2012
DOI: 10.1088/1751-8113/45/37/374009
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Thermal Yang–Mills theory in the Einstein universe

Abstract: We study the stability of a non-Abelian chromomagnetic vacuum in Yang-Mills theory in Euclidean Einstein universe S 1 × S 3 . We assume that the gauge group is a simple compact group G containing the group SU (2) as a subgroup and consider static covariantly constant gauge fields on S 3 taking values in the adjoint representation of the group G and forming a representation of the group SU (2). We compute the heat kernel for the Laplacian acting on fields on S 3 in an arbitrary representation of SU (2) and use … Show more

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Cited by 2 publications
(12 citation statements)
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“…The T 3 dependence is characteristic of the photon gas and, as has been found in our previous paper [12], of the gluon gas as well.…”
Section: Jhep11(2015)193supporting
confidence: 82%
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“…The T 3 dependence is characteristic of the photon gas and, as has been found in our previous paper [12], of the gluon gas as well.…”
Section: Jhep11(2015)193supporting
confidence: 82%
“…This heat trace can be computed by using the heat kernel diagonal for the Laplacian ∆ j on the unit sphere S 3 given by the eq. (6.16) of our paper [12]. To get the heat trace we have to multiply the heat kernel diagonal by the volume of the sphere S 3 equal to vol (S 3 ) = 2π 2 and by the dimension of the representation j equal to (2j + 1).…”
Section: Heat Trace For Irreducible Representationsmentioning
confidence: 99%
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