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Parastatistics and the equation of state for the early Universe

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.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.relation.ispartofAstrophysics and Space Science
dc.sourceScopus
dc.titleParastatistics and the equation of state for the early Universeen
dc.typeArtigo
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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