The minimum rotation period of millisecond pulsars

Abstract

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.

3 pages, 1 figure, accepted for publication in MNRAS Letters

References in corpus (6)

• The ATNF Pulsar Catalogue
• A Radio Pulsar/X-ray Binary Link
• Timing Observations of PSR J1023+0038 During a Low-Mass X-ray Binary State
• Vortex Creep Against Toroidal Flux Lines, Crustal Entrainment, and Pulsar Glitches
• Magnetic Fields of Neutron Stars
• On the Torque Reversals of Accreting Neutron Stars

Cited by in corpus (6)

• Searches for Continuous-Wave Gravitational Radiation
• Model-based cross-correlation search for gravitational waves from the low-mass X-ray binary Scorpius X-1 in LIGO O3 data
• Gravitational waves from neutron-star mountains
• On the spin period distribution of millisecond pulsars
• On the minimum spin period of accreting pulsars
• The role of equation of state on the spin-up of millisecond pulsars