Axion decay in a strong magnetic field and radio fluxes from magnetic white dwarfs

Details Axion decay in a strong magnetic field and radio fluxes from magnetic white dwarfs Axion decay in a strong magnetic field and radio fluxes from magnetic white dwarfs

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169..271g&link_type=abstract

(IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics a

Astronomy and Astrophysics

Astrophysics

Magnetic Stars, Particle Flux Density, Radio Emission, Stellar Magnetic Fields, White Dwarf Stars, Dark Matter, Neutron Stars, Particle Mass, Red Giant Stars, Stellar Evolution

Scientific paper

Radio emission of isolated magnetic white dwarfs due to invisible axions
decay in a strong magnetic field is estimated. It is possible to reach
theoretical limits on the abundance and coupling of cosmic axions,
provided that radio fluxes would be observed at the level of 1 microJy
or less.

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