Relaxation versus collision times in the cosmological radiative era

Diego Pavón, Roberte A. Sussman

Producción científica: Contribución a una revistaArtículoInvestigaciónrevisión exhaustiva

8 Citas (Scopus)

Resumen

We consider the Lemaître - Tolman - Bondi metric with an inhomogeneous viscous fluid source satisfying the equation of state of an interactive mixture of radiation and matter. Assuming conditions prior to the decoupling era, we apply extended irreversible thermodynamics (EIT) to this mixture. Using the full transport equation of EIT we show that the relaxation time of shear viscosity can be several orders of magnitude larger than the Thomson collision time between photons and electrons. A comparison with the 'truncated' transport equation for these models reveals that the latter cannot properly describe the decoupling of matter and radiation.
Idioma originalInglés
Páginas (desde-hasta)1625-1636
PublicaciónClassical and Quantum Gravity
Volumen18
DOI
EstadoPublicada - 7 may 2001

Huella

Profundice en los temas de investigación de 'Relaxation versus collision times in the cosmological radiative era'. En conjunto forman una huella única.

Citar esto