2005
DOI: 10.1142/s0217732305018104
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Simple Cosmological Model With Relativistic Gas

Abstract: We construct simple and useful approximation for the relativistic gas of massive particles. The equation of state is given by an elementary function and admits analytic solution of the Friedmann equation, including more complex cases when the relativistic gas of massive particles is considered together with radiation or with dominating cosmological constant. The model of relativistic gas may be interesting for the description of primordial Universe, especially as a candidate for the role of a Dark Matter.

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Cited by 34 publications
(95 citation statements)
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“…We generalized a previously constructed, simplified RRGbased cosmological model [6,8,9], made of WDM, a cosmological constant, baryons and photons by taking into account an out-of-equilibrium interaction within the baryon-photon fluid. Such interaction, characterized here by a single phenomenological parameter ξ , is supposed to be relevant before decoupling when the scattering rate ceases to be much higher than the Hubble rate and deviations from equilibrium are expected.…”
Section: Discussionmentioning
confidence: 99%
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“…We generalized a previously constructed, simplified RRGbased cosmological model [6,8,9], made of WDM, a cosmological constant, baryons and photons by taking into account an out-of-equilibrium interaction within the baryon-photon fluid. Such interaction, characterized here by a single phenomenological parameter ξ , is supposed to be relevant before decoupling when the scattering rate ceases to be much higher than the Hubble rate and deviations from equilibrium are expected.…”
Section: Discussionmentioning
confidence: 99%
“…The new aspect of the present work is the interaction which we introduced phenomenologically in Eqs. (5) and (6). It is easy to see that Eq.…”
Section: Basic Equations Of the Interacting Rrg Modelmentioning
confidence: 93%
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