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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4220
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dc.contributor.authorKapoor, R. C-
dc.contributor.authorDatta, B-
dc.date.accessioned2008-12-30T14:04:15Z-
dc.date.available2008-12-30T14:04:15Z-
dc.date.issued1985-10-
dc.identifier.citationAstrophysical Journal, Part 1, Vol. 297, pp. 413 - 422en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/4220-
dc.description.abstractThe effects of spacetime curvature and rotation on the pulse profile of fast pulsars are studied using a rotationally perturbed spherical metric and a representative choice of the equation of state for neutron star matter. Spacetime curvature is found to produce a divergence in the pulse width and a deamplification of the pulse intensity. Rotation is found to produce an asymmetry in the final pulse profile accompanied by a tilt of the pulse cone axis from its original direction of emission. The astrophysical implications of these results pertaining to the pulse characteristics of fast pulsars are discussed.en
dc.language.isoenen
dc.publisherThe American Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1985ApJ...297..413Ken
dc.relation.urihttp://dx.doi.org/10.1086/163540en
dc.subjectEquations Of Stateen
dc.subjectPerturbation Theoryen
dc.subjectPulsarsen
dc.subjectRelativityen
dc.subjectSpace-Time Functionsen
dc.subjectNeutron Starsen
dc.subjectRed Shiften
dc.subjectStabilityen
dc.titleFast pulsars - Effects of spacetime curvature and rotation on the pulse characteristicsen
dc.typeArticleen
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