Small-eccentricity binary pulsars and relativistic gravity

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dc.creatorWex, N.
dc.date2000-02-07
dc.date.accessioned2026-07-07T03:24:45Z
dc.date.available2026-07-07T03:24:45Z
dc.descriptionSmall-eccentricity binary pulsars with white dwarf companions provide excellent test laboratories for various effects predicted by alternative theories of gravity, in particular tests for the emission of gravitational dipole radiation and the existence of gravitational Stark effects. We will present new limits to these effects. The statistical analysis presented here, for the first time, takes appropriately care of selection effects.
dc.description4 pages, to be published in Proc. of IAU Colloq. 177, "Pulsar Astronomy - 2000 and Beyond", eds. M. Kramer, N. Wex & R. Wielebinski
dc.identifierhttps://arxiv.org/abs/gr-qc/0002032
dc.identifierhttp://arxiv.org/abs/gr-qc/0002032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33453
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSmall-eccentricity binary pulsars and relativistic gravity
dc.typetext

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