The effect of core-collapse supernova accretion phase turbulence on neutrino flavor evolution
Author:
Funder
Nuclear Physics
Publisher
IOP Publishing
Subject
Nuclear and High Energy Physics
Link
http://iopscience.iop.org/article/10.1088/1361-6471/aa7bc8/pdf
Reference58 articles.
1. Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport
2. Simulation of the Spherically Symmetric Stellar Core Collapse, Bounce, and Postbounce Evolution of a Star of 13 Solar Masses with Boltzmann Neutrino Transport, and Its Implications for the Supernova Mechanism
3. Stability of Standing Accretion Shocks, with an Eye toward Core‐Collapse Supernovae
4. Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport
5. Non-spherical core collapse supernovae
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2. On probing turbulence in core-collapse supernovae in upcoming neutrino detectors;Journal of Cosmology and Astroparticle Physics;2024-03-01
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