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We revisit gravitational wave (GW) memory as the key to measuring spacetime symmetries, extending beyond its traditional role in GW searches. In particular, we show how these symmetries may be probed via displacement and spin memory observations, respectively. We further find that the Einstein Telescope's (ET) sensitivity enables constraining the strain amplitude of a displacement memory to 2% and that of spin memory to 22%. Finally, we point out that neglecting memory could lead to an overestimation of measurement uncertainties for parameters of binary black hole (BBH) mergers by about 10% in ET.Received 29 December 2023Accepted 1 May 2024DOI:https://doi.org/10.1103/PhysRevLett.132.241401© 2024 American Physical SocietyPhysics Subject Headings (PhySH)Research AreasAstrophysical studies of gravityExperimental studies of gravityGeneral relativityGravitational wave detectionGravitational wave sourcesGravitational wavesPhysical SystemsAstronomical black holesPropertiesSpacetime symmetriesTechniquesGravitational wave detectorsGravitation, Cosmology & Astrophysics
Goncharov et al. (Thu,) studied this question.