When do supernova neutrinos of different flavors have similar luminosities but different spectra?-Reference-Cited by-同舟云学术

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When do supernova neutrinos of different flavors have similar luminosities but different spectra?

Published:1995-08 Issue:4 Volume:3 Page:377-383
ISSN:0927-6505
Container-title:Astroparticle Physics
language:en
Short-container-title:Astroparticle Physics

Author:

Janka H.-Thomas

Publisher

Elsevier BV

Subject

Astronomy and Astrophysics

Reference20 articles.

1. Neutrinos from gravitational collapse

2. Supernovae;Mayle,1990

3. The Nuclear Equation of State, Part A;Wilson,1989

4. Neutrinos from SN1987A and current models of stellar-core collapse

5. Nuclear Physics in the Universe;Bruenn,1993

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1. Comparison of the Core-collapse Evolution of Two Nearly Equal-mass Progenitors;The Astrophysical Journal;2023-04-01

2. Equation of state of hot dense hyperonic matter in the Quark–Meson-Coupling (QMC-A) model;Monthly Notices of the Royal Astronomical Society;2021-01-04

3. Fast neutrino flavor conversion, ejecta properties, and nucleosynthesis in newly-formed hypermassive remnants of neutron-star mergers;Physical Review D;2020-11-12

4. Impact of nucleon-nucleon bremsstrahlung rates beyond one-pion exchange;Physical Review D;2016-10-28

5. Effects of density-dependent lepton fraction on the properties of protoneutron stars;Physical Review C;2013-06-10

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