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- W2995890342 abstract "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 becomes possible in principle. The possibility of such a direct test is thus higher than an earlier expectation (Hagihara et al., Phys. Rev. D 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." @default.
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- W2995890342 date "2020-02-28" @default.
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- W2995890342 title "Condition for directly testing scalar modes of gravitational waves by four detectors" @default.
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- W2995890342 doi "https://doi.org/10.1103/physrevd.101.041501" @default.
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