Sphaleron

Since a sphaleron may convert baryons to antileptons and antibaryons to leptons and thus change the baryon number, if the density of sphalerons was at some stage high enough, they could wipe out any net excess of baryons or anti-baryons. This has two important implications in any theory of baryogenesis within the Standard Model:[4][5]

• Any baryon net excess arising before the electroweak symmetry breaking would be wiped out due to abundant sphalerons caused by high temperatures existing in the early universe.
• While a baryon net excess can be created during the electroweak symmetry breaking, it can be preserved only if this phase transition was first-order. This is because in a second-order phase transition, sphalerons would wipe out any baryon asymmetry as it is created, while in a first-order phase transition, sphalerons would wipe out baryon asymmetry only in the unbroken phase.

In absence of processes which violate B − L it is possible for an initial baryon asymmetry to be protected if it has a non-zero projection onto B − L. In this case the sphaleron processes would impose an equilibrium which distributes the initial B asymmetry between both B and L numbers.[6] In some theories of baryogenesis, an imbalance of the number of leptons and antileptons is formed first by leptogenesis and sphaleron transitions then convert this to an imbalance in the numbers of baryons and antibaryons.

For an SU(2) gauge theory, neglecting ${\displaystyle \theta _{W}}$, we have the following equations for the gauge field and the Higgs field in the gauge ${\displaystyle A_{0}=A_{r}=0}$ [7]

${\displaystyle \mathbf {A} =\nu \,{\frac {\,f(\xi )\,}{\xi }}~{\hat {\mathbf {r} }}\times \mathbf {\sigma } \,,\qquad \phi ={\frac {\nu }{\,{\sqrt {2\,}}\,}}~h(\xi )~{\hat {\mathbf {r} }}\cdot \mathbf {\sigma } ~\phi _{0}}$

where ${\displaystyle ~\xi =r\,g\,\nu ~}$, ${\displaystyle ~\phi _{0}={\begin{bmatrix}1\\0\end{bmatrix}}~}$, the symbols ${\displaystyle ~\sigma }$ represent the generators of SU(2), ${\displaystyle ~g~}$ is the electroweak coupling constant, and ${\displaystyle ~\nu ~}$ is the Higgs VEV absolute value. The functions ${\displaystyle ~h(\xi )~}$ and ${\displaystyle ~f(\xi )~}$, which must be determined numerically, go from 0 to 1 in value as their argument, ${\displaystyle ~\xi ~}$, goes from 0 to ${\displaystyle \infty }$.

For a sphaleron in the background of a non-broken phase, the Higgs field must obviously fall off eventually to zero as ${\displaystyle ~\xi ~}$ goes to infinity.

Note that in the limit ${\displaystyle \xi \rightarrow \infty }$, the gauge sector approaches one of the pure-gauge transformation ${\displaystyle {\frac {~\mathbf {r} \cdot \mathbf {\sigma } ~}{r}}}$, which is the same as the pure gauge transformation to which the BPST instanton approaches as ${\displaystyle r\rightarrow \infty }$ at ${\displaystyle t=0}$, hence establishing the connection between the sphaleron and the instanton.

Baryon number violation is caused by the "winding" of the fields from one equilibrium to another. Each time the weak gauge fields wind, the count for each of the quark families and each of the lepton families is raised (or lowered, depending on the winding direction) by one; as there are three quark families, baryon number can only change in multiples of three.[8] The baryon number violation can alternatively be visualized in terms of a kind of Dirac sea: in the course of the winding, a baryon originally considered to be part of the vacuum is now considered a real baryon, or vice versa, and all the other baryons stacked inside the sea are accordingly shifted by one energy level.[9]

According to physicist Max Tegmark, the theoretical energy efficiency from conversion of baryons to antileptons would be orders of magnitude higher than the energy efficiency of existing power-generation technology such as nuclear fusion. Tegmark speculates that an extremely advanced civilization might use a "sphalerizer" to generate energy from ordinary baryonic matter.[10]

• Chiral anomaly
• Instanton
• Theta vacuum