Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...286..216f&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 286, Nov. 1, 1984, p. 216-220.
Astronomy and Astrophysics
Astrophysics
17
Magnetic Monopoles, Stellar Temperature, White Dwarf Stars, Galaxies, Main Sequence Stars, Stellar Evolution, Stellar Luminosity, Stellar Magnitude
Scientific paper
Although theoretical cooling curves predict large numbers of faint white dwarfs (Mbol ≥ 16), none have been observed singly or even inferred as the missing objects in binary systems. The author suggests magnetic monopole-catalyzed nucleon decay as a mechanism for keeping white dwarfs hot (Mbol < 16). At the same time the observed luminosities of old white dwarfs (L = 10-4L_sun;) place an upper limit on the product of monopole flux times cross section for catalysis, (F/cm-2s-1sr-1)(σv/10-28cm2) ≤ 2×10-18.
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