Improved Bounds on Violation of the Strong Equivalence Principle

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dc.creatorArzoumanian, Z.
dc.date2002-12-07
dc.date.accessioned2026-07-07T02:06:46Z
dc.date.available2026-07-07T02:06:46Z
dc.descriptionI describe a unique, 20-year-long timing program for the binary pulsar B0655+64, the stalwart control experiment for measurements of gravitational radiation damping in relativistic neutron-star binaries. Observed limits on evolution of the B0655+64 orbit provide new bounds on the existence of dipolar gravitational radiation, and hence on violation of the Strong Equivalence Principle.
dc.description6 pages, 2 figures, to appear in proceedings: "Radio Pulsars," Chania, Crete, August 2002 (ASP conference series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0212180
dc.identifierhttp://arxiv.org/abs/astro-ph/0212180
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5477
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleImproved Bounds on Violation of the Strong Equivalence Principle
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