Do monopoles keep white dwarfs hot?

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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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