Evolution of primordial H2 for different cosmological models

Simple item page
dc.creatorPuy, Denis
dc.date1999-11-15
dc.date.accessioned2026-07-07T02:34:26Z
dc.date.available2026-07-07T02:34:26Z
dc.descriptionPrimordial chemistry began in the recombination epoch when the adiabatic expansion caused the temperature of the radiation to fall below 4000 K. The chemistry of the early Universe involves the elements hydrogen, its isotope deuterium, helium with its isotopic forms and lithium. In this communication I will present results on the evolution of the primordial $H_2$ abundance for different cosmological models and the influence on the thermal decoupling.
dc.descriptionTalk given at the International Conference "H2 in space" IAP-Paris (France), September 28th, October 1st, 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9911267
dc.identifierhttp://arxiv.org/abs/astro-ph/9911267
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15242
dc.subjectAstrophysics
dc.titleEvolution of primordial H2 for different cosmological models
dc.typetext

Files

Collections

arXiv