dc.creatorTorres, Diego F.
dc.creatorVucetich, Héctor
dc.date1998
dc.date2021-08-13T17:37:03Z
dc.date.accessioned2023-07-15T02:41:51Z
dc.date.available2023-07-15T02:41:51Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/122664
dc.identifierissn:0378-4371
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7462933
dc.descriptionWe study the primordial neutron to baryon ratio in a cosmological expanding background within the context of non-extensive statistics, in a fully analytical approach. First order corrections to the weak interaction rates and energy densities in the early universe are obtained and their consequences on the Helium synthesis are analyzed. We find that, if the nucleosynthesis scenario should be in agreement with observation, this entails a very restrictive bound upon q, the non-extensive parameter. We also study some cosmologically interesting situations such as the moment of pair annihilation, conserved comoving quantities and derive for the nonextensive statistics, temperature relationships, before and after the removal of pairs.
dc.descriptionFacultad de Ciencias Exactas
dc.formatapplication/pdf
dc.format397-414
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectFísica
dc.subjectPhysics
dc.subjectBaryon
dc.subjectMoment (physics)
dc.subjectAnnihilation
dc.subjectWeak interaction
dc.subjectCosmology
dc.subjectContext (language use)
dc.subjectTheoretical physics
dc.subjectNucleosynthesis
dc.subjectQuantum mechanics
dc.subjectUniverse
dc.titleCosmology in a non-standard statistical background
dc.typeArticulo
dc.typePreprint


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