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Parastatistics and the equation of state for the early Universe

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dc.contributor.authorAldrovandi, R.
dc.contributor.authorMonte Lima, I.
dc.contributor.institutionInstituto de Física Teórica
dc.date.accessioned2022-04-29T08:42:50Z
dc.date.available2022-04-29T08:42:50Z
dc.date.issued1983-02-01
dc.description.abstractThe equation of state for an ideal mixture of relativistic quantum gases obeying any (para-)statistics is given. Recursion formulae are obtained for the distribution function and correlations are analysed. The equation of state can be applied to the early Universe, allowing the quarks to be treated either as coloured fermions or (unequivalently) as parafermions of order 3. In the latter case, they exhibit a tendency of aggregate into triads by a mere statistical effect. © 1983 D. Reidel Publishing Co.en
dc.description.affiliationInstituto de Física Teórica, São Paulo
dc.format.extent179-195
dc.identifierhttp://dx.doi.org/10.1007/BF00651559
dc.identifier.citationAstrophysics and Space Science, v. 90, n. 1, p. 179-195, 1983.
dc.identifier.dimensionspub.1053242113
dc.identifier.doi10.1007/BF00651559
dc.identifier.issn0004-640X
dc.identifier.issn1572-946X
dc.identifier.scopus2-s2.0-0040902599
dc.identifier.urihttp://hdl.handle.net/11449/230944
dc.language.isoeng
dc.publisherSpringer Nature
dc.relation.ispartofAstrophysics and Space Science
dc.rights.accessRightsAcesso abertopt
dc.rights.sourceRightsoa_all
dc.rights.sourceRightsgreen
dc.sourceScopus
dc.sourceDimensions
dc.titleParastatistics and the equation of state for the early Universeen
dc.typeArtigopt
dspace.entity.typePublication
relation.isOrgUnitOfPublication41d94a5b-139b-457c-90a7-77b71f4e94df
relation.isOrgUnitOfPublication.latestForDiscovery41d94a5b-139b-457c-90a7-77b71f4e94df
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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