Monday, July 1, 2013

1306.6719 (Ming-Lei Tong et al.)

Pulsar Timing Residuals Induced by Gravitational Waves from Single
Sources of 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
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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