Published April 3, 2019
| Version v1
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Neutrinos from Beta Processes in a Presupernova: Probing the Isotopic Evolution of a Massive Star
- 1. Institute for Nuclear Theory, University of Washington
- 2. Arizona State University
- 3. University of Amsterdam
- 4. School of Earth and Space Exploration, Arizona State University
Description
We present datasets for neutrino luminosity, differential in neutrino energy, of 15 \(M_{\odot}\)and 30 \(M_{\odot}\) presupernova stars at various times during the stellar evolution. We include here the total luminosity from both pair production and beta processes. The beta process neutrino luminosities are also split into contributions from individual isotopes. For more information, please see the attached README.txt file.
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15NuSeparateIsotopes.zip
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Additional details
References
- K. M. Patton, C. Lunardini, R. J. Farmer, and F. X. Timmes ApJ 851, 6 (2017)