is the magnetic vector potential and

\phi(q)

is the electric scalar potential. For each particle the components of the momentum

pi

and position

ri

are related by the equations of Hamiltonian mechanics:
\begin{align} p

i&=-\partiall{H}/\partial

r
i\\ r

i&=\partiall{H}/\partialpi. \end{align}

Therefore,
r

i\proptopi-

e
c

Ai,

so the moment

\mu

is a linear function of the momenta

pi

.[6]

The thermally averaged moment,

\langle\mu\rangle=

\int\mudP
\intdP

,

is the sum of terms proportional to integrals of the form
infty
\int
-infty

(pi-

e
c

Ai)dP,

where

p

represents one of the momentum coordinates.

The integrand is an odd function of

p

, so it vanishes.

Therefore,

\langle\mu\rangle=0

.[6]

Applications

The Bohr–Van Leeuwen theorem is useful in several applications including plasma physics: "All these references base their discussion of the Bohr–Van Leeuwen theorem on Niels Bohr's physical model, in which perfectly reflecting walls are necessary to provide the currents that cancel the net contribution from the interior of an element of plasma, and result in zero net diamagnetism for the plasma element."[9]

Diamagnetism of a purely classical nature occurs in plasmas but is a consequence of thermal disequilibrium, such as a gradient in plasma density. Electromechanics and electrical engineering also see practical benefit from the Bohr–Van Leeuwen theorem.

External links

Notes and References

  1. [John Hasbrouck van Vleck]
  2. Alicki. Robert. Jenkins. Alejandro. 2020-10-30. Quantum Theory of Triboelectricity. Physical Review Letters. en. 125. 18. 186101. 10.1103/PhysRevLett.125.186101. 33196235. 0031-9007. 1904.11997. 2020PhRvL.125r6101A. 10669/82347 . 139102854.
  3. Book: Bohr, Niehls . The Doctor's Dissertation (Text and Translation) . 1972 . originally published as "Studier over Metallernes Elektrontheori", Københavns Universitet (1911) . Early Works (1905-1911) . Rosenfeld . L. . Nielsen . J. Rud . . 1 . Niels Bohr Collected Works . 163, 165–393 . 10.1016/S1876-0503(08)70015-X . 978-0-7204-1801-9.
  4. Hendrika Johanna . Van Leeuwen . Problèmes de la théorie électronique du magnétisme . . 2 . 12 . 361–377 . 1921. 10.1051/jphysrad:01921002012036100 . 97259591 .
  5. Book: Van Vleck, J. H. . The theory of electric and magnetic susceptibilities . . 1932 . 0-19-851243-0.
  6. Book: Aharoni, Amikam . Amikam Aharoni . Introduction to the Theory of Ferromagnetism . . 1996 . 0-19-851791-2 . 6–7 .
  7. Book: Van Vleck, J. H. . John Hasbrouck Van Vleck . Quantum mechanics: The key to understanding magnetism (Nobel lecture, 8 December 1977) . Nobel Lectures in Physics 1971-1980 . Lundqvist . Stig . . 1992 . 981-02-0726-3.
  8. Book: Feynman . Richard P. . Richard Feynman . Robert B. . Leighton . Robert B. Leighton . Matthew . Sands . Matthew Sands . . 2 . 34-8 . 2006 . 978-0465024940.
  9. Web site: Plasma Stability and the Bohr–Van Leeuwen Theorem . Reece . Roth . 1967 . NASA . 2008-10-27.