Poisson equation for weak gravitational lensing

dc.creatorKling, Thomas P.
dc.creatorCampbell, Bryan
dc.date2008-06-17
dc.date.accessioned2026-07-07T11:33:55Z
dc.date.available2026-07-07T11:33:55Z
dc.descriptionUsing the Newman and Penrose spin coefficient (NP) formalism, we examine the full Bianchi identities of general relativity in the context of gravitational lensing, where the matter and space-time curvature are projected into a lens plane perpendicular to the line of sight. From one component of the Bianchi identity, we provide a rigorous, new derivation of a Poisson equation for the projected matter density where the source term involves second derivatives of the observed weak gravitational lensing shear. We also show that the other components of the Bianchi identity reveal no new results. Numerical integration of the Poisson equation in test cases shows an accurate mass map can be constructed from the combination of a ground-based, wide-field image and a Hubble Space Telescope image of the same system.
dc.descriptionaccepted to Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/0806.2834
dc.identifierhttp://arxiv.org/abs/0806.2834
dc.identifierPhys.Rev.D77:123012,2008
dc.identifierdoi:10.1103/PhysRevD.77.123012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198068
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titlePoisson equation for weak gravitational lensing
dc.typetext

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