Gravitational Radiation From Pulsar Creation
High Energy Astrophysical Phenomena
2019-12-06 v3
Abstract
We estimate the gravitational wave amplitude as a function of frequency produced during the creation of pulsars from the gravitational collapse of a massive star. The three main quantities needed are the magnitude of the magnetic field producing pulsar kicks, the temperature which determines the velocity of the pulsar and the duration time for the gravitational radiation.res
Keywords
Cite
@article{arxiv.1808.05265,
title = {Gravitational Radiation From Pulsar Creation},
author = {Leonard S. Kisslinger and Bijit Singha and Zhou Li-juan},
journal= {arXiv preprint arXiv:1808.05265},
year = {2019}
}
Comments
7 pages,2 figures