A model of the radiation emitted by a source in the vicinity of a Kerr black hole
dc.audience | generalPublic | es_MX |
dc.contributor | Silva Ortigoza, Gilberto | |
dc.contributor.advisor | SILVA ORTIGOZA, GILBERTO; 12295 | |
dc.contributor.author | González Juárez, Adriana | |
dc.creator | GONZALEZ JUAREZ, ADRIANA; 446473 | |
dc.date.accessioned | 2021-10-25T23:02:06Z | |
dc.date.available | 2021-10-25T23:02:06Z | |
dc.date.issued | 2021-06 | |
dc.description.abstract | “The present thesis is the study of: the physics that characterizes the Bessel beams, the behavior of the reected radiation by a parabolic mirror considering inclined incident light rays and Kirchho's diraction theory applied to the phenomenon of reection of light ray by a parabolic mirror, in particular that of the LMT/GTM antenna. It is shown that adiractional beams which are invariant under translations along the axis of propagation, are characterized by a family of wavefronts and a caustic, and it is found that the caustic qualitatively coincides with the absolute maximum of the intensity pattern. Then, expressions for: the incident light rays and wavefronts, the reected light rays, the reected wavefronts, the caustic and the ronchigram have been ob- tained; those general results are applied to the parameters of the antenna of the LMT/GTM and it is shown that the caustic has a singularity of the hyperbolic umbilic type, which is locally stable under small perturbations of the optical system. The results presented could be associated to the radiation of a static source, in the geometrical optics limit. Finally, an expression for the intensity pattern associated with the reection of a Bessel beam of order m by the LMT/GTM antenna has been determined; the preliminary results are presented”. | es_MX |
dc.folio | 20210812141006-8890-T | es_MX |
dc.format | es_MX | |
dc.identificator | 1 | es_MX |
dc.identifier.uri | https://hdl.handle.net/20.500.12371/14888 | |
dc.language.iso | eng | es_MX |
dc.matricula.creator | 217570103 | es_MX |
dc.rights.acces | openAccess | es_MX |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0 | es_MX |
dc.subject.classification | CIENCIAS FÍSICO MATEMÁTICAS Y CIENCIAS DE LA TIERRA | es_MX |
dc.subject.dbgunam | Astronomía--Observaciones | es_MX |
dc.subject.lcc | Óptica física | es_MX |
dc.subject.oclc | Large Millimeter Telescope | es_MX |
dc.subject.oclc | Haz de Bessel | es_MX |
dc.thesis.career | Doctorado en Ciencias (Física Aplicada) | es_MX |
dc.thesis.degreediscipline | Área de Ingeniería y Ciencias Exactas | es_MX |
dc.thesis.degreegrantor | Facultad de Ciencias Físico Matemáticas | es_MX |
dc.thesis.degreetoobtain | Doctor (a) en Ciencias (Física Aplicada) | es_MX |
dc.title | A model of the radiation emitted by a source in the vicinity of a Kerr black hole | es_MX |
dc.type | Tesis de doctorado | es_MX |
dc.type.conacyt | doctoralThesis | es_MX |
dc.type.degree | Doctorado | es_MX |
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