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arXiv · 1306.6719

Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits

Ming-Lei Tong·Bao-Rong Yan·Cheng-Shi Zhao·Dong-Shan Yin·Shu-Hong Zhao·Ting-Gao Yang·Yu-Ping Gao
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Abstract

The pulsar timing residuals induced by gravitational waves from non-evolving single binary sources with general elliptical orbits will be analyzed. For different orbital eccentricities, the timing residuals present different properties. The standard deviations of the timing residuals induced by a fixed gravitational wave source will be calculated for different values of the eccentricity. We will also analyze the timing residuals of PSR J0437-4715 induced by one of the best known single gravitational wave sources, the supermassive black hole binary in the blazar OJ287.

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Ming-Lei Tong, Bao-Rong Yan, Cheng-Shi Zhao, Dong-Shan Yin, Shu-Hong Zhao, Ting-Gao Yang, Yu-Ping Gao. 2013-06-28. Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits. https://doi.org/10.1088/0256-307x/30/10/100402

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