Multipole expansion method for supernova neutrino oscillations
Journal Article
·
· Journal of Cosmology and Astroparticle Physics
- Univ. of New Mexico, Albuquerque, NM (United States). Dept. of Physics and Astronomy
Here, we demonstrate a multipole expansion method to calculate collective neutrino oscillations in supernovae using the neutrino bulb model. We show that it is much more efficient to solve multi-angle neutrino oscillations in multipole basis than in angle basis. The multipole expansion method also provides interesting insights into multi-angle calculations that were accomplished previously in angle basis.
- Research Organization:
- Univ. of New Mexico, Albuquerque, NM (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), Basic Energy Sciences (BES)
- Grant/Contract Number:
- SC0008142
- OSTI ID:
- 1454417
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Vol. 2014, Issue 10; ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 9 works
Citation information provided by
Web of Science
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