Bose-Einstein condensation as symmetry breaking in compact curved spacetimes

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dc.creatorSmith, John D.
dc.creatorToms, David J.
dc.date1996-02-09
dc.date.accessioned2026-07-07T10:34:16Z
dc.date.available2026-07-07T10:34:16Z
dc.descriptionWe examine Bose-Einstein condensation as a form of symmetry breaking in the specific model of the Einstein static universe. We show that symmetry breaking never occursin the sense that the chemical potential $μ$ never reaches its critical value.This leads us to some statements about spaces of finite volume in general. In an appendix we clarify the relationship between the standard statistical mechanical approaches and the field theory method using zeta functions.
dc.descriptionRevtex, 25 pages, 3 figures, uses EPSF.sty. To be published in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/hep-th/9602046
dc.identifierhttp://arxiv.org/abs/hep-th/9602046
dc.identifierPhys.Rev.D53:5771-5780,1996
dc.identifierdoi:10.1103/PhysRevD.53.5771
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179420
dc.subjectHigh Energy Physics - Theory
dc.titleBose-Einstein condensation as symmetry breaking in compact curved spacetimes
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