Study of the delta-cp dependence of astrophysical neutrino oscillations
This work presents a formalism for computing the neutrino time evolution operator in the general case for when the neutrinos travel through a medium of varying density. This takes up Chapter 2. The following chapter studies the relevant considerations for when evolution of the neutrinos through the...
- Autores:
-
Aguirre Lamus, Santiago
- Tipo de recurso:
- Trabajo de grado de pregrado
- Fecha de publicación:
- 2017
- Institución:
- Universidad de los Andes
- Repositorio:
- Séneca: repositorio Uniandes
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.uniandes.edu.co:1992/61473
- Acceso en línea:
- http://hdl.handle.net/1992/61473
- Palabra clave:
- Astrofísica de neutrinos
Neutrinos
Partículas (Física nuclear)
- Rights
- openAccess
- License
- http://creativecommons.org/licenses/by-nc-sa/4.0/
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Al consultar y hacer uso de este recurso, está aceptando las condiciones de uso establecidas por los autores.http://creativecommons.org/licenses/by-nc-sa/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Sanabria Arenas, Juan Carlosvirtual::7859-1Aguirre Lamus, Santiago49d8d1ce-3ccd-4bc3-873b-e9e91dab3271500Reyes Lega, Andrés Fernando2022-09-26T22:22:10Z2022-09-26T22:22:10Z2017http://hdl.handle.net/1992/61473instname:Universidad de los Andesreponame:Repositorio Institucional Sénecarepourl:https://repositorio.uniandes.edu.co/795172-1001This work presents a formalism for computing the neutrino time evolution operator in the general case for when the neutrinos travel through a medium of varying density. This takes up Chapter 2. The following chapter studies the relevant considerations for when evolution of the neutrinos through the Earth is considered. This provides understanding of the important phenomena that will be taken into account in Chapter 4, for when time evolution through the Earth is taken to calculate the muon-track to shower ratio as function of delta-CP.These results are analysed in Chapter 5, where the behaviour of the obtained plots is studied and the feasibility of measuring delta-CP experimentally is explored. The concluding remarks of the thesis are summarised in Chapter 6.El presente trabajo presenta un formalismo para calcular el operador de evolución temporal de los neutrinos para el caso general en el que estos viajan a través de un medio de densidad variable. Esto comprende el Capítulo 2. El siguiente capítulo estudia las consideraciones relevantes para cuando se considera la evolución de neutrinos a través de la Tierra. Esto provee entendimiento de los fenónemos importantes que serán tenidos en cuenta en el Capítulo 4, donde la evolución temporal a través de la Tierra es tomada para calcular la razón entre muon-"tracks" y lluvias como función de delta-CP . Estos resultados son analizados en el Capítulo 5, donde se estudia el comportamiento de las gráficas obtenidas y se explora la posibilidad de medir delta-CP experimentalmente. Las observaciones finales de la tesis están resumidas en el Capítulo 6.FísicoPregrado61 hojasapplication/pdfengUniversidad de los AndesFísicaFacultad de CienciasDepartamento de FísicaStudy of the delta-cp dependence of astrophysical neutrino oscillationsTrabajo de grado - Pregradoinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_7a1fTexthttp://purl.org/redcol/resource_type/TPAstrofísica de neutrinosNeutrinosPartículas (Física nuclear)201223615Publication2e3cac64-ccc2-42c3-b3f9-2ef8e094ba71virtual::7859-12e3cac64-ccc2-42c3-b3f9-2ef8e094ba71virtual::7859-1https://scienti.minciencias.gov.co/cvlac/visualizador/generarCurriculoCv.do?cod_rh=0000008419virtual::7859-1ORIGINAL12786.pdfapplication/pdf1081213https://repositorio.uniandes.edu.co/bitstreams/71522b66-33c8-47c6-bd76-3cd66eb6a923/download9255013b8d7a1f3fe470ff3f80382d51MD51THUMBNAIL12786.pdf.jpg12786.pdf.jpgIM Thumbnailimage/jpeg5354https://repositorio.uniandes.edu.co/bitstreams/c6565520-7350-4400-b6ce-44f0312d5d43/downloadbaf66ba1b41b2852332b588520cae4dbMD53TEXT12786.pdf.txt12786.pdf.txtExtracted texttext/plain84939https://repositorio.uniandes.edu.co/bitstreams/598e2927-92fb-4f4f-9c84-ac03628c0017/download3f185032ec032c352516ad537990aa89MD521992/61473oai:repositorio.uniandes.edu.co:1992/614732024-03-13 13:32:09.445http://creativecommons.org/licenses/by-nc-sa/4.0/open.accesshttps://repositorio.uniandes.edu.coRepositorio institucional Sénecaadminrepositorio@uniandes.edu.co |
