The Physics Travel Guide

Sphalerons

Prerequisites: Instantons, Standard Model of Particle Physics. Full path (38 pages)

Why is it interesting?

Sphalerons are an important part of several proposed solutions of the Baryon asymmetry problem such as Leptogenesis.

Intuitive

The electroweak theory has infinitely many classical lowest-energy states. They all have the same energy and differ in how the gauge field is "wound up" in space, which is counted by an integer. Neighbouring vacua are separated by an energy barrier. A picture is a ball rolling in a long row of identical valleys separated by hills of equal height.

There are two ways to get from one valley to the next. At zero temperature the system can only tunnel through the hill. This is the process described by instantons, and in the electroweak theory it is so strongly suppressed that it has never been observed and plays no practical role today. At high temperature, as in the early universe, thermal fluctuations can instead carry the system over the top of the hill. The field configuration at the top of the hill, at the lowest pass between two valleys, is the sphaleron. It is a static solution of the field equations, but an unstable one: a small push sends it down into one valley or the other. The name comes from a Greek word meaning "ready to fall". Its energy is of order 10 TeV.

The reason sphalerons matter is that moving from one valley to the next changes the number of baryons and leptons. Because of a quantum anomaly, each step creates or destroys three baryons and three leptons together (one of each per generation), while the difference between baryon and lepton number stays fixed. In the hot early universe these transitions were frequent, so they can convert a lepton asymmetry into a baryon asymmetry, which is the mechanism behind leptogenesis, or wash out an asymmetry created earlier.

Concrete

A sphaleron is a maximum of the energy functional in the direction of changing winding number, and a minimum in the orthogonal direction. Thus it is a saddle point. (page 336 in An introduction to gauge theories and modern particle physics by E. Leader and E. Predazzi.)

Abstract

Consider the bosonic part of the electroweak theory, or for simplicity the SU(2)SU(2) gauge theory with a Higgs doublet (g′=0g' = 0). In the temporal gauge W0=0W_0 = 0, finite energy requires the Higgs field at spatial infinity to lie in the vacuum manifold {Φ†Φ=v2/2}≅S3\{\Phi^\dagger\Phi = v^2/2\} \cong S^3, and the classical vacua are pure gauge configurations Wi=−ig(∂iU)U−1W_i = -\frac{i}{g}(\partial_i U)U^{-1} (with Wi=Wiaτa/2W_i = W_i^a \tau^a/2 and Dμ=∂μ−igWμD_\mu = \partial_\mu - i g W_\mu), Φ=U (0,v/2)T\Phi = U\,(0, v/\sqrt2)^T with U:R3∪{∞}≅S3→SU(2)U:\mathbb{R}^3\cup\{\infty\} \cong S^3 \to SU(2). These are classified by π3(SU(2))=Z\pi_3(SU(2)) = \mathbb{Z}, and the integer is the Chern-Simons number NCSN_{CS} of the vacuum. For a general static configuration NCSN_{CS} is a real number, and a path from one vacuum to the next changes it by one.

The fermion number currents are anomalous. With NfN_f generations,

∂μjBμ=∂μjLμ=Nf32π2(g2 WμνaW~a μν−g′2 BμνB~μν),W~a μν=12ϵμνρσWρσa,\partial_\mu j^\mu_B = \partial_\mu j^\mu_L = \frac{N_f}{32\pi^2}\left( g^2\, W^a_{\mu\nu}\widetilde{W}^{a\,\mu\nu} - g'^2\, B_{\mu\nu}\widetilde{B}^{\mu\nu} \right), \qquad \widetilde{W}^{a\,\mu\nu} = \tfrac12\epsilon^{\mu\nu\rho\sigma}W^a_{\rho\sigma},

(with the overall sign fixed by the convention for ϵ0123\epsilon^{0123}), so B−LB - L is conserved and a transition between vacua whose Chern-Simons numbers differ by ΔNCS\Delta N_{CS} changes BB and LL by Nf ΔNCSN_f\,\Delta N_{CS} each ('t Hooft). The BB~B\widetilde{B} term is also a total derivative, but the abelian hypercharge field has no topologically distinct vacua, and its contribution vanishes for transitions between vacua.

Manton showed that the configuration space of the SU(2)SU(2)-Higgs theory contains non-contractible loops of field configurations that begin and end at the vacuum. Along each such loop the energy has a maximum, and minimizing this maximum over all loops in the class (a minimax procedure) yields a static saddle point of the energy functional. This is the sphaleron of Klinkhamer and Manton. It has NCS=12N_{CS} = \frac12, exactly one unstable direction (along the path between neighbouring vacua) and energy

Esph=4πvg f ⁣(λ/g2),E_{\text{sph}} = \frac{4\pi v}{g}\, f\!\left(\lambda/g^2\right),

where λ\lambda is the Higgs quartic coupling and ff is a slowly varying function of order 2 (between about 1.5 and 2.7 over the full range of λ/g2\lambda/g^2). With v≈246v \approx 246 GeV this is of order 10 TeV.

Because the sphaleron is a saddle point with one negative mode, it sets the rate of thermal transitions. At zero temperature, tunnelling between vacua is suppressed by e−16π2/g2=e−4π/αWe^{-16\pi^2/g^2} = e^{-4\pi/\alpha_W}. In the Higgs phase at temperature TT below the electroweak crossover, the rate per unit volume is proportional to e−Esph(T)/Te^{-E_{\text{sph}}(T)/T}, with the temperature-dependent sphaleron energy computed with v(T)v(T). In the symmetric phase there is no barrier set by vv, and the rate per volume scales as αW5T4\alpha_W^5 T^4 up to logarithms and a numerical constant obtained from lattice simulations. This makes baryon and lepton number violation fast in the early universe above the electroweak scale and negligible today.

Path to this page

  1. Calculus
  2. Imaginary Numbers
  3. Linear Algebra
  4. Functional
  5. Group Theory
  6. Hilbert Space
  7. Legendre Transformation
  8. Manifold
  9. Newton's Second Law
  10. Product Spaces
  11. Vector Calculus
  12. Coulomb's law
  13. Fiber Bundles
  14. Newtonian Mechanics
  15. Symmetry
  16. Topology
  17. Variational Calculus
  18. Configuration Space
  19. Euler-Lagrange Equations
  20. Maxwell Equations
  21. Special Relativity
  22. Lagrangian Formalism
  23. Phase Space
  24. Classical Field Theory
  25. Gauge Symmetry
  26. Hamiltonian Formalism
  27. Symmetry Breaking
  28. Gauge Models
  29. Goldstone's theorem
  30. Schrödinger Equation
  31. Canonical Quantum Mechanics
  32. Higgs Mechanism
  33. Canonical Quantum Field Theory
  34. Path Integral Quantum Mechanics
  35. Non-Perturbative QFT
  36. Standard Model of Particle Physics
  37. Wick Rotation
  38. Instantons