ar X iv : a st ro - p h / 97 04 25 4 v 1 2 5 A pr 1 99 7 Upper limit to Ω B in scalar - tensor gravity theories
نویسنده
چکیده
In a previous paper (Serna & Alimi 1996b), we have pointed out the existence of some particular scalar-tensor gravity theories able to relax the nucleosynthesis constraint on the cosmic baryonic density. In this paper, we present an exhaustive study of primordial nucleosynthesis in the framework of such theories taking into account the currently adopted observational constraints. We show that a wide class of them allows for a baryonic density very close to that needed for the universe closure. This class of theories converges soon enough towards General Relativity and, hence, is compatible with all solar-system and binary pulsar gravitational tests. In other words, we show that primordial nucleosynthesis does not always impose a very stringent bound on the baryon contribution to the density parameter. Subject headings: cosmology:early universe, cosmology:dark matter, cosmology: theory UPPER LIMIT TO ΩB IN SCALAR-TENSOR GRAVITY THEORIES 3
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تاریخ انتشار 1997