dc.title.spa.fl_str_mv |
Study of the delta-cp dependence of astrophysical neutrino oscillations |
title |
Study of the delta-cp dependence of astrophysical neutrino oscillations |
spellingShingle |
Study of the delta-cp dependence of astrophysical neutrino oscillations Astrofísica de neutrinos Neutrinos Partículas (Física nuclear) |
title_short |
Study of the delta-cp dependence of astrophysical neutrino oscillations |
title_full |
Study of the delta-cp dependence of astrophysical neutrino oscillations |
title_fullStr |
Study of the delta-cp dependence of astrophysical neutrino oscillations |
title_full_unstemmed |
Study of the delta-cp dependence of astrophysical neutrino oscillations |
title_sort |
Study of the delta-cp dependence of astrophysical neutrino oscillations |
dc.creator.fl_str_mv |
Aguirre Lamus, Santiago |
dc.contributor.advisor.none.fl_str_mv |
Sanabria Arenas, Juan Carlos |
dc.contributor.author.none.fl_str_mv |
Aguirre Lamus, Santiago |
dc.contributor.jury.none.fl_str_mv |
Reyes Lega, Andrés Fernando |
dc.subject.keyword.spa.fl_str_mv |
Astrofísica de neutrinos Neutrinos Partículas (Física nuclear) |
topic |
Astrofísica de neutrinos Neutrinos Partículas (Física nuclear) |
description |
This work presents a formalism for computing the neutrino time evolution operator in the general case for when the neutrinos travel through a medium of varying density. This takes up Chapter 2. The following chapter studies the relevant considerations for when evolution of the neutrinos through the Earth is considered. This provides understanding of the important phenomena that will be taken into account in Chapter 4, for when time evolution through the Earth is taken to calculate the muon-track to shower ratio as function of delta-CP.These results are analysed in Chapter 5, where the behaviour of the obtained plots is studied and the feasibility of measuring delta-CP experimentally is explored. The concluding remarks of the thesis are summarised in Chapter 6. |
publishDate |
2017 |
dc.date.issued.spa.fl_str_mv |
2017 |
dc.date.accessioned.none.fl_str_mv |
2022-09-26T22:22:10Z |
dc.date.available.none.fl_str_mv |
2022-09-26T22:22:10Z |
dc.type.spa.fl_str_mv |
Trabajo de grado - Pregrado |
dc.type.driver.spa.fl_str_mv |
info:eu-repo/semantics/bachelorThesis |
dc.type.version.spa.fl_str_mv |
info:eu-repo/semantics/acceptedVersion |
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http://purl.org/coar/resource_type/c_7a1f |
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Text |
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http://purl.org/redcol/resource_type/TP |
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http://purl.org/coar/resource_type/c_7a1f |
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acceptedVersion |
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http://hdl.handle.net/1992/61473 |
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instname:Universidad de los Andes |
dc.identifier.reponame.spa.fl_str_mv |
reponame:Repositorio Institucional Séneca |
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repourl:https://repositorio.uniandes.edu.co/ |
dc.identifier.local.spa.fl_str_mv |
795172-1001 |
url |
http://hdl.handle.net/1992/61473 |
identifier_str_mv |
instname:Universidad de los Andes reponame:Repositorio Institucional Séneca repourl:https://repositorio.uniandes.edu.co/ 795172-1001 |
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eng |
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dc.rights.uri.*.fl_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ |
dc.rights.accessrights.spa.fl_str_mv |
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http://purl.org/coar/access_right/c_abf2 |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ http://purl.org/coar/access_right/c_abf2 |
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openAccess |
dc.format.extent.spa.fl_str_mv |
61 hojas |
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application/pdf |
dc.publisher.spa.fl_str_mv |
Universidad de los Andes |
dc.publisher.program.spa.fl_str_mv |
Física |
dc.publisher.faculty.spa.fl_str_mv |
Facultad de Ciencias |
dc.publisher.department.spa.fl_str_mv |
Departamento de Física |
institution |
Universidad de los Andes |
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