On the Bottom Magnetic Fields of the Millisecond Pulsars

Details On the Bottom Magnetic Fields of the Millisecond Pulsars On the Bottom Magnetic Fields of the Millisecond Pulsars

2003-09-24

arxiv.org/abs/astro-ph/0309658v1

IAUS 218 (2004) 47-48

Astronomy and Astrophysics

Astrophysics

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

Scientific paper

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.

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