Statistical characteristics of a stochastic background of gravitational waves from neutron star formation

Details Statistical characteristics of a stochastic background of gravitational waves from neutron star formation Statistical characteristics of a stochastic background of gravitational waves from neutron star formation

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19.1303c&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 7, pp. 1303-1307 (2002).

Computer Science

6

Scientific paper

By using a recent model for the evolving star formation rate, we investigate the statistical distribution of gravitational wave amplitudes due to supernovae that result in neutron star formation in the Einstein-de Sitter cosmology. To account for the uncertainty in gravitational wave emission for this source type, we use a random mixture of three simulated waveform types computed by Zwerger and Müller. We investigate statistical parameters of the resulting gravitational wave amplitude distribution in our frame.

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