On the Circular Orbit Approximation for Binary Compact Objects In General Relativity

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10 pages, 12 figures, revtex4

Scientific paper

10.1103/PhysRevD.69.124013

One often-used approximation in the study of binary compact objects (i.e., black holes and neutron stars) in general relativity is the instantaneously circular orbit assumption. This approximation has been used extensively, from the calculation of innermost circular orbits to the construction of initial data for numerical relativity calculations. While this assumption is inconsistent with generic general relativistic astrophysical inspiral phenomena where the dissipative effects of gravitational radiation cause the separation of the compact objects to decrease in time, it is usually argued that the timescale of this dissipation is much longer than the orbital timescale so that the approximation of circular orbits is valid. Here, we quantitatively analyze this approximation using a post-Newtonian approach that includes terms up to order ({Gm/(rc^2)})^{9/2} for non-spinning particles. By calculating the evolution of equal mass black hole / black hole binary systems starting with circular orbit configurations and comparing them to the more astrophysically relevant quasicircular solutions, we show that a minimum initial separation corresponding to at least 6 (3.5) orbits before plunge is required in order to bound the detection event loss rate in gravitational wave detectors to < 5% (20%). In addition, we show that the detection event loss rate is > 95% for a range of initial separations that include all modern calculations of the innermost circular orbit (ICO).

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

On the Circular Orbit Approximation for Binary Compact Objects In General Relativity 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 On the Circular Orbit Approximation for Binary Compact Objects In General Relativity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Circular Orbit Approximation for Binary Compact Objects In General Relativity will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-263353

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.