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Rapid Spin Deceleration of Magnetized Proto-Neutron Stars via Asymmetric Neutrino Emission

We calculate the spin deceleration of proto-neutron stars by asymmetric neutrino absorption in the context of a fully relativistic mean field theory. We calculate for the first time the spin deceleration of neutron stars due to asymmetric neutrino absorption in a toroidal magnetic field configurations. We find a surprising effect that the deceleration can much larger for asymmetric neutrino absorption in a toroidal magnetic field than the usually presumed braking due to magnetic dipole radiation. This may explain the observation that magnetars appear to have had a more rapid deceleration in the past.

preprint2014arXivOpen access
T. MaruyamaJ. HidakaT. KajinoN. YasutakeT. KurodaM. K. CheounC. Y. RyuGrant. J. Mathews
hep-phastro-ph.HEnucl-thastro-ph.SR
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Open access8 authors4 topics
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T. MaruyamaJ. HidakaT. KajinoN. YasutakeT. KurodaM. K. CheounC. Y. RyuGrant. J. Mathews

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