English

Measuring Parity Violation in the Stochastic Gravitational Wave Background with the LISA-Taiji network

Cosmology and Nongalactic Astrophysics 2021-04-02 v2 General Relativity and Quantum Cosmology

Abstract

Parity violation is a powerful observable to distinguish a cosmological background of Gravitational Waves (GWs) from an astrophysical one. Planar single GW interferometers, both on ground and in space, are unable to measure the net circular polarization of an isotropic Stochastic Gravitational Wave Background (SGWB). In this paper, we explore the possibility of detecting circular polarization of an isotropic SGWB by cross-correlating two space-based detectors planned to be launched around 2034: LISA and Taiji. We compute the response of such a network to chirality and we perform a Fisher forecast analysis on the II and VV Stokes parameters for the SGWB. We find that a clear measurement of chirality can be claimed for a maximally chiral signal with h2ΩGW1012h^2 \, \Omega_{\rm GW} \simeq 10^{-12}.

Keywords

Cite

@article{arxiv.2011.07059,
  title  = {Measuring Parity Violation in the Stochastic Gravitational Wave Background with the LISA-Taiji network},
  author = {Giorgio Orlando and Mauro Pieroni and Angelo Ricciardone},
  journal= {arXiv preprint arXiv:2011.07059},
  year   = {2021}
}

Comments

22 pages, 4 figures