English

Magnetic Field-Decay-Induced Electron Captures: a Strong Heat Source in Magnetar Crusts

High Energy Astrophysical Phenomena 2015-05-14 v2 Solar and Stellar Astrophysics Nuclear Experiment Nuclear Theory

Abstract

We propose a new heating mechanism in magnetar crusts. Magnetars' crustal magnetic fields are much stronger than their surface fields; therefore, magnetic pressure partially supports the crust against gravity. The crust loses magnetic pressure support as the field decays and must compensate by increasing the electron degeneracy pressure; the accompanying increase in the electron Fermi energy induces nonequilibrium, exothermic electron captures. The total heat released via field-decay electron captures is comparable to the total magnetic energy in the crust. Thus, field-decay electron captures are an important, if not the primary, mechanism powering magnetars' soft X-ray emission.

Keywords

Cite

@article{arxiv.0910.2466,
  title  = {Magnetic Field-Decay-Induced Electron Captures: a Strong Heat Source in Magnetar Crusts},
  author = {Randall L. Cooper and David L. Kaplan},
  journal= {arXiv preprint arXiv:0910.2466},
  year   = {2015}
}

Comments

4 pages, 2 figures, minor improvements, results and conclusions unchanged; accepted by ApJL