Axion emission from neutron stars

Details Axion emission from neutron stars Axion emission from neutron stars

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phrvl..53.1198i&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 53, Sept. 17, 1984, p. 1198-1201. NASA-supported research.

Physics

102

Bosons, Broken Symmetry, Neutron Stars, Stellar Radiation, Particle Mass, Stellar Temperature

Scientific paper

The author shows that axion emission from neutron stars is the dominant
energy-loss mechanism for a range of values of the Peccei-Quinn
symmetry-breaking scale (F) not excluded by previous constraints. This
gives the possibility of obtaining a better bound on F from measurements
of surface temperature of neutron stars.

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