Impact of late-time neutrino emission on the diffuse supernova neutrino background

Ekanger, Nick; Horiuchi, Shunsaku; Kotake, Kei; Sumiyoshi, Kohsuke

doi:10.1103/physrevd.106.043026

Title: Impact of late-time neutrino emission on the diffuse supernova neutrino background

Journal Article · 26 August 2022 · Physical Review. D.

DOI: https://doi.org/10.1103/physrevd.106.043026 · OSTI ID:1980166

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Virginia Polytechnic Institute and State University (Virginia Tech), Blacksburg, VA (United States); OSTI
Virginia Polytechnic Institute and State University (Virginia Tech), Blacksburg, VA (United States); University of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)
Fukuoka University (Japan)
Numazu College of Technology (Japan)

In the absence of high-statistics supernova neutrino measurements, estimates of the diffuse supernova neutrino background (DSNB) hinge on the precision of simulations of core-collapse supernovae. Understanding the cooling phase of protoneutron star (PNS) evolution (≳ 1 s after core bounce) is crucial, since approximately 50% of the energy liberated by neutrinos is emitted during the cooling phase. We model the cooling phase with a hybrid method by combining the neutrino emission predicted by 3D hydrodynamic simulations with several cooling-phase estimates, including a novel two-parameter correlation depending on the final baryonic PNS mass and the time of shock revival. We find that the predicted DSNB event rate at Super-Kamiokande can vary by a factor of ~2–3 depending on the cooling-phase treatment. Here we also find that except for one cooling estimate, the range in predicted DSNB events is largely driven by the uncertainty in the neutrino mean energy. With a good understanding of the late-time neutrino emission, more precise DSNB estimates can be made for the next generation of DSNB searches.

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Research Organization:: Virginia Polytechnic Institute and State University (Virginia Tech), Blacksburg, VA (United States)

Sponsoring Organization:: Japan Society for the Promotion of Science (JSPS); Ministry of Education, Science and Culture of Japan (MEXT); National Science Foundation (NSF); USDOE Office of Science (SC)

Grant/Contract Number:: SC0020262

OSTI ID:: 1980166

Journal Information:: Physical Review. D., Journal Name: Physical Review. D. Journal Issue: 4 Vol. 106; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Title: Impact of late-time neutrino emission on the diffuse supernova neutrino background

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