Axion Emission from Neutron Stars - INSPIRE

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Axion Emission from Neutron Stars

N. Iwamoto
(
- UC, Santa Barbara and
- Washington U., St. Louis
)

1984

4 pages

Published in:

Phys.Rev.Lett. 53 (1984) 1198-1201

DOI:

10.1103/PhysRevLett.53.1198

{{\mathit A}^{0}}

(Axion) MASS LIMITS from Astrophysics and Cosmology

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Abstract: (APS)

We show 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.

N: MATTER
ASTROPHYSICS
POSTULATED PARTICLE: AXION
N N: INTERACTION
INTERACTION: N N
EMISSION: AXION
AXION: EMISSION
ENERGY LOSS
FEYNMAN GRAPH
NUMERICAL CALCULATIONS

References(34)

Figures(0)

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