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Axion cooling of white dwarfs

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arxiv 1304.7652 v1 pith:VP6LCMNV submitted 2013-04-29 astro-ph.SR

Axion cooling of white dwarfs

J. Isern (CSIC-IEEC) , S. Catalan (University of Hertfordshire) , E. Garcia--Berro (Universitat Politecnica Catalunya - IEEC) , M. Salaris (Liverpool John Moores University) , S. Torres (Universitat Politecnica Catalunya - IEEC) This is my paper
classification astro-ph.SR
keywords whiteaxiondwarfsfunctionluminosityprocessstarsconstrained
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The evolution of white dwarfs is a simple gravothermal process. This process can be tested in two ways, through the luminosity function of these stars and through the secular variation of the period of pulsation of those stars that are variable. Here we show how the mass of the axion can be constrained using the white dwarf luminosity function.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Axion-photon conversion in stochastic magnetic fields

    hep-ph 2025-12 accept novelty 6.0

    Axion-photon conversion in random Gaussian magnetic fields fixes the expectation values and variances of photon Stokes parameters, including a circular-polarization signal from helical fields.