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

doi:10.1088/0256-307X/30/10/100402

Chin. Phys. Lett.

2013, Vol. 30

Issue (10): 100402 DOI: 10.1088/0256-307X/30/10/100402

GENERAL

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

TONG Ming-Lei^1,2**, YAN Bao-Rong^1,3, ZHAO Cheng-Shi^1,2, YIN Dong-Shan^1,2, ZHAO Shu-Hong^1,2, YANG Ting-Gao^1,2, GAO Yu-Ping^1,2

¹National Time Service Center, Chinese Academy of Sciences, Xi'an 710600
²Key Laboratory of Time and Frequency Primary Standards, Chinese Academy of Sciences, Xi'an 710600
³Key Laboratory of Precision Navigation and Timing Technology, Chinese Academy of Sciences, Xi'an 710600

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TONG Ming-Lei, YAN Bao-Rong, ZHAO Cheng-Shi et al 2013 Chin. Phys. Lett. 30 100402

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Abstract The pulsar timing residuals induced by gravitational waves from non-evolving single binary sources with general elliptical orbits are 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 are calculated for different values of the eccentricity. We 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.

Received: 28 June 2013 Published: 21 November 2013

PACS:	04.30.Db	(Wave generation and sources)
	97.60.Gb	(Pulsars)
	95.85.Sz	(Gravitational radiation, magnetic fields, and other observations)

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https://cpl.iphy.ac.cn/10.1088/0256-307X/30/10/100402 OR https://cpl.iphy.ac.cn/Y2013/V30/I10/100402

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	TONG Ming-Lei
	YAN Bao-Rong
	ZHAO Cheng-Shi
	YIN Dong-Shan
	ZHAO Shu-Hong
	YANG Ting-Gao
	GAO Yu-Ping

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