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

被引：7

作者：

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
]}

机构：

[1] Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Peoples R China

[2] Chinese Acad Sci, Key Lab Time & Frequency Primary Stand, Xian 710600, Peoples R China

[3] Chinese Acad Sci, Key Lab Precis Nav & Timing Technol, Xian 710600, Peoples R China

来源：

CHINESE PHYSICS LETTERS | 2013年 / 30卷 / 10期

基金：

中国国家自然科学基金;

关键词：

LIMITS; POLARIZATION; SENSITIVITY; RADIATION; ARRAY;

D O I：

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

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

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.

引用

页数：4

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[2] Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits (vol 30, 100402, 2013)
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[3] Erratum:Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits[Chin.Phys.Lett.30(2013) 100402]
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