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The Concordance Cosmic Star Formation Rate: Implications from and for the Supernova Neutrino and Gamma Ray Backgrounds

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, no. 4 (2005): 017-017

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supernova neutrinosneutrino and gamma astronomycosmological neutrinosstar formation

Abstract

We constrain the cosmic star formation rate (CSFR) by requiring that massive stars produce the observed UV, optical, and IR light and at the same time not overproduce the diffuse supernova neutrino background as bounded by Super-Kamiokande. With the massive star component so constrained we then show that a reasonable choice of stellar ini...More

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