Polarized Gravitational Waves from Gamma-Ray Bursts

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Published 2003 February 13 © 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Shiho Kobayashi and Peter Mészáros 2003 ApJ 585 L89 DOI 10.1086/374307

1538-4357/585/2/L89

Abstract

Significant gravitational-wave emission is expected from gamma-ray bursts arising from compact stellar mergers and possibly also from bursts associated with fast-rotating massive stellar core collapses. These models have in common a high angular rotation rate, and observations provide evidence for jet collimation of the photon emission, with properties depending on the polar angle. Here we consider the gravitational-wave emission and its polarization as a function of angle that is expected from such sources. We discuss possible correlations between the burst photon luminosity or the delay between gravitational-wave bursts and X-ray flashes and the polarization degree of the gravitational waves.

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10.1086/374307