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Classical Gravitational Bremsstrahlung from a Worldline Quantum Field Theory
Using the recently established formalism of a worldline quantum field theory description of the classical scattering of two spinless black holes, we compute the far-field time-domain waveform of the gravitational waves produced in the encounter at leading order in the post-Minkowskian (weak field bu...
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Published in: | Physical review letters 2021-05, Vol.126 (20), p.1-201103, Article 201103 |
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container_end_page | 201103 |
container_issue | 20 |
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container_title | Physical review letters |
container_volume | 126 |
creator | Jakobsen, Gustav Uhre Mogull, Gustav Plefka, Jan Steinhoff, Jan |
description | Using the recently established formalism of a worldline quantum field theory description of the classical scattering of two spinless black holes, we compute the far-field time-domain waveform of the gravitational waves produced in the encounter at leading order in the post-Minkowskian (weak field but generic velocity) expansion. We reproduce the previous results of Kovacs and Thorne in a highly economic way. Then, using the waveform, we extract the leading-order total radiated angular momentum and energy (including differential results). Our work may enable crucial improvements of gravitational-wave predictions in the regime of large relative velocities. |
doi_str_mv | 10.1103/PhysRevLett.126.201103 |
format | article |
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subjects | Angular momentum Bremsstrahlung Far fields Field theory Gravitational waves Quantum field theory Quantum theory Waveforms |
title | Classical Gravitational Bremsstrahlung from a Worldline Quantum Field Theory |
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