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 differen...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.展开更多
PACS:99.10.−x,04.30.Db,97.60.Gb,95.85.Sz DOI:10.1088/0256-307X/30/11/119901 One regrettable error appeared in Eq.(21)of our article[Chin.Phys.Lett.30(2013)100402].The cor-rect one of the equation is as follows.
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。
文摘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.
文摘PACS:99.10.−x,04.30.Db,97.60.Gb,95.85.Sz DOI:10.1088/0256-307X/30/11/119901 One regrettable error appeared in Eq.(21)of our article[Chin.Phys.Lett.30(2013)100402].The cor-rect one of the equation is as follows.
