Título: | PHENOMENOLOGY OF NEUTRINOS AND PHYSICS BEYOND THE STANDARD MODEL | ||||||||||||
Autor: |
FABIO ALEX PEREIRA DOS SANTOS |
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Colaborador(es): |
HIROSHI NUNOKAWA - Orientador |
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Catalogação: | 03/DEZ/2012 | Língua(s): | PORTUGUESE - BRAZIL |
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Tipo: | TEXT | Subtipo: | THESIS | ||||||||||
Notas: |
[pt] Todos os dados constantes dos documentos são de inteira responsabilidade de seus autores. Os dados utilizados nas descrições dos documentos estão em conformidade com os sistemas da administração da PUC-Rio. [en] All data contained in the documents are the sole responsibility of the authors. The data used in the descriptions of the documents are in conformity with the systems of the administration of PUC-Rio. |
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Referência(s): |
[pt] https://www.maxwell.vrac.puc-rio.br/projetosEspeciais/ETDs/consultas/conteudo.php?strSecao=resultado&nrSeq=20782&idi=1 [en] https://www.maxwell.vrac.puc-rio.br/projetosEspeciais/ETDs/consultas/conteudo.php?strSecao=resultado&nrSeq=20782&idi=2 |
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DOI: | https://doi.org/10.17771/PUCRio.acad.20782 | ||||||||||||
Resumo: | |||||||||||||
With advances in the measurements of the neutrino oscillation
parameters, we can assume that neutrino physics is going to a precision
era, as a consequence we can explore new scenarios beyond the standard
mass and mixing with three neutrino flavors , that is, we can look for a new
physics that affects in a subleading way and that can not be explained by
the standard oscillation framework. For instance, the reactor antineutrino
and Gallium anomalies, both anomalies will be discussed in chapter 3.
We propose an explanation for these anomalies based on a scenario with
large extra dimension. We also explore the capability of an experiment
with ultramonochromatic neutrinos based on M ossbauer effect detects or
constrains some new physics scenarios beyond the standard model. In this
thesis we consider: sterile neutrinos, large extra dimensions, non standard
quantum decoherence and mass varying neutrinos. We also show the impact
on the determination of the standard oscillation parameters delta m2 31 and teta 13
if we assume non standard physics scenarios.
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