Constraints on mass of the DFSZ axions from the carbon - oxygen burning stage of stars
19922 pages
Published in:
- Phys.Lett.B 291 (1992) 97-98
- Published: 1992
Citations per year
Abstract: (Elsevier)
It is believed that carbon burning of detonation or deflagration is an essential process for producing type I supernovae. We consider the effect of the energy loss due to the DFSZ axions on the core temperature of the star, and we use the minimum core temperature needed for a type I supernova to constrain the mass of DFSZ axions.- postulated particle: axion
- mass: axion
- axion: mass
- astrophysics: supernova
- energy loss
- numerical calculations
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