Abstract
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 2 couplings must be less than 10-11.
| Original language | English |
|---|---|
| Pages (from-to) | 1522-1525 |
| Number of pages | 4 |
| Journal | Physical Review Letters |
| Volume | 48 |
| Issue number | 22 |
| DOIs | |
| Publication status | Published - Jan 1 1982 |
| Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy(all)
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Cite this
Fukugita, M., Watamura, S., & Yoshimura, M. (1982). Light pseudoscalar particle and stellar energy loss. Physical Review Letters, 48(22), 1522-1525. https://doi.org/10.1103/PhysRevLett.48.1522