Star Formation in the Multiverse

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dc.creatorBousso, Raphael
dc.creatorLeichenauer, Stefan
dc.date2008-10-17
dc.date.accessioned2026-07-07T13:13:20Z
dc.date.available2026-07-07T13:13:20Z
dc.descriptionWe develop a simple semi-analytic model of the star formation rate (SFR) as a function of time. We estimate the SFR for a wide range of values of the cosmological constant, spatial curvature, and primordial density contrast. Our model can predict such parameters in the multiverse, if the underlying theory landscape and the cosmological measure are known.
dc.description26 pages, 11 figures. For Mathematica notebook, go to http://panic.berkeley.edu/~sleichen/ComputeSFR.nb
dc.identifierhttps://arxiv.org/abs/0810.3044
dc.identifierhttp://arxiv.org/abs/0810.3044
dc.identifierPhys.Rev.D79:063506,2009
dc.identifierdoi:10.1103/PhysRevD.79.063506
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229858
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleStar Formation in the Multiverse
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