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.

中文翻译：

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宇宙超新星遗迹中微子背景中的不确定性回顾

我们回顾了由于核心坍缩超新星、黑洞形成和中子星合并事件导致的残余中微子背景的当前理解的计算和相关的不确定性。我们考虑了由于核状态方程 (EoS)、前身质量、源超新星中微子光谱、宇宙恒星形成率、恒星初始质量函数、中微子振荡和中微子自相互作用而导致的不确定性的现状。我们总结了未来中微子探测器目前的可行性，以通过探测到的超新星中微子光谱来区分核 EoS 和超新星中微子的温度。