Critical phenomena at the threshold of immediate merger in binary black hole systems: The extreme mass ratio case

Carsten Gundlach, Sarp Akcay, Leor Barack, and Alessandro Nagar
Phys. Rev. D 86, 084022 – Published 4 October 2012

Abstract

In numerical simulations of black hole binaries, Pretorius and Khurana [Classical Quantum Gravity 24, S83 (2007)] have observed critical behavior at the threshold between scattering and immediate merger. The number of orbits scales as nγln|pp*| along any one-parameter family of initial data such that the threshold is at p=p*. Hence, they conjecture that in ultrarelativistic collisions almost all the kinetic energy can be converted into gravitational waves if the impact parameter is fine-tuned to the threshold. As a toy model for the binary, they consider the geodesic motion of a test particle in a Kerr black hole spacetime, where the unstable circular geodesics play the role of critical solutions, and calculate the critical exponent γ. Here, we incorporate radiation reaction into this model using the self-force approximation. The critical solution now evolves adiabatically along a sequence of unstable circular geodesic orbits under the effect of the self-force. We confirm that almost all the initial energy and angular momentum are radiated on the critical solution. Our calculation suggests that, even for infinite initial energy, this happens over a finite number of orbits given by n0.41/η, where η is the (small) mass ratio. We derive expressions for the time spent on the critical solution, number of orbits and radiated energy as functions of the initial energy and impact parameter.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
6 More
  • Received 21 July 2012

DOI:https://doi.org/10.1103/PhysRevD.86.084022

© 2012 American Physical Society

Authors & Affiliations

Carsten Gundlach1, Sarp Akcay1,2, Leor Barack1, and Alessandro Nagar2

  • 1School of Mathematics, University of Southampton, Southampton SO17 1BJ, United Kingdom
  • 2Institut des Hautes Etudes Scientifiques, 91440 Bures-sur-Yvette, France

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 86, Iss. 8 — 15 October 2012

Reuse & Permissions
Access Options

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×