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  • Access by Xinjiang University

Radial Motion of a Spinning Test Body in the Field of a Black Hole

R. F. O'Connell

  • Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803

Phys. Rev. D 6, 3035 – Published 15 November, 1972

DOI: https://doi.org/10.1103/PhysRevD.6.3035

Abstract

The gravitational radiation emitted by a test particle falling radially into a Schwarzchild black hole has been analyzed by Zerilli. Here we investigate the effect of assigning spin to both the test particle and the source. We find that more (less) gravitational radiation is emitted if the spins are antiparallel (parallel).

Original Article

Gravitational Field of a Particle Falling in a Schwarzschild Geometry Analyzed in Tensor Harmonics

Frank J. Zerilli
Phys. Rev. D 2, 2141 (1970)

References (6)

  1. F. Zerilli, Phys. Rev. D 2, 2141 (1970)
  2. B. M. Barker and R. F. O'Connell, Phys. Rev. D 2, 1428 (1970)
  3. R. F. O'Connell, Phys. Letters 32A, 402 (1970)
  4. R. F. O'Connell, in Proceedings of the Varenna 1972 Summer School on Experimental Gravitation (unpublished)
  5. [2]
  6. V. B. Berestetskii, E. M. Lifshitz, and L. P. Pitaevskii, Relativistic Quantum Theory (Addison-Wesley, Reading, Mass., 1971), p. 286

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