GRAVITATIONAL WAVEFORMS FOR FINITE MASS BINARIES-Reference-Cited by-同舟云学术

GRAVITATIONAL WAVEFORMS FOR FINITE MASS BINARIES

Published:2007-05-20 Issue:13 Volume:22 Page:2405-2414
ISSN:0217-751X
Container-title:International Journal of Modern Physics A
language:en
Short-container-title:Int. J. Mod. Phys. A

Author:

VASÚTH MÁTYÁS¹,MAJÁR JÁNOS¹

Affiliation:

1. KFKI Research Institute for Particle and Nuclear Physics, Budapest 114, PO Box 49, H-1525, Hungary

Abstract

One of the promising sources of gravitational radiation is a binary system composed of compact stars. It is an important question of how the rotation of the bodies and the eccentricity of the orbit affect the detectable signal. Here we present a method to evaluate the gravitational wave polarization states for inspiralling compact binaries with comparable mass. We consider eccentric orbits and the spin-orbit contribution in the case of one spinning object up to 1.5 post-Newtonian order. For circular orbits our results are in agreement with existing calculations.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0217751X07036488

Reference21 articles.

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