On the Bottom Magnetic Fields of the Millisecond Pulsars
| dc.creator | Zhang, Chengmin | |
| dc.date | 2003-09-24 | |
| dc.date.accessioned | 2026-07-07T07:37:18Z | |
| dc.date.available | 2026-07-07T07:37:18Z | |
| dc.description | 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. | |
| dc.description | 2 pages. "To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0309658 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0309658 | |
| dc.identifier | IAUS 218 (2004) 47-48 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/120729 | |
| dc.subject | Astrophysics | |
| dc.title | On the Bottom Magnetic Fields of the Millisecond Pulsars | |
| dc.type | text |