2018/08/15 by Leonard S. Kisslinger, Kisslinger, Leonard S., Bijit Singha +4 · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #FOS: Physical sciences #Geophysics and Gravity Measurements #High Energy Astrophysical Phenomena (astro-ph.HE) #Pulsars and Gravitational Waves Research #astro-ph.HE
paper · pdf · doi:10.48550/arxiv.1808.05265
7 pages,2 figures
openalex publication_date 2018/08/15 · arxiv created 2019/12/05 · arxiv updated 2019/12/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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