Gyroscopic gravitational memory

Abstract We study the motion of a gyroscope located far away from an isolated gravitational source in an asymptotically flat spacetime. As seen from a local frame tied to distant stars, the gyroscope precesses when gravitational waves cross its path, resulting in a net ‘orientation memory’ that carr...

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Main Authors: Ali Seraj, Blagoje Oblak
Format: Article
Language:English
Published: SpringerOpen 2023-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP11(2023)057
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author Ali Seraj
Blagoje Oblak
author_facet Ali Seraj
Blagoje Oblak
author_sort Ali Seraj
collection DOAJ
description Abstract We study the motion of a gyroscope located far away from an isolated gravitational source in an asymptotically flat spacetime. As seen from a local frame tied to distant stars, the gyroscope precesses when gravitational waves cross its path, resulting in a net ‘orientation memory’ that carries information on the wave profile. At leading order in the inverse distance to the source, the memory consists of two terms: the first is linear in the metric perturbation and coincides with the spin memory effect, while the second is quadratic and measures the net helicity of the wave burst. Both are closely related to symmetries of the gravitational radiative phase space at null infinity: spin memory probes superrotation charges, while helicity is the canonical generator of local electric-magnetic duality on the celestial sphere.
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spelling doaj.art-5ac22c7ba4384fcbb1884845567a066d2024-04-21T11:05:46ZengSpringerOpenJournal of High Energy Physics1029-84792023-11-0120231112410.1007/JHEP11(2023)057Gyroscopic gravitational memoryAli Seraj0Blagoje Oblak1Centre for Gravitational Waves, Université Libre de Bruxelles, International Solvay InstitutesCPHT, CNRS, Ecole Polytechnique, IP ParisAbstract We study the motion of a gyroscope located far away from an isolated gravitational source in an asymptotically flat spacetime. As seen from a local frame tied to distant stars, the gyroscope precesses when gravitational waves cross its path, resulting in a net ‘orientation memory’ that carries information on the wave profile. At leading order in the inverse distance to the source, the memory consists of two terms: the first is linear in the metric perturbation and coincides with the spin memory effect, while the second is quadratic and measures the net helicity of the wave burst. Both are closely related to symmetries of the gravitational radiative phase space at null infinity: spin memory probes superrotation charges, while helicity is the canonical generator of local electric-magnetic duality on the celestial sphere.https://doi.org/10.1007/JHEP11(2023)057Classical Theories of GravityDuality in Gauge Field TheoriesSpace-Time SymmetriesGauge Symmetry
spellingShingle Ali Seraj
Blagoje Oblak
Gyroscopic gravitational memory
Journal of High Energy Physics
Classical Theories of Gravity
Duality in Gauge Field Theories
Space-Time Symmetries
Gauge Symmetry
title Gyroscopic gravitational memory
title_full Gyroscopic gravitational memory
title_fullStr Gyroscopic gravitational memory
title_full_unstemmed Gyroscopic gravitational memory
title_short Gyroscopic gravitational memory
title_sort gyroscopic gravitational memory
topic Classical Theories of Gravity
Duality in Gauge Field Theories
Space-Time Symmetries
Gauge Symmetry
url https://doi.org/10.1007/JHEP11(2023)057
work_keys_str_mv AT aliseraj gyroscopicgravitationalmemory
AT blagojeoblak gyroscopicgravitationalmemory