Spin Period Evolution of Recycled Pulsar in Accreting Binary

Details Spin Period Evolution of Recycled Pulsar in Accreting Binary Spin Period Evolution of Recycled Pulsar in Accreting Binary

2010-11-23

arxiv.org/abs/1011.5013v1

2011, Astron & Astrophys, 526, 88

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

9 pages, 6 figs, accepted by A\& A 2010

Scientific paper

We investigate the spin-period evolutions of recycled pulsars in binary accreting systems. Taking both the accretion induced field decay and spin-up into consideration, we calculate their spin-period evolutions influenced by the initial magnetic-field strengths, initial spin-periods and accretion rates, respectively. The results indicate that the minimum spin-period (or maximum spin frequency) of millisecond pulsar (MSP) is independent of the initial conditions and accretion rate when the neutron star (NS) accretes $\sim> 0.2\ms$. The accretion torque with the fastness parameter and gravitational wave (GW) radiation torque may be responsible for the formation of the minimum spin-period (maximum spin frequency). The fastest spin frequency (716 Hz) of MSP can be inferred to associate with a critical fastness parameter about $\omega_{c}=0.55$. Furthermore, the comparisons with the observational data are presented in the field-period ($B-P$) diagram.

Affiliated with

Also associated with

No associations

Rating

Spin Period Evolution of Recycled Pulsar in Accreting Binary does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spin Period Evolution of Recycled Pulsar in Accreting Binary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spin Period Evolution of Recycled Pulsar in Accreting Binary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-587545