Using NRGR To Model Gravitational Radiation

Details Using NRGR To Model Gravitational Radiation Using NRGR To Model Gravitational Radiation

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21347715p&link_type=abstract

American Astronomical Society, AAS Meeting #213, #477.15

Astronomy and Astrophysics

Astronomy

Scientific paper

Predicted by general relativity but not yet directly observed, gravitational waves could soon be detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO). Coalescing compact binaries are powerful emitters of gravitational waves, and provide a strong gravity environment ideal for the testing of gravity theories. We study the gravitational wave emission in non-relativistic binary systems using NRGR - an effective field theory formalism which takes into account the different length scales in the system. This formalism is applicable to all orders in the orbital velocity. We calculate in this framework the subleading spin-orbit corrections to the newtonian potential.

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