Physics
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phlb..144..391k&link_type=abstract
Physics Letters B, Volume 144, Issue 5-6, p. 391-394.
Physics
44
Scientific paper
We consider the contribution of bremsstrahlung emission of axions to stellar energy losses. This process has a much weaker temperature dependence than previously considered axion emission processes. It is comparable to these processes in the sun, and for objects with non-degenerate core temperatures less than 85% that of the solar core, axion bremsstrahlung will dominate. We briefly consider the implications of these axionsemission losses for altering the evolution of old globular cluster stars.
Research supported in part by the National Science Foundation under Grant No. PHY77-27084.
Krauss Lawrence M.
Moody John E.
Wilczek Frank
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