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      New Insights into Uncertainties in the Relic Neutrino Background and Effects from the Nuclear Equation of State

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          Abstract

          We review the computation of and associated uncertainties in the current understanding of the relic neutrino background due to core-collapse supernovae, black hole formation and neutron-star merger events. We consider the current status of uncertainties due to the nuclear equation of state (EoS), the progenitor masses, the source supernova neutrino spectrum, the cosmological star formation rate, the stellar initial mass function, neutrino oscillations, and neutrino self-interactions. We summarize the current viability of future neutrino detectors to distinguish the nuclear EoS and the temperature of supernova neutrinos via the detected relic supernova neutrino spectrum.

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          COUNTING LOW-MASS STARS IN INTEGRATED LIGHT

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            Supernova Reverse Shocks: SiC Growth and Isotopic Composition

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              Author and article information

              Journal
              19 July 2019
              Article
              1907.10088
              c51b249b-d66b-4b88-88b4-0733e3591f75

              http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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              Custom metadata
              19 pages, 9 figures, submitted to IJMPA. arXiv admin note: text overlap with arXiv:1405.0458
              astro-ph.HE

              High energy astrophysical phenomena
              High energy astrophysical phenomena

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