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The Diffuse Supernova Neutrino Background

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arxiv 2001.07510 v1 pith:AXVHKOB3 submitted 2020-01-15 astro-ph.HE

Samalka Anandagoda , Dieter H. Hartmann , Marco Ajello , Abhishek Desai This is my paper · ORCID
classification astro-ph.HE
keywords dsnbsfrdfluxneutrinobackgrounddiffuseestimatedsupernova
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abstract

The Diffuse Supernova Neutrino Background (DSNB) in the MeV regime represents the cumulative cosmic neutrino emission, predominantly due to core collapse supernovae. We estimate the DSNB flux for different Star Formation Rate Density (SFRD) models. We find that the DSNB flux estimated using the SFRD derived from Fermi-LAT Collaboration et al. (2018) is significantly higher ($\approx$ 32$\%$) relative to the flux estimated using the SFRD from Madau & Fragos (2017). This depicts the sensitivity between the DSNB flux and the SFRD estimates which shows that future detection of the DSNB can be used as a valuable tool to constrain the SFRD.

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