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• W2891100029 abstract "Treating general relativity as an effective field theory, we compute the leading-order quantum corrections to the orbits and gravitational-wave emission of astrophysical compact binaries. These corrections are independent of the (unknown) nature of quantum gravity at high energies, and generate a phase shift and amplitude increase in the observed gravitational-wave signal. Unfortunately (but unsurprisingly), these corrections are undetectably small, even in the most optimistic observational scenarios." @default.
• W2891100029 created "2018-09-27" @default.
• W2891100029 creator A5011231754 @default.
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• W2891100029 date "2018-11-20" @default.
• W2891100029 modified "2023-10-03" @default.
• W2891100029 title "Can we detect quantum gravity with compact binary inspirals?" @default.
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• W2891100029 doi "https://doi.org/10.1103/physrevd.98.104032" @default.
• W2891100029 hasPublicationYear "2018" @default.
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