About pulsars dynamical evolution

Details About pulsars dynamical evolution About pulsars dynamical evolution

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..279l&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Pulsars: General, Stars: Neutron

Scientific paper

Based on the assumption that pulsars are losing their rotational energy according to dot{ν}=-kν^n where ν is the frequency, dot{ν} its first derivative, and n is the braking index, four evolutionary models are created. Using them, thousands of artificial pulsar populations were generated. A comparison between these populations, and the no glitches and no milisecond pulsars reported by Hobbs et al. (2004) is performed using a Kolmogorov-Smirnov test (K-S).

Affiliated with

Also associated with

No associations

Rating

About pulsars dynamical evolution 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 About pulsars dynamical evolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and About pulsars dynamical evolution will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674517