Constraints on Gravitational Dipole Radiation from Pulsars

Simple item page
dc.creatorSivaram, C.
dc.date2008-03-13
dc.date.accessioned2026-07-07T09:26:34Z
dc.date.available2026-07-07T09:26:34Z
dc.descriptionRecent suggestions for a modification of general relativity to provide an alternative approach to gravity in connection with the dark energy (matter) problem imply a long range vector component of the gravitational field. This could lead to emission of gravitational dipole emission from objects such as pulsars. Stringent observational limits on period changes of binary and millisecond pulsars and their consistency with general relativity impose severe limits on couplings of such forces. These bounds are tighter than those implied by lunar laser ranging experiments.
dc.description5 pages, 6 equations
dc.identifierhttps://arxiv.org/abs/0803.1896
dc.identifierhttp://arxiv.org/abs/0803.1896
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/156796
dc.subjectAstrophysics
dc.titleConstraints on Gravitational Dipole Radiation from Pulsars
dc.typetext

Files

Collections

arXiv