Pulsar timing residuals due to individual non-evolving gravitational wave sources

Abstract

The pulsar timing residuals induced by gravitational waves from non-evolving single binary sources are affected by many parameters related to the relative positions of the pulsar and the gravitational wave sources. We will fully analyze the effects due to different parameters one by one. The standard deviations of the timing residuals will be calculated with a variable parameter fixing a set of other parameters. The orbits of the binary sources will be generally assumed to be elliptical. The influences of different eccentricities on the pulsar timing residuals will also studied in detail. We find that effects of the related parameters are quite different, and some of them present certain regularities.

12 pages, 6 figures, 2 tables, some minor revisions. arXiv admin note: text overlap with arXiv:1306.6719

References in corpus (9)

• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project
• The Parkes Pulsar Timing Array Project
• TEMPO2, a new pulsar timing package. III: Gravitational wave simulation
• ASTROD-GW: Overview and Progress
• Relic Gravitational Waves in the Accelerating Universe
• Using polarized maser to detect high-frequency relic gravitational waves
• Relic gravitational waves in the frame of slow-roll inflation with a power-law potential and the detection
• Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits