On the Bottom Magnetic Fields of the Millisecond Pulsars

Chengmin Zhang

On the Bottom Magnetic Fields of the Millisecond Pulsars

Astrophysics 2007-05-23 v1

Authors: Chengmin Zhang

Abstract

The magnetic field strengths of most millisecond pulsars(MSP) are about $10^{8-9}$ Gauss. The accretion induced magnetic field evolution scenario here concludes that the field decay is invesely related to the accreted mass and the minimum field or bottom field stops at about $10^{8}$ Gauss if accreted with the Eddington accretion rate, which is proportionally related with the accretion rate as $\dot{M}^{1/2}$ . The possibility of the low field $\sim 10^{7}$ Gauss MSPs has been proposed for the future radio observation.

Keywords

Abell 168 multicolor study subclusters dynamics luminosity function

Cite

@article{arxiv.astro-ph/0309658,
  title  = {On the Bottom Magnetic Fields of the Millisecond Pulsars},
  author = {Chengmin Zhang},
  journal= {arXiv preprint arXiv:astro-ph/0309658},
  year   = {2007}
}

Comments

2 pages. "To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler"

On the Bottom Magnetic Fields of the Millisecond Pulsars

Abstract

Keywords

Cite

Comments

Related papers