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- W2786010987 abstract "We use the inspiral phase of the GW170814 gravitational wave event detected by the three LIGO-VIRGO observatories to study the polarization properties of the gravitational waves. We find that standard tensor polarization is able to explain the amplitude ratios among the three detectors for the LIGO-VIRGO maximum a posteriori gravitational wave source sky location. However, within the 90% credible region of sky locations, there is a range in which pure vector polarization is also consistent with the observed amplitude ratios. If vector polarization of gravitational waves is confirmed, this will open a new era of post-general relativity physics." @default.
- W2786010987 created "2018-02-23" @default.
- W2786010987 creator A5018269401 @default.
- W2786010987 date "2018-02-04" @default.
- W2786010987 modified "2023-09-27" @default.
- W2786010987 title "Gravitational Wave Polarization Analysis of GW170814" @default.
- W2786010987 hasPublicationYear "2018" @default.
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