Multi-dimensional solution of fast neutrino conversions in binary neutron star merger remnants

DOI10.1088/1475-7516/2021/01/017zbMath1484.85021arXiv2009.01843OpenAlexW3122842759MaRDI QIDQ5025260

Shashank Shalgar, Irene Tamborra, Ian Padilla-Gay

Publication date: 1 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2009.01843

zbMATH Keywords

neutron starsneutrino properties

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Strong interaction, including quantum chromodynamics (81V05) Weak interaction in quantum theory (81V15) Galactic and stellar structure (85A15) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (1)

COSE\(\nu\): a collective oscillation simulation engine for neutrinos

Uses Software

• SciPy

Cites Work

• Collective neutrino flavor conversion: recent developments
• Dispelling a myth on dense neutrino media: fast pairwise conversions depend on energy

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