Probing circular polarization in stochastic gravitational wave background with pulsar timing arrays

Ryo Kato and Jiro Soda
Phys. Rev. D 93, 062003 – Published 21 March 2016

Abstract

We study the detectability of circular polarization in a stochastic gravitational wave background from various sources such as supermassive black hole binaries, cosmic strings, and inflation in the early universe with pulsar timing arrays. We calculate generalized overlap reduction functions for the circularly polarized stochastic gravitational wave background. We find that the circular polarization cannot be detected for an isotropic background. However, there is a chance to observe the circular polarization for an anisotropic gravitational wave background. We also show how to separate polarized gravitational waves from unpolarized gravitational waves.

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  • Received 13 January 2016

DOI:https://doi.org/10.1103/PhysRevD.93.062003

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Ryo Kato* and Jiro Soda

  • Department of Physics, Kobe University, Rokkodai 1-1, Kobe 657-8501, Japan

  • *153s107s@stu.kobe-u.ac.jp
  • jiro@phys.sci.kobe-u.ac.jp

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Issue

Vol. 93, Iss. 6 — 15 March 2016

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