Supernova Neutrino Light Curves from Proto-Neutron Star Cooling with Various Nuclear Equation of State

We present the model spectra of neutrinos emitted from proto-neutron star (PNS) cooling used in Nakazato et al., Astrophys. J. <strong>925</strong> (2022) 98, arXiv:2108.03009 [astro-ph.HE]. So as to obtain the time evolution of neutrino spectra, PNS cooling simulations are performed with use of four nuclear equation of state (EOS) models and eight PNS cooling models with different initial conditions are involved for each EOS. The format of the spectral data is the same with that of Supernova Neutrino Database. For the details, see readme.pdf本数据集提供了Nakazato 等在《天体物理学杂志》（Astrophys. J.）925卷（2022年）第98页、预印本arXiv:2108.03009 [astro-ph.HE] 中使用的原中子星（proto-neutron star, PNS）冷却过程所产生的中微子能谱模型。为获取中微子能谱的时间演化规律，本研究开展了基于4种核物态方程（nuclear equation of state, EOS）模型的原中子星冷却模拟，且针对每种物态方程模型，均纳入了8种具备不同初始条件的原中子星冷却模型。该能谱数据的格式与超新星中微子数据库（Supernova Neutrino Database）完全一致，详细细节请参阅readme.pdf文件。