2019
DOI: 10.1103/physrevd.100.104036
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Abstract: The detection of gravitational waves by Advanced LIGO and Advanced Virgo provides an opportunity to test general relativity in a regime that is inaccessible to traditional astronomical observations and laboratory tests. We present four tests of the consistency of the data with binary black hole gravitational waveforms predicted by general relativity. One test subtracts the best-fit waveform from the data and checks the consistency of the residual with detector noise. The second test checks the consistency of t… Show more

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Cited by 889 publications
(1,242 citation statements)
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References 128 publications
(247 reference statements)
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“…We can use the inverse of these equations (see Eqs. (7.13)) to express V 2 and Y 2 in terms of V m0(2) and V mk (2) . When expanding to second order our basic field equations E 1 -E 5 ,(5.17)-(5.21), we first get algebraic equations for F 2 and Λ 2 of the form…”
Section: Second Order Perturbationsmentioning
confidence: 99%
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“…We can use the inverse of these equations (see Eqs. (7.13)) to express V 2 and Y 2 in terms of V m0(2) and V mk (2) . When expanding to second order our basic field equations E 1 -E 5 ,(5.17)-(5.21), we first get algebraic equations for F 2 and Λ 2 of the form…”
Section: Second Order Perturbationsmentioning
confidence: 99%
“…where the second-order source terms S m0 (2) and S mk (2) consist of terms bilinear in V 1 , Y 1 , F 1 , Λ 1 , together with additional contributions linear in the pressure P 2 (remembering that P is second-order, see section VII). We recall that P 2 is obtained by solving the matter equation…”
Section: Second Order Perturbationsmentioning
confidence: 99%
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