Observational constraints in Delta Gravity : CMB and supernovas
dc.contributor.advisor | Alfaro Solís, Jorge Luis | |
dc.contributor.author | San Martín Hormazábal, Marco | |
dc.contributor.other | Pontificia Universidad Católica de Chile. Facultad de Física | |
dc.date.accessioned | 2021-01-07T14:25:41Z | |
dc.date.available | 2021-01-07T14:25:41Z | |
dc.date.issued | 2020 | |
dc.date.updated | 2021-01-05T22:54:36Z | |
dc.description | Tesis (Ph.D. in Astrophysics)--Pontificia Universidad Católica de Chile, 2020 | |
dc.description.abstract | I study the cosmological implications of Delta Gravity (DG), which is a gravitational model based on the extension of General Relativity (GR) by a new symmetry called δ ̃. In this model, new matter fields are added to the original matter fields, motivated by the additional symmetry. We call them δ ̃ matter fields. This theory predicts an accelerating Universe without introducing a Cosmological Constant Λ by hand in the equations. To test the Delta Gravity implications, I examine two critical observations in Cosmology: the rate of the Universe expansion through type Ia supernovae (SNe-Ia) and the power spectrum calculated from the cosmic microwave background radiation (CMB). To compare the observations with these model's predictions, I used a Markov Chain Monte Carlo (MCMC) analysis with the most updated SNe-Ia and Planck satellite data catalog. I obtain the fitted parameters needed to explain both SNe-Ia data and CMB measurements. I analyze the DG model's compatibility with both observations and constrain the cosmological parameters associated with the astrophysical evidence. Finally, I discuss if the Hubble Constant and the Accelerating Universe are compatible with the DG context's observational evidence. | |
dc.format.extent | xi, 178 páginas | |
dc.identifier.doi | 10.7764/tesisUC/FIS/50175 | |
dc.identifier.uri | https://doi.org/10.7764/tesisUC/FIS/50175 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/50175 | |
dc.language.iso | en | |
dc.nota.acceso | Contenido completo | |
dc.rights | acceso abierto | |
dc.subject.other | Radiación cósmica de fondo - Modelos matemáticos | es_ES |
dc.subject.other | Relatividad generalizada (Física) | es_ES |
dc.subject.other | Astrofísica - Modelos matemáticos | es_ES |
dc.title | Observational constraints in Delta Gravity : CMB and supernovas | es_ES |
dc.type | tesis doctoral | |
sipa.codpersvinculados | 49962 | |
sipa.codpersvinculados | 213497 |
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