A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations

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Cosmic Rays have come to play an important role in understanding the universe, and astroparticle physics has undergone major developments in the last few decades. As such, several observatories have been set up with the purpose of detecting these particles, and simulation frameworks have been develo...

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Detalles Bibliográficos
Autor: Olivares Schneider, José Gabriel
Formato: tesis de grado
Fecha de Publicación:2021
Institución:Pontificia Universidad Católica del Perú
Repositorio:PUCP-Tesis
Lenguaje:inglés
OAI Identifier:oai:tesis.pucp.edu.pe:20.500.12404/18220
Enlace del recurso:http://hdl.handle.net/20.500.12404/18220
Nivel de acceso:acceso abierto
Materia:Partículas (Física nuclear)
Rayos cósmicos
https://purl.org/pe-repo/ocde/ford#1.03.00
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dc.title.es_ES.fl_str_mv A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
title A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
spellingShingle A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
Olivares Schneider, José Gabriel
Partículas (Física nuclear)
Rayos cósmicos
https://purl.org/pe-repo/ocde/ford#1.03.00
title_short A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
title_full A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
title_fullStr A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
title_full_unstemmed A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
title_sort A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulations
author Olivares Schneider, José Gabriel
author_facet Olivares Schneider, José Gabriel
author_role author
dc.contributor.advisor.fl_str_mv Bazo Alba, José Luis
dc.contributor.author.fl_str_mv Olivares Schneider, José Gabriel
dc.subject.es_ES.fl_str_mv Partículas (Física nuclear)
Rayos cósmicos
topic Partículas (Física nuclear)
Rayos cósmicos
https://purl.org/pe-repo/ocde/ford#1.03.00
dc.subject.ocde.es_ES.fl_str_mv https://purl.org/pe-repo/ocde/ford#1.03.00
description Cosmic Rays have come to play an important role in understanding the universe, and astroparticle physics has undergone major developments in the last few decades. As such, several observatories have been set up with the purpose of detecting these particles, and simulation frameworks have been developed in order to further analyze their behavior by creating highly variable environments and parameters. This work covers the essential theory required to study propagation of Ultra- High-Energy Cosmic Rays restricted to linear one-dimensional propagation only; this includes the primary methods of energy loss during propagation, mainly through reactions with the photon background like photo-pion production and photo-disintegration, and additional cosmological effects. The study was done using the CRPropa 3.0 simulation framework. To determine the best possible maximum energy for the simulations, initial trials were done by testing the GZK cutoff for multiple energy values, followed by an analysis of heavier nuclei propagation. As a final complete test run, a model of the cosmic ray spectrum for energies above 1018 eV was made based on two data sets, one made from the average composition of the whole CR energy spectrum, and the other from The Pierre-Auger Observatory measurements for the high energy range. The results showed that initial source composition was the determining factor in the shape of the CR spectrum. These initial simulations done in this work will set the ground for future more complex simulations and studies.
publishDate 2021
dc.date.accessioned.none.fl_str_mv 2021-02-16T00:52:07Z
dc.date.available.none.fl_str_mv 2021-02-16T00:52:07Z
dc.date.created.none.fl_str_mv 2021
dc.date.issued.fl_str_mv 2021-02-15
dc.type.es_ES.fl_str_mv info:eu-repo/semantics/bachelorThesis
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dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12404/18220
url http://hdl.handle.net/20.500.12404/18220
dc.language.iso.es_ES.fl_str_mv eng
language eng
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dc.publisher.es_ES.fl_str_mv Pontificia Universidad Católica del Perú
dc.publisher.country.es_ES.fl_str_mv PE
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spelling Bazo Alba, José LuisOlivares Schneider, José Gabriel2021-02-16T00:52:07Z2021-02-16T00:52:07Z20212021-02-15http://hdl.handle.net/20.500.12404/18220Cosmic Rays have come to play an important role in understanding the universe, and astroparticle physics has undergone major developments in the last few decades. As such, several observatories have been set up with the purpose of detecting these particles, and simulation frameworks have been developed in order to further analyze their behavior by creating highly variable environments and parameters. This work covers the essential theory required to study propagation of Ultra- High-Energy Cosmic Rays restricted to linear one-dimensional propagation only; this includes the primary methods of energy loss during propagation, mainly through reactions with the photon background like photo-pion production and photo-disintegration, and additional cosmological effects. The study was done using the CRPropa 3.0 simulation framework. To determine the best possible maximum energy for the simulations, initial trials were done by testing the GZK cutoff for multiple energy values, followed by an analysis of heavier nuclei propagation. As a final complete test run, a model of the cosmic ray spectrum for energies above 1018 eV was made based on two data sets, one made from the average composition of the whole CR energy spectrum, and the other from The Pierre-Auger Observatory measurements for the high energy range. The results showed that initial source composition was the determining factor in the shape of the CR spectrum. These initial simulations done in this work will set the ground for future more complex simulations and studies.Los rayos cósmicos juegan un papel importante en nuestro entendimiento del universo, por eso, la física de astropartículas ha sido desarrollada en gran medida en estas últimas décadas. Varios observatorios han sido construidos con el propósito de detectar estas partículas, y a su vez se han desarrollado programas de simulaciones para analizar su comportamiento usando ambientes y variables con una alta variabilidad. Este trabajo cubre la teoría necesaria para estudiar la propagación de rayos cósmicos de ultra-altas energías restringido a una sola dimensión; esto incluye las principales causas de pérdida de energía durante su propagación, principalmente a través de interacciones con el fondo de fotones como la fotoproducción de piones y fotodesintegración, así como otros efectos cosmológicos. Este estudio fue realizado con el programa de simulaciones CRPropa 3.0. Para determinar la mejor energía máxima para las simulaciones, los primeros ensayos comprobaron el límite GZK para múltiples valores de energía, seguido de un análisis de la propagación de núcleos más pesados. A manera de ensayo final, un modelo del espectro de rayos cósmicos para energías mayores a 1018 eV fue hecho basado en dos grupos de datos, uno a partir de la composición general promedio de todo el espectro de energías de los rayos cósmicos, y el otro a partir de mediciones hechas por el observatorio Pierre-Auger para altas energías. Los resultados muestran que la composición inicial de la fuente es el factor determinante en la forma del espectro. Las simulaciones iniciales hechas en este trabajo serán utilizadas como base para futuras y más complejas investigaciones.engPontificia Universidad Católica del PerúPEinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc/2.5/pe/Partículas (Física nuclear)Rayos cósmicoshttps://purl.org/pe-repo/ocde/ford#1.03.00A study of Ultra-High-Energy Cosmic Ray propagation in one-dimensional simulationsinfo:eu-repo/semantics/bachelorThesisreponame:PUCP-Tesisinstname:Pontificia Universidad Católica del Perúinstacron:PUCPSUNEDUBachiller en Ciencias con mención en FísicaBachilleratoPontificia Universidad Católica del Perú. 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