Cooling of white dwarfs - A method of determining their mean mass and constraints on neutrino properties

Details Cooling of white dwarfs - A method of determining their mean mass and constraints on neutrino properties Cooling of white dwarfs - A method of determining their mean mass and constraints on neutrino properties

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..362b&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 70, no. 2, p. 362-371.

Astronomy and Astrophysics

Astronomy

3

Neutrinos, Stellar Evolution, Stellar Mass, Stellar Temperature, White Dwarf Stars, Stellar Luminosity, Stellar Models

Scientific paper

Calculations of the evolution of white dwarfs with 0.5-0.8 solar mass
are carried out. An upper limit for a neutrino magnetic moment of less
than 10 exp -11 mu(B) is confirmed. In the 'standard' theory of cooling
(with a zeroth neutrino magnetic moment), the best agreement with
observations is achieved when M = 0.7 solar mass.

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