The minimum rotation period of millisecond pulsars

The minimum rotation period of millisecond pulsars

A simple and natural explanation for the minimum period of millisecond pulsars follows from a correlation between the accretion rate and the frozen surface dipole magnetic field resulting from Ohmic diffusion through the neutron star crust in initial stages of accretion in low mass X-ray binaries.

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Veröffentlicht in:arXiv.org 2021-06
Hauptverfasser: Ertan, Unal, Alpar, M. Ali
Format: Artikel
Sprache:eng
Schlagworte:
Deposition
Diffusion rate
Dipoles
Millisecond pulsars
Neutron stars
Physics - High Energy Astrophysical Phenomena
X ray binaries
X ray stars
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description A simple and natural explanation for the minimum period of millisecond pulsars follows from a correlation between the accretion rate and the frozen surface dipole magnetic field resulting from Ohmic diffusion through the neutron star crust in initial stages of accretion in low mass X-ray binaries.
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subjects Deposition
Diffusion rate
Dipoles
Millisecond pulsars
Neutron stars
Physics - High Energy Astrophysical Phenomena
X ray binaries
X ray stars
title The minimum rotation period of millisecond pulsars
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