Light Pseudoscalar Particle and Stellar Energy Loss

Details Light Pseudoscalar Particle and Stellar Energy Loss Light Pseudoscalar Particle and Stellar Energy Loss

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phrvl..48.1522f&link_type=abstract

Physical Review Letters, Volume 48, Issue 22, May 31, 1982, pp.1522-1525

Physics

156

Elementary Particle Processes

Scientific paper

A bound on the coupling strengths of a very light pseudoscalar particle
is derived from stellar energy loss at various stages of evolution: the
sun, red giants, and cooling white dwarfs. The dimensionless Yukawa and
2γ couplings must be less than 10-11.

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