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

作　　者：TONG Ming-Lei YAN Bao-Rong ZHAO Cheng-Shi YIN Dong-Shan ZHAO Shu-Hong YANG Ting-Gao GAO Yu-Ping 童明雷;燕保荣;赵成仕;尹东山;赵书红;杨廷高;高玉平(National Time Service Center,Chinese Academy of Sciences,Xi'an 710600;Key Laboratory of Time and Frequency Primary Standards,Chinese Academy of Sciences,Xi'an 710600;Key Laboratory of Precision Navigation and Timing Technology,Chinese Academy of Sciences,Xi'an 710600)

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

出　　处：《Chinese Physics Letters》2013年第10期30-33,共4页中国物理快报（英文版）

基　　金：Supported by the National Natural Science Foundation of China under Grant No 11103024 and the Program of the Light in China’s Western Region of CAS。

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.

关 键 词：massive GRAVITATIONAL properties 

分 类 号：P14[天文地球—天体物理]