Constraints of the neutrino magnetic moment from white dwarf cooling

Details Constraints of the neutrino magnetic moment from white dwarf cooling Constraints of the neutrino magnetic moment from white dwarf cooling

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.189....1w&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 189, no. 1, March 1992, p. 1-4.

Astronomy and Astrophysics

Astrophysics

3

Cooling, Magnetic Moments, Neutrinos, Stellar Temperature, White Dwarf Stars, Energy Dissipation, Stellar Luminosity, Stellar Mass

Scientific paper

The neutrino magnetic moment provides an additional energy emission in stars. It will accelerate the white dwarf cooling process and reduce the life time of the white dwarf, but it causes a conflict with the observation. Observational constraints are used to derive an upper limit for the neutrino magnetic moment: munu is about 4.0 x 10 exp -12 mu sub B.

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