Gravitational waves from r-modes

Details Gravitational waves from r-modes Gravitational waves from r-modes

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.308..557s&link_type=abstract

Astrophysics and Space Science, Volume 308, Issue 1-4, pp. 557-561

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Detectability of gravitational waves emitted by newly born, hot, rapidly rotating neutron stars as they spin down due to the r-mode instability is discussed. It is shown that differential rotation induced by r-modes plays a fundamental role in the evolution of the mode’s instability, making it more difficult to detect these gravitational waves.

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