Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays

Detalhes bibliográficos
Autor(a) principal: Rodrigo Guedes Lang
Data de Publicação: 2021
Tipo de documento: Tese
Idioma: eng
Título da fonte: Biblioteca Digital de Teses e Dissertações da USP
Texto Completo: https://doi.org/10.11606/T.76.2021.tde-13052021-093011
Resumo: In this thesis, we use a phenomenological approach to the propagation of astroparticles in order to study two relevant topics in astrophysics: Lorentz invariance violation (LIV) and the origin of ultra-high energy cosmic rays (UHECR). Lorentz invariance is proposed as a fundamental symmetry of nature according to relativity. However, quantum gravity models assume or accommodate some level of LIV. We present a broad study of the potential of testing LIV with different data sets and experiments in astroparticle physics. Novel techniques are proposed for testing LIV using TeV gamma-ray and UHECR data, in special using data from Imaging Air Cherenkov Telescopes and the Pierre Auger Observatory. No signature of LIV is found and restraining limits are imposed. We present a review of the most common astrophysical tests and a compilation of the currently most restrictive limits of LIV. We also address the long-lasting question about the origin of UHECR. CR are charged particles and, thus, magnetic fields mask the information about the position of their sources. We study how the energy spectrum, composition and distribution of arrival directions can be used to retrieve information about the source distribution. Constraints on the maximum distance of the nearest UHECR source are imposed. We study the arising of a large-scale anisotropy in the form of a dipole measured by the Pierre Auger Observatory and build an understanding of the evolution with energy of the dipole strength.
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spelling info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesis Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays Fenomenologia da propagação de astropartículas: violação da invariância de Lorentz e a origem dos raios cósmicos de altíssima energia 2021-02-04Luiz Vitor de Souza FilhoRogério Menezes de AlmeidaJonathan BiteauKarl-heinz KampertEdivaldo Moura SantosRodrigo Guedes LangUniversidade de São PauloFísicaUSPBR Anisotropia Anisotropy Fontes de raios cósmicos de altíssima energia Gamma rays Lorentz invariance violation Raios cósmicos de altíssima energia Raios gama UHECR UHECR sources Violação da invariância de Lorentz In this thesis, we use a phenomenological approach to the propagation of astroparticles in order to study two relevant topics in astrophysics: Lorentz invariance violation (LIV) and the origin of ultra-high energy cosmic rays (UHECR). Lorentz invariance is proposed as a fundamental symmetry of nature according to relativity. However, quantum gravity models assume or accommodate some level of LIV. We present a broad study of the potential of testing LIV with different data sets and experiments in astroparticle physics. Novel techniques are proposed for testing LIV using TeV gamma-ray and UHECR data, in special using data from Imaging Air Cherenkov Telescopes and the Pierre Auger Observatory. No signature of LIV is found and restraining limits are imposed. We present a review of the most common astrophysical tests and a compilation of the currently most restrictive limits of LIV. We also address the long-lasting question about the origin of UHECR. CR are charged particles and, thus, magnetic fields mask the information about the position of their sources. We study how the energy spectrum, composition and distribution of arrival directions can be used to retrieve information about the source distribution. Constraints on the maximum distance of the nearest UHECR source are imposed. We study the arising of a large-scale anisotropy in the form of a dipole measured by the Pierre Auger Observatory and build an understanding of the evolution with energy of the dipole strength. Nesta tese, nós usamos um tratamento fenomenológico para a propagação de astropartículas com o intuito de estudar dois relevantes tópicos em astrofísica: violação da invariância de Lorentz (LIV, do inglês Lorentz invariance violation) e a origem de raios cósmicos de altíssima energia (UHECR, do inglês ultra-high energy cosmic rays). Em relatividade, a invariância de Lorentz é proposta como uma simetria fundamental da natureza. Todavia, modelos de gravitação quântica assumem ou acomodam um certo nível de LIV. Nós apresentamos um amplo estudo do potencial de se testar LIV com diferentes conjuntos de dados e experimentos em astrofísica de partículas. Técnicas inovadoras são propostas para testar LIV usando raios gama com energia da ordem de TeV e UHECR, em especial usando dados de telescópios atmosféricos de Cherenkov e do Observatório Pierre Auger. Nenhum sinal de LIV é encontrado e limites restritivos são impostos. Nós apresentamos uma revisão dos testes de LIV mais comuns em astrofísica de partículas e uma coleção dos limites de LIV mais restritivos da atualidade. Nós também tratamos a questão sobre a origem dos UHECR. Raios cósmicos