Shock waves from black holes

dc.contributor.advisorWilson‑Ewing, Edward
dc.contributor.authorSantacruz, Robert
dc.date.accessioned2023-11-08T14:54:35Z
dc.date.available2023-11-08T14:54:35Z
dc.date.issued2023-02
dc.description.abstractBlack holes are among the most interesting objects in the universe. While in the classical description of gravity (general relativity) these objects contain singular points in which the theory breaks down, it is expected that these problematic points are avoided in a quantum theory of gravity. In this thesis, I present two different models based on an effective description of loop quantum gravity: a vacuum description of black holes and an extension for matter collapse. The study of the vacuum model is presented in Chapter 2 and the matter collapse is described in Chapters 3, as a first point of contact, and 4, which contains a more detailed analysis in both analytic and numerical calculations. The features and predictions that these models offer are several: i) provide a comprehensive evolution of dust matter collapse; ii) present a bounce after the contracting phase of matter; iii) predict the disappearance of the black hole and the emission of a shockwave; iv) determine the lifetime of the black hole to be proportional to its mass squared.
dc.description.copyright© Robert Santacruz, 2023
dc.format.extentx, 203
dc.format.mediumelectronic
dc.identifier.oclc(OCoLC)1419555266en
dc.identifier.otherThesis 11185en
dc.identifier.urihttps://unbscholar.lib.unb.ca/handle/1882/37530
dc.language.isoen
dc.publisherUniversity of New Brunswick
dc.rightshttp://purl.org/coar/access_right/c_abf2
dc.subject.disciplineMathematics and Statistics
dc.subject.lcshBlack holes (Astronomy)en
dc.subject.lcshShock waves.en
dc.subject.lcshQuantum gravity.en
dc.titleShock waves from black holes
dc.typedoctoral thesis
oaire.license.conditionother
thesis.degree.disciplineMathematics and Statistics
thesis.degree.grantorUniversity of New Brunswick
thesis.degree.leveldoctorate
thesis.degree.namePh.D.

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