Entropy Bounds in Spherical Space

dc.creatorBrevik, Iver
dc.creatorMilton, Kimball A.
dc.creatorOdintsov, Sergei D.
dc.date2002-10-29
dc.date.accessioned2026-07-07T04:14:24Z
dc.date.available2026-07-07T04:14:24Z
dc.descriptionExact calculations are given for the Casimir energy for various fields in $R\times S^3$ geometry. The Green's function method naturally gives a result in a form convenient in the high-temperature limit, while the statistical mechanical approach gives a form appropriate for low temperatures. The equivalence of these two representations is demonstrated. Some discrepancies with previous work are noted. In no case, even for ${\cal N}=4$ SUSY, is the ratio of entropy to energy found to be bounded.
dc.description9 pages, no figures, requires sc3conf.sty
dc.identifierhttps://arxiv.org/abs/hep-th/0210286
dc.identifierhttp://arxiv.org/abs/hep-th/0210286
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51612
dc.subjectHigh Energy Physics - Theory
dc.titleEntropy Bounds in Spherical Space
dc.typetext

Files

Collections