são partículas carregadas e, portanto, campos magnéticos mascaram a informação sobre a posição de suas fontes. Nós estudamos como o espectro de energia, a composição e a distribuição de direções de chegada podem ser usados para recuperar a informação sobre a distribuição de fontes. Restrições na máxima distância da fonte mais próxima de UHECR são impostas. Nós estudamos o surgimento de uma anisotropia de larga escala na forma de um dipolo medida pelo Observatório Pierre Auger e desenvolvemos um entendimento da evolução com energia da intensidade desse dipolo. https://doi.org/10.11606/T.76.2021.tde-13052021-093011info:eu-repo/semantics/openAccessengreponame:Biblioteca Digital de Teses e Dissertações da USPinstname:Universidade de São Paulo (USP)instacron:USP2023-12-21T18:51:21Zoai:teses.usp.br:tde-13052021-093011Biblioteca Digital de Teses e Dissertaçõeshttp://www.teses.usp.br/PUBhttp://www.teses.usp.br/cgi-bin/mtd2br.plvirginia@if.usp.br|| atendimento@aguia.usp.br||virginia@if.usp.bropendoar:27212023-12-22T12:35:48.841382Biblioteca Digital de Teses e Dissertações da USP - Universidade de São Paulo (USP)false
dc.title.en.fl_str_mv Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
dc.title.alternative.pt.fl_str_mv Fenomenologia da propagação de astropartículas: violação da invariância de Lorentz e a origem dos raios cósmicos de altíssima energia
title Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
spellingShingle Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
Rodrigo Guedes Lang
title_short Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
title_full Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
title_fullStr Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
title_full_unstemmed Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
title_sort Phenomenology of the propagation of astroparticles: Lorentz invariance violation and the origin of ultra-high energy cosmic rays
author Rodrigo Guedes Lang
author_facet Rodrigo Guedes Lang
author_role author
dc.contributor.advisor1.fl_str_mv Luiz Vitor de Souza Filho
dc.contributor.referee1.fl_str_mv Rogério Menezes de Almeida
dc.contributor.referee2.fl_str_mv Jonathan Biteau
dc.contributor.referee3.fl_str_mv Karl-heinz Kampert
dc.contributor.referee4.fl_str_mv Edivaldo Moura Santos
dc.contributor.author.fl_str_mv Rodrigo Guedes Lang
contributor_str_mv Luiz Vitor de Souza Filho
Rogério Menezes de Almeida
Jonathan Biteau
Karl-heinz Kampert
Edivaldo Moura Santos
description In this thesis, we use a phenomenological approach to the propagation of astroparticles in order to study two relevant topics in astrophysics: Lorentz invariance violation (LIV) and the origin of ultra-high energy cosmic rays (UHECR). Lorentz invariance is proposed as a fundamental symmetry of nature according to relativity. However, quantum gravity models assume or accommodate some level of LIV. We present a broad study of the potential of testing LIV with different data sets and experiments in astroparticle physics. Novel techniques are proposed for testing LIV using TeV gamma-ray and UHECR data, in special using data from Imaging Air Cherenkov Telescopes and the Pierre Auger Observatory. No signature of LIV is found and restraining limits are imposed. We present a review of the most common astrophysical tests and a compilation of the currently most restrictive limits of LIV. We also address the long-lasting question about the origin of UHECR. CR are charged particles and, thus, magnetic fields mask the information about the position of their sources. We study how the energy spectrum, composition and distribution of arrival directions can be used to retrieve information about the source distribution. Constraints on the maximum distance of the nearest UHECR source are imposed. We study the arising of a large-scale anisotropy in the form of a dipole measured by the Pierre Auger Observatory and build an understanding of the evolution with energy of the dipole strength.
publishDate 2021
dc.date.issued.fl_str_mv 2021-02-04
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/doctoralThesis
format doctoralThesis
status_str publishedVersion
dc.identifier.uri.fl_str_mv https://doi.org/10.11606/T.76.2021.tde-13052021-093011
url https://doi.org/10.11606/T.76.2021.tde-13052021-093011
dc.language.iso.fl_str_mv eng
language eng
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Universidade de São Paulo
dc.publisher.program.fl_str_mv Física
dc.publisher.initials.fl_str_mv USP
dc.publisher.country.fl_str_mv BR
publisher.none.fl_str_mv Universidade de São Paulo
dc.source.none.fl_str_mv reponame:Biblioteca Digital de Teses e Dissertações da USP
instname:Universidade de São Paulo (USP)
instacron:USP
instname_str Universidade de São Paulo (USP)
instacron_str USP
institution USP
reponame_str Biblioteca Digital de Teses e Dissertações da USP
collection Biblioteca Digital de Teses e Dissertações da USP
repository.name.fl_str_mv Biblioteca Digital de Teses e Dissertações da USP - Universidade de São Paulo (USP)
repository.mail.fl_str_mv virginia@if.usp.br|| atendimento@aguia.usp.br||virginia@if.usp.br
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