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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2022
License: CC BY
Data sources: ZENODO
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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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Claim

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

Research datakeyboard_double_arrow_right Dataset 31 Jan 2022Publisher:Zenodo
Authors: NAKAZATO, Ken'ichiro; Collaboration, The NuLC;

doi: 10.5281/zenodo.5778224 , 10.5281/zenodo.5778223

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

Abstract

We present the model spectra of neutrinos emitted from proto-neutron star (PNS) cooling used in Nakazato et al., Astrophys. J. 925 (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

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supernova neutrinos

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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