Gravitational Radiation in Quantum Gravity
arXiv:1809.07606 · doi:10.1140/epjc/s10052-018-6265-3
Abstract
The effective field theory of quantum gravity generically predicts non-locality to be present in the effective action, which results from the low-energy propagation of gravitons and massless matter. Working to second order in gravitational curvature, we reconsider the effects of quantum gravity on the gravitational radiation emitted from a binary system. In particular, we calculate for the first time the leading order quantum gravitational correction to the classical quadrupole radiation formula which appears at second order in Newton's constant.
References in corpus (17)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- General relativity as an effective field theory: The leading quantum corrections
- Quantum Corrections to the Schwarzschild and Kerr Metrics
- Non-local quantum effects in cosmology 1: Quantum memory, non-local FLRW equations and singularity avoidance
- Scale of Quantum Gravity
- One-loop gravitational wave spectrum in de Sitter spacetime
- Quantum Corrections to Schwarzschild Black Hole
- On the covariant formalism of the effective field theory of gravity and leading order corrections
- The Lightest of Black Holes
- Gravitational Effective Action at Second Order in Curvature and Gravitational Waves
- Graviton propagator, renormalization scale and black-hole like states
- Particle creation in the effective action method
- Three Waves for Quantum Gravity
- A renormalization group improved non-local gravitational effective Lagrangian
- Dark Matter in Quantum Gravity
- What is the final state of a black hole merger?
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