Perturbative approach to an orbital evolution around a supermassive black hole

By Y. Mino. 2003

256 citations recorded by the source corpus.

A charge-free, point particle of infinitesimal mass orbiting a Kerr black hole is known to move along a geodesic. When the particle has a finite mass or charge, it emits radiation which carries away orbital energy and angular momentum, and the orbit deviates from a geodesic. In this paper we assume that the deviation is small and show that the half-advanced minus half-retarded field surprisingly provides the correct radiation reaction force, in a time-averaged sense, and determines the orbit of the particle.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/a7b7e4fd65f55d5279dabb61d715b7c69f1f9b60

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

  1. A. Pound
  2. E. Poisson
  3. B. Wardell
  4. T. Hinderer
  5. I. Vega
  6. E. Flanagan
  7. S. Drasco
  8. S. Hughes

In Statistical and Nonlinear Physics

  1. S. Drasco
  2. E. Flanagan
  3. B. Wardell
  4. A. Pound
  5. S. Hughes
  6. T. Hinderer
  7. E. Poisson
  8. T. Sotiriou

Citations in the corpus