Microscopic magnetic dipole radiation in neutron stars

Abstract

There is ${}^3{P}_2$ neutron superfluid region in NS (neutron star) interior. For a rotating NS, the ${}^3{P}_2$ superfluid region is like a system of rotating magnetic dipoles. It will give out electromagnetic radiation, which may provides a new heating mechanism of NSs. This heating mechanism plus some cooling agent may give sound explanation to NS glitches.

To be published by ChJAA

References in corpus (3)

• Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations
• Thermal evolution of rotating hybrid stars
• Improbability of DUrca process constraints EOS