Gravitational Collapse of Population III Stars

Details Gravitational Collapse of Population III Stars Gravitational Collapse of Population III Stars

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1101s&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

We have simulated the collapse of rotating Population III stars with numerical simulation and extracted the gravitational waves from the mass motions via the quadrupole formula. In addition, we estimate the gravitational wave emission by anisotropic neutrino radiation. With these wave forms, we calculate the gravitational wave background from Population III stars. As a result, we have found that the gravitational wave background from Population III stars is large enough to be detected by interferometers such as BBO and DECIGO without correlation.

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