Constraints on mass of the DFSZ axions from the carbon-oxygen burning stage of stars

Details Constraints on mass of the DFSZ axions from the carbon-oxygen burning stage of stars Constraints on mass of the DFSZ axions from the carbon-oxygen burning stage of stars

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..291...97w&link_type=abstract

Physics Letters B, Volume 291, Issue 1-2, p. 97-98.

Physics

3

Scientific paper

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.

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