Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral

Details Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral

2009-11-20

arxiv.org/abs/0911.3899v4

Phys.Rev.D84:044019,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

21 pages, 5 figures. v4: added section with numerical evaluation of the ringdown amplitudes

Scientific paper

10.1103/PhysRevD.84.044019

An extreme mass ratio inspiral consists of two parts: adiabatic inspiral and plunge. The plunge trajectory from the innermost stable circular orbit (ISCO) is special (somewhat independent of initial conditions). We write an expression for its solution in closed-form and for the emitted waveform. In particular we extract an expression for the associated black-hole ringdown amplitudes, and evaluate them numerically.

Affiliated with

Also associated with

No associations

Rating

Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral 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 Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-431179