The Physics Travel Guide

bohr magneton

Prerequisites: Spin. Full path (19 pages)

Intuitive

The Bohr magneton is the natural unit expressing the magnetic moment of the electron. Electrons have a magnetic moment because they have a property called spin (a sort of intrinsic angular momentum) and because they sometimes go in circles.

Concrete

The Bohr magneton is defined as

μB=eℏ2me≈9.274×10−24 J T−1≈5.788×10−5 eV T−1(SI),\mu_B = \frac{e\hbar}{2m_e} \approx 9.274\times 10^{-24}\ \mathrm{J\,T^{-1}} \approx 5.788\times 10^{-5}\ \mathrm{eV\,T^{-1}} \qquad \text{(SI)},

with e>0e > 0 the elementary charge and mem_e the electron mass. In Gaussian units it reads μB=eℏ/(2mec)\mu_B = e\hbar/(2m_ec).

Where it comes from. A charge qq of mass mm moving on a circle of radius rr with speed vv is a current loop with current I=qv/(2πr)I = qv/(2\pi r) and area πr2\pi r^2. Its magnetic moment is

μ=I⋅πr2=qvr2=q2m L,\mu = I\cdot \pi r^2 = \frac{q v r}{2} = \frac{q}{2m}\,L,

where L=mvrL = mvr is the angular momentum. The ratio q/2mq/2m between magnetic moment and angular momentum is the classical gyromagnetic ratio. In quantum mechanics orbital angular momentum comes in units of ℏ\hbar, so for an electron the natural size of the magnetic moment is eℏ/2me=μBe\hbar/2m_e = \mu_B. For orbital motion, taking into account the negative charge,

μ⃗L=−e2meL⃗=−μB L⃗ℏ.\vec\mu_L = -\frac{e}{2m_e}\vec L = -\mu_B\,\frac{\vec L}{\hbar} .

Spin magnetic moment. The electron spin S⃗\vec S also carries a magnetic moment,

μ⃗S=−gs μB S⃗ℏ,gs≈2.0023.\vec\mu_S = -g_s\,\mu_B\,\frac{\vec S}{\hbar}, \qquad g_s \approx 2.0023 .

The value gs=2g_s = 2 follows from the Dirac equation. The small deviation is the anomalous magnetic moment, ae=(gs−2)/2≈α/2π≈0.00116a_e = (g_s - 2)/2 \approx \alpha/2\pi \approx 0.00116 at leading order in quantum electrodynamics. Since Sz=±ℏ/2S_z = \pm\hbar/2, the spin magnetic moment along a field axis is close to ∓μB\mp\mu_B, which is why the electron's magnetic moment is often quoted as about one Bohr magneton.

Zeeman effect. In a magnetic field B⃗=Bz^\vec B = B\hat z the energy of a magnetic moment is E=−μ⃗⋅B⃗E = -\vec\mu\cdot\vec B. Ignoring spin, an atomic level with magnetic quantum number mlm_l shifts by

ΔE=μB B ml,\Delta E = \mu_B\, B\, m_l ,

so a field of 1 T1\ \mathrm{T} splits neighbouring levels by about 5.8×10−5 eV5.8\times 10^{-5}\ \mathrm{eV}.

For nuclei the corresponding unit is the nuclear magneton μN=eℏ/(2mp)\mu_N = e\hbar/(2m_p), smaller than μB\mu_B by the mass ratio me/mp≈1/1836m_e/m_p \approx 1/1836.

Abstract

From the Dirac equation. The factor gs=2g_s = 2 appears in the nonrelativistic limit of the Dirac equation. For a particle of charge qq in an electromagnetic field, with kinetic momentum π⃗=p⃗−qA⃗\vec\pi = \vec p - q\vec A and p⃗=−iℏ∇\vec p = -i\hbar\nabla, the leading term is the Pauli equation Hamiltonian (σ⃗⋅π⃗)2/2m+qϕ(\vec\sigma\cdot\vec\pi)^2/2m + q\phi. Using (σ⃗⋅a⃗)(σ⃗⋅b⃗)=a⃗⋅b⃗+iσ⃗⋅(a⃗×b⃗)(\vec\sigma\cdot\vec a)(\vec\sigma\cdot\vec b) = \vec a\cdot\vec b + i\vec\sigma\cdot(\vec a\times\vec b) and π⃗×π⃗=iqℏB⃗\vec\pi\times\vec\pi = iq\hbar\vec B,

(σ⃗⋅π⃗)22m=π⃗ 22m−qℏ2m σ⃗⋅B⃗.\frac{(\vec\sigma\cdot\vec\pi)^2}{2m} = \frac{\vec\pi^{\,2}}{2m} - \frac{q\hbar}{2m}\,\vec\sigma\cdot\vec B .

For the electron, q=−eq = -e, the last term is +μB σ⃗⋅B⃗=−μ⃗S⋅B⃗+\mu_B\,\vec\sigma\cdot\vec B = -\vec\mu_S\cdot\vec B with μ⃗S=−2μBS⃗/ℏ\vec\mu_S = -2\mu_B\vec S/\hbar and S⃗=ℏσ⃗/2\vec S = \hbar\vec\sigma/2, which is gs=2g_s = 2. The same expansion of π⃗ 2\vec\pi^{\,2} to first order in a uniform field gives the orbital term μBL⃗⋅B⃗/ℏ\mu_B\vec L\cdot\vec B/\hbar with gL=1g_L = 1.

Form factors. In quantum field theory the coupling of a spin-12\frac12 particle to the electromagnetic field is described by the vertex function. For on-shell particles, current conservation and Lorentz invariance restrict it to two form factors. With incoming momentum pp, outgoing momentum p′p' and q=p′−pq = p' - p (units ℏ=c=1\hbar = c = 1), the vertex is proportional to uˉ(p′)Γμu(p)\bar u(p')\Gamma^\mu u(p) with

Γμ=γμF1(q2)+iσμνqν2mF2(q2),σμν=i2[γμ,γν].\Gamma^\mu = \gamma^\mu F_1(q^2) + \frac{i\sigma^{\mu\nu}q_\nu}{2m}F_2(q^2), \qquad \sigma^{\mu\nu} = \frac{i}{2}[\gamma^\mu, \gamma^\nu] .

F1(0)=1F_1(0) = 1 fixes the charge, and the gyromagnetic factor is g=2(F1(0)+F2(0))=2+2F2(0)g = 2\big(F_1(0) + F_2(0)\big) = 2 + 2F_2(0). At one loop F2(0)=α/2πF_2(0) = \alpha/2\pi. The Bohr magneton is thus the scale set by the charge, mass and ℏ\hbar of the particle, and gg measures the coupling in these units. A term ψˉσμνψFμν\bar\psi\sigma^{\mu\nu}\psi F_{\mu\nu} (Pauli term) in an effective Lagrangian shifts gg away from 22; it has mass dimension 55, so it is not renormalizable and is not present in the QED Lagrangian, which is why g−2g - 2 is a calculable loop effect there.

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