General metric theories in a four-dimensional spacetime allow at most six polarization states (two spin-0, two spin-1 and two spin-2) of gravitational waves (GWs). If a sky location of a GW source with the electromagnetic counterpart satisfies a single equation that we propose in this paper, both the spin-1 modes and spin-2 ones can be eliminated from a certain combination of strain outputs at four ground-based GW interferometers (e.g. a network of aLIGO-Hanford, aLIGO-Livingston, Virgo and KAGRA), where this equation describes curves on the celestial sphere. This means that, if a GW source is found in the curve (or its neighborhood practically), a direct test of scalar (spin-0) modes separately from the other (vector and tensor) modes become possible in principle. The possibility of such a direct test is thus higher than an earlier expectation (Hagihara et al. PRD, 100, 064010, 2019), in which they argued that the vector modes could not be completely eliminated. We discuss also that adding the planned LIGO-India detector as a fifth detector will increase the feasibility of scalar polarization tests.
@article{arxiv.1912.06340,
title = {Condition for directly testing scalar modes of gravitational waves by four detectors},
author = {Yuki Hagihara and Naoya Era and Daisuke Iikawa and Naohiro Takeda and Hideki Asada},
journal= {arXiv preprint arXiv:1912.06340},
year = {2020}
}
Comments
6 pages, 4 figures, 2 tables, adding discussions on a fifth detector (LIGO-India), accepted by PRD (as a Rapid Communication)