PSNS index

Astrophysical sources of the neutrinos

Neutrino processes and spectra

Artwork

Presentations

Publications

Numerical data and codes

People and collaboration

Astro-neutrino links

Basically, we can group processess leading to the neutrino emission into two groups:

• thermal neutrinos
• weak nuclear (NSE) neutrinos

Thermal neutrino emission depends only on temperature and electron density. Three classic processes are:

1. Pair-annihilation:
   
   
2. Plasmon decay:
   
   
3. Photoproduction:
   
   

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Main page , Author: A. Odrzywolek, andrzej.odrzywolek@uj.edu.pl Template modified: 2015-03-15