1989
DOI: 10.1103/physrevd.40.588
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Free energy of the sphaleron in the Weinberg-Salam model

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Cited by 43 publications
(39 citation statements)
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“…The zero-mode factors and (the naive version of) ω − were evaluated in Refs. [29,30], while κ was determined numerically in Refs. [31,32].…”
Section: Chern-simons Diffusion Ratementioning
confidence: 99%
“…The zero-mode factors and (the naive version of) ω − were evaluated in Refs. [29,30], while κ was determined numerically in Refs. [31,32].…”
Section: Chern-simons Diffusion Ratementioning
confidence: 99%
“…The sphaleron field configuration was first discretised, and then allowed to evolve under the classical Euler-Lagrange field equations with an imposed condition of spherical symmetry [45][46][47]. The restriction to spherical symmetry is permissible because the sole decay channel of the Klinkhamer-Manton sphaleron is spherically symmetric [48]; it should be noted, however, that this approach may be used only in the limit of vanishing weak mixing angle θ W . As a consequence of the imposed spherical symmetry, it is expected that equal numbers of W + , W − and Z 0 of any given polarisation state will be produced after the decay.…”
Section: Sphaleron Decaymentioning
confidence: 99%
“…Here, we consider only the sector of spherically symmetric fluctuations, where the instabilities of the zerotemperature sphaleron are known to reside as well as the unstable breathing mode of the bubble. The fluctuations $ and $G decouple in the quadratic form from the fluctuations X , qH, and $K [15], yielding a system of two equations (two channel) and a system of three equations (three channel), respectively:…”
Section: Normal Modesmentioning
confidence: 99%