Axion emission rates in stars and constraints on its mass

Details Axion emission rates in stars and constraints on its mass Axion emission rates in stars and constraints on its mass

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..33.3509p&link_type=abstract

Physical Review D (Particles and Fields), Volume 33, Issue 12, 15 June 1986, pp.3509-3518

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54

Applications Of Electroweak Models To Specific Processes, Elementary Particle Processes, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

We have calculated in detail the emission rates of the invisible axion of Dine, Fischler, and Srednicki in several representative types of stars and derived upper bounds for its mass. We give, in particular, complete reaction amplitudes and energy rates for axion emission. Our results for the axion mass limits are in qualitative agreement with previous estimates for most of the cases except for the neutron stars which give a stronger bound on the axion mass.

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