Published December 25, 2020
| Version v1
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Neutrino emission by plasmon decay in a strong magnetic field: Data material
Authors/Creators
- 1. Tripura University (retired)
- 2. West Bengal University of Technology
Description
This data reference paper summarizes the fundamental calculated results obtained analytically for the case of a neutron star (NS) crust: it’s cooling rate, time-scale evolution and neutrino luminosity, based on two different theories- Photo-Neutrino (PN) interaction and conventional weak interaction. Considering the NS environment as a degenerate plasmon composition the calculation tables are given.
Files
data table for PN.pdf
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(834.1 kB)
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Additional details
References
- Majumder, Brajagopal. PhD thesis: Some aspects of stellar neutrino emission in a strong magnetic field from the view point of photo-neutrino weak coupling theory. Awarded by Calcutta University, India.