SIMBAD references

2013ApJ...775..124F - Astrophys. J., 775, 124 (2013/October-1)

Population synthesis of young isolated neutron stars: the effect of fallback disk accretion and magnetic field evolution.

FU L. and LI X.-D.

Abstract (from CDS):

The spin evolution of isolated neutron stars (NSs) is dominated by their magnetic fields. The measured braking indices of young NSs show that the spin-down mechanism due to magnetic dipole radiation with constant magnetic fields is inadequate. Assuming that the NS magnetic field is buried by supernova fallback matter and re-emerges after accretion stops, we carry out a Monte Carlo simulation of the evolution of young NSs, and show that most of the pulsars have braking indices ranging from -1 to 3. The results are compatible with the observational data of NSs associated with supernova remnants. They also suggest that the initial spin periods of NSs might occupy a relatively wide range.

Abstract Copyright:

Journal keyword(s): accretion, accretion disks - magnetic fields - pulsars: general - stars: neutron

Simbad objects: 98

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2019.09.21-12:03:07

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