Some Comments on the Theory of Bose Condensation, with particular reference to the Interiors of Stars

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dc.creatorDunning-Davies, J.
dc.date2004-05-26
dc.date.accessioned2026-07-07T05:51:56Z
dc.date.available2026-07-07T05:51:56Z
dc.descriptionThe possibility of the phenomenon of Bose condensation having a part to play in the discussion of neutron stars has been around for some time. Here the sorts of temperatures and densities that might be involved are discussed. Also, an alternative way of viewing the Bose condensation phenomenon is examined once more and, although found to lead to more accurate results in traditional examples, is found to have little numerical effect in astrophysical examples.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/physics/0405139
dc.identifierhttp://arxiv.org/abs/physics/0405139
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/86166
dc.subjectGeneral Physics
dc.titleSome Comments on the Theory of Bose Condensation, with particular reference to the Interiors of Stars
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