On measuring the gravitational-wave background using Pulsar Timing Arrays

Abstract

Long-term precise timing of Galactic millisecond pulsars holds great promise for measuring the long-period (months-to-years) astrophysical gravitational waves. Several gravitational-wave observational programs, called Pulsar Timing Arrays (PTA), are being pursued around the world. Here we develop a Bayesian algorithm for measuring the stochastic gravitational-wave background (GWB) from the PTA data. Our algorithm has several strengths: (1) It analyses the data without any loss of information, (2) It trivially removes systematic errors of known functional form, including quadratic pulsar spin-down, annual modulations and jumps due to a change of equipment, (3) It measures simultaneously both the amplitude and the slope of the GWB spectrum, (4) It can deal with unevenly sampled data and coloured pulsar noise spectra. We sample the likelihood function using Markov Chain Monte Carlo (MCMC) simulations. We extensively test our approach on mock PTA datasets, and find that the algorithm has significant benefits over currently proposed counterparts. We show the importance of characterising all red noise components in pulsar timing noise by demonstrating that the presence of a red component would significantly hinder a detection of the GWB. Lastly, we explore the dependence of the signal-to-noise ratio on the duration of the experiment, number of monitored pulsars, and the magnitude of the pulsar timing noise. These parameter studies will help formulate observing strategies for the PTA experiments.

10 pages, 12 figures

References in corpus (10)

• TEMPO2, a new pulsar timing package. I: Overview
• Gravitational radiation from cosmic (super)strings: bursts, stochastic background, and observational windows
• Self-Regulated Growth of Supermassive Black Holes in Galaxies as the Origin of the Optical and X-ray Luminosity Functions of Quasars
• Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries
• Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects
• Detecting the stochastic gravitational wave background using pulsar timing
• Optimal strategies for gravitational wave stochastic background searches in pulsar timing data
• Relic Gravitational Waves and Cosmology
• Radio Astronomical Polarimetry and the Lorentz Group
• Low-Frequency Gravitational Radiation from Coalescing Massive Black Holes

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