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dc.contributor.authorDúmet-Montoya, Habib S.pt_BR
dc.contributor.authorCaminha, Gabriel Bartoschpt_BR
dc.contributor.authorMoraes, Bruno Azevedo Lemospt_BR
dc.contributor.authorMakler, Martínpt_BR
dc.contributor.authorGill, Mandeep S. S.pt_BR
dc.contributor.authorSantiago, Basilio Xavierpt_BR
dc.date.accessioned2014-04-13T01:50:00Zpt_BR
dc.date.issued2013pt_BR
dc.identifier.issn0035-8711pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/93388pt_BR
dc.description.abstractThe perturbative approach (PA) introduced by Alard provides analytic solutions for gravitational arcs by solving the lens equation linearized around the Einstein ring solution. This is a powerful method for lens inversion and simulations in which it can be used, in principle, for generic lens models. In this paper, we aim to quantify the domain of validity of this method for three quantities derived from the linearized mapping: caustics, critical curves and the deformation cross-section (i.e. the arc cross-section in the infinitesimal circular source approximation). We consider lens models with elliptical potentials, in particular the singular isothermal elliptic potential and pseudo-elliptical Navarro–Frenk–White models. We show that the PA is exact for this first model. For the second, we obtain constraints on the model parameter space (given by the potential ellipticity parameter ε and characteristic convergence κs) such that the PA is accurate for the aforementioned quantities. In this process, we obtain analytic expressions for several lensing functions, which are valid for the PA in general. The determination of this domain of validity could have significant implications for the use of the PA, but it still needs to be probed with extended sources.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofMonthly notices of the royal astronomical society. Oxford. Vol. 433, no. 4 (Aug. 2013), p. 2975-2985pt_BR
dc.rightsOpen Accessen
dc.subjectGravitational lensing: strongen
dc.subjectGaláxiaspt_BR
dc.subjectMatéria escurapt_BR
dc.subjectGalaxies: clusters: generalen
dc.subjectLentes gravitacionaispt_BR
dc.subjectDark matteren
dc.titleOn the accuracy of the perturbative approach for strong lensing : local distortion for pseudo-elliptical modelspt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000903105pt_BR
dc.type.originEstrangeiropt_BR


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