Big Bang Nucleosynthesis Constraints on the Self-Gravity of Pressure

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dc.creatorRappaport, Saul
dc.creatorSchwab, Josiah
dc.creatorBurles, Scott
dc.creatorSteigman, Gary
dc.date2007-10-28
dc.date.accessioned2026-07-07T11:12:42Z
dc.date.available2026-07-07T11:12:42Z
dc.descriptionUsing big bang nucleosynthesis and present, high-precision measurements of light element abundances, we constrain the self-gravity of radiation pressure in the early universe. The self-gravity of pressure is strictly non-Newtonian, and thus the constraints we set provide a direct test of this prediction of general relativity and of the standard, Robertson-Walker-Friedmann cosmology.
dc.description5 pages, 1 figure. This paper was developed from an earlier version which was posted as arXiv:0707.3589
dc.identifierhttps://arxiv.org/abs/0710.5300
dc.identifierhttp://arxiv.org/abs/0710.5300
dc.identifierPhys.Rev.D77:023515,2008
dc.identifierdoi:10.1103/PhysRevD.77.023515
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191470
dc.subjectAstrophysics
dc.titleBig Bang Nucleosynthesis Constraints on the Self-Gravity of Pressure
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