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dc.contributor.advisorAscasibar Sequeiros, Yago 
dc.contributor.advisorMollá Lorente, Mercedes
dc.contributor.authorRomero Calleja, Mario 
dc.contributor.otherUAM. Departamento de Física Teóricaes_ES
dc.date.accessioned2022-11-07T07:52:16Z
dc.date.available2022-11-07T07:52:16Z
dc.date.issued2022-09-29
dc.identifier.urihttp://hdl.handle.net/10486/705025
dc.descriptionTesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 29 -09-2022es_ES
dc.descriptionEsta tesis tiene embargado el acceso al texto completo hasta el 29-03-2024es_ES
dc.description.abstractGalaxy formation and evolution involve several physical processes where stars, gas and dust play important roles. While analytical and numerical models have successfully accounted for most of them over the years, radiative transfer, that considers the interaction between light and the interstellar medium, is still the elephant in the room. Despite its importance as a driver of galactic evolution and as one of the main observables, radiation is often treated under very restrictive assumptions because an on-the-fy radiative transfer prescription is computationally expensive. This thesis advocates the importance and feasibility of including radiation by developing several models and codes with modest computational requirements. To illustrate this, I include radiation felds into the well-studied problem of supernova remnant evolution to study its efects, highlighting the main diferences and improvements with respect to previous works in the literature. Then, I model the interstellar radiation feld of the Milky Way in a self-consistent way, based on a distribution of stars, gas and dust predicted by chemical evolution models. This opens the door to use the interstellar radiation feld both as a prediction to calibrate evolutionary galaxy models, as well as an efcient method to consider this ingredient on other physical processes, as done with supernova remnantsen_US
dc.format.extent87 pag.es_ES
dc.format.mimetypeapplication/pdfen_US
dc.language.isoengen_US
dc.subject.otherGalaxiases_ES
dc.subject.otherSupernovases_ES
dc.subject.otherRadiaciónes_ES
dc.titleAnalytical and numerical model of radiative transfer in galaxiesen_US
dc.title.alternativeModelos analíticos y numéricos de transporte radiativo en galaxiases_ES
dc.typedoctoralThesisen_US
dc.subject.ecienciaFísicaes_ES
dc.date.embargoend2024-03-29
dc.rights.ccReconocimiento – NoComercial – SinObraDerivadaes_ES
dc.rights.accessRightsopenAccessen_US
dc.facultadUAMFacultad de Cienciases_ES


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