On the time delay in binary systems

dc.creatorTartaglia, Angelo
dc.creatorRuggiero, Matteo Luca
dc.creatorNagar, Alessandro
dc.date2005-01-19
dc.date2005-01-28
dc.date.accessioned2026-07-07T06:38:11Z
dc.date.available2026-07-07T06:38:11Z
dc.descriptionThe aim of this paper is to study the time delay on electromagnetic signals propagating across a binary stellar system. We focus on the antisymmetric gravitomagnetic contribution due to the angular momentum of one of the stars of the pair. Considering a pulsar as the source of the signals, the effect would be manifest both in the arrival times of the pulses and in the frequency shift of their Fourier spectra. We derive the appropriate formulas and we discuss the influence of different configurations on the observability of gravitomagnetic effects. We argue that the recently discovered PSR J0737-3039 binary system does not permit the detection of the effects because of the large size of the eclipsed region.
dc.description7 pages, 2 eps figures, RevTex, to appear in Physical Review D
dc.identifierhttps://arxiv.org/abs/gr-qc/0501059
dc.identifierhttp://arxiv.org/abs/gr-qc/0501059
dc.identifierPhys.Rev. D71 (2005) 023003
dc.identifierdoi:10.1103/PhysRevD.71.023003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/100650
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleOn the time delay in binary systems
dc.typetext

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