Effect of collective neutrino oscillations on the neutrino mechanism of core-collapse supernovae
Author:
Affiliation:
1. Department of Astronomy; The Ohio State University; 140 West 18th Avenue; Columbus; OH; 43210; USA
2. Center for Cosmology and Astroparticle Physics; The Ohio State University; 191 West Woodruff Avenue; Columbus; OH; 43210; USA
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/425/2/1083/4014390/425-2-1083.pdf
Reference61 articles.
1. The Magnetorotational Instability in Core‐Collapse Supernova Explosions
2. Revival of a stalled supernova shock by neutrino heating
3. The prompt-shock supernova mechanism. I - The effect of the free-proton mass fraction and the neutrino transport algorithm
4. The prompt-shock supernova mechanism. II - Supranuclear EOS behavior and the precollapse model
5. The Role of Doubly Diffusive Instabilities in the Core-Collapse Supernova Mechanism
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3. Fast neutrino flavor conversions near the supernova core with realistic flavor-dependent angular distributions;Journal of Cosmology and Astroparticle Physics;2017-02-10
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