Parametric Classification of Gravitational Wave Chirp Signals

Details Parametric Classification of Gravitational Wave Chirp Signals Parametric Classification of Gravitational Wave Chirp Signals

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprs12005g&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

A possible approach to the classification of gravitational-wave chirp signals is presented. This approach is theory neutral and parametric in the spirit of the parameterized post-Newtonian (PPN) approach to classifying alternate theories of gravity. Also similar to the PPN approach, all possible chirps are parameterized in terms of their deviation from the chirps predicted by general relativity (GR). Separation of theoretical from astrophysical parameters is considered. The evolution of the phase, amplitude, and shape of the quasi-sinusoidal chirp is parameterized. The relation of these directly observable parameters to the determination of the time-varying eccentricity, inclination and orientation of the source system during the inspiral is considered. The possibility of determining the mass, spin, angular momentum and distance of the source system is also considered.

Affiliated with

Also associated with

No associations

Rating

Parametric Classification of Gravitational Wave Chirp Signals does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Parametric Classification of Gravitational Wave Chirp Signals, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Parametric Classification of Gravitational Wave Chirp Signals will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1539408