Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits
General Relativity and Quantum Cosmology
2015-06-16 v2 High Energy Astrophysical Phenomena
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.
Keywords
Cite
@article{arxiv.1306.6719,
title = {Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits},
author = {Ming-Lei Tong and Bao-Rong Yan and Cheng-Shi Zhao and Dong-Shan Yin and Shu-Hong Zhao and Ting-Gao Yang and Yu-Ping Gao},
journal= {arXiv preprint arXiv:1306.6719},
year = {2015}
}
Comments
3 figures, 1 table, 7 pages, Match with the publication version and the Erratum: Chin. Phys. Lett. 30, 119901, 2013