English

From microphysics to dynamics of magnetars

High Energy Astrophysical Phenomena 2017-07-11 v1 Solar and Stellar Astrophysics Nuclear Theory

Abstract

MeV-scale magnetic fields in the interiors of magnetars suppress the pairing of neutrons and protons in the SS-wave state. In the case of a neutron condensate the suppression is the consequence of the Pauli-paramagnetism of the neutron gas, i.e., the alignment of the neutron spins along the magnetic field. The proton SS-wave pairing is suppressed because of the Landau diamagnetic currents of protons induced by the field. The Ginzburg-Landau and BCS theories of the critical magnetic fields for unpairing are reviewed. The macrophysical implications of the suppression (unpairing) of the condensates are discussed for the rotational crust-core coupling in magnetars and the neutrino-dominated cooling era of their thermal evolution.

Keywords

Cite

@article{arxiv.1701.00895,
  title  = {From microphysics to dynamics of magnetars},
  author = {Armen Sedrakian and Xu-Guang Huang and Monika Sinha and John W. Clark},
  journal= {arXiv preprint arXiv:1701.00895},
  year   = {2017}
}

Comments

10 pages, 4 figures, Proceedings of "Compact Stars in the QCD phase diagram V", 23-27 May 2016 GSSI and LNGS, L'Aquila, Italy

R2 v1 2026-06-22T17:40:35.552Z