Detectability of Gravitational Waves from the R-Mode Instability in Newly-Born Neutron Stars

Details Detectability of Gravitational Waves from the R-Mode Instability in Newly-Born Neutron Stars Detectability of Gravitational Waves from the R-Mode Instability in Newly-Born Neutron Stars

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1142s&link_type=abstract

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

Physics

Neutron Stars, Gravitational Waves, R-Mode Instability

Scientific paper

Recently, it was shown that differential rotation is an unavoidable feature of r-modes. We investigate its influence on the detectability of gravitational waves emitted by a newly-born, hot, rapidly-rotating neutron star, as it spins down due to the r-mode instability. We conclude that gravitational radiation could be detected by advanced laser interferometer detectors if the amount of differential rotation at the time the r-mode instability becomes active is not too high.

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