Gravitational Radiation from Keplerian Binary with Oscillating Orbital Plane

Authors

  • Syed Badiuzzaman Faruque
  • Muhammad Ali Nawaz
  • Muhammad Habibul Ahsan

DOI:

https://doi.org/10.3329/jsr.v1i1.1093

Keywords:

Gravitational wave, Energy, Binary, Oscillating orbit.

Abstract

The gravitational radiation from two point masses in Keplerian circular or elliptic orbit is calculated with the assumption that the orbital plane of the binary undergoes small oscillation about the equilibrium x-y plane. This problem is simplification of a physically possible orbit where one of the point masses is spinning whereby the spin-orbit force drives the orbital plane to wobble in a complicated manner. It is shown that the total energy of gravitational radiation emitted by the binary in this case is greater than the energy emitted when the binary orbit is fixed in the x-y plane. The results presented are in fact a generalization of the classic results of Landau and Lifshitz.

Keywords: Gravitational wave; Energy; Binary; Oscillating orbit.


©2009 JSR Publications. ISSN: 2070-0237(Print); 2070-0245 (Online). All rights

reserved.

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Author Biographies

Syed Badiuzzaman Faruque

Associate Professor
Department of Physics
Shahjalal University of Science and Technology, Sylhet, Bangladesh

Muhammad Ali Nawaz

Department of Physics
Shahjalal University of Science and Technology, Sylhet, Bangladesh

Muhammad Habibul Ahsan

Professor
Department of Physics
Shahjalal University of Science and Technology, Sylhet, Bangladesh

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Published

2008-12-12

How to Cite

Faruque, S. B., Nawaz, M. A., & Ahsan, M. H. (2008). Gravitational Radiation from Keplerian Binary with Oscillating Orbital Plane. Journal of Scientific Research, 1(1), 22–30. https://doi.org/10.3329/jsr.v1i1.1093

Issue

Vol. 1 No. 1 (2009)

Section

Section A: Physical and Mathematical Sciences

License

© Journal of Scientific Research

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