Title Information
Title
"A Tale of 2-Spheres": How Conformal Symmetry, Chaos, and Some Elementary Algebra Led to Insights in Black Holes and Quantum Cosmology
Type of Resource (primo)
dissertations
Name: Personal
Name Part
Liu, Chang
Role
Role Term: Text
creator
Name: Personal
Name Part
Lowe, David
Role
Role Term: Text
Advisor
Name: Personal
Name Part
Jevicki, Antal
Role
Role Term: Text
Reader
Name: Personal
Name Part
Alexander, Stephon
Role
Role Term: Text
Reader
Name: Corporate
Name Part
Brown University. Department of Physics
Role
Role Term: Text
sponsor
Origin Information
Copyright Date
2022
Physical Description
Extent
xi, 64 p.
digitalOrigin
born digital
Note: thesis
Thesis (Ph. D.)--Brown University, 2022
Genre (aat)
theses
Abstract
The unification of quantum mechanics and general relativity is the holy grail of fundamental theoretical physics. This thesis represents a small part of that effort, where we consider a number of problems that might be of interest to the theoretical studies of black holes and quantum cosmology. Why study black holes and quantum cosmology, one might ask? The answer lies in the fact that they are the only two systems where it is necessary to apply quantum mechanics and general relativity simultaneously. In particular, they both have event horizons, which are global structures of the spacetime that prevent events from making causal contact. They therefore have become the primary arenas where logical incompatibilities of quantum mechanics and general relativity can be made most transparent. One of the most dramatic incompatibilities is the black hole information paradox, which concerns the unitarity of processes that involve the formation and the evaporation of black holes. This thesis will first discuss a proposed resolution to the information paradox called black hole complementarity, and a closely linked issue known as quantum scrambling, in particular in the context of a 2D conformal field theory. We will then present a microscopic quantum model of the de-Sitter universe that incorporates the required quantum scrambling on the cosmological horizon. This quantum model of cosmology is a so-called "holographic" map between the stretched horizon of the de-Sitter spacetime and the static patch (colloquially known as the "bulk"). Continuing in a similar vein, the rest of the thesis will be concerned with building holographic theories between flat spacetime and its boundary, and we present two holographic theories of the flat spacetime, first for massive scalar particles and then extending the results to gravitons. As these all have something to do with mappings between boundary 2-spheres and their bulk, this is therefore a story of building holography on 2-spheres. Hence the title of this thesis.
Subject (fast) (authorityURI="http://id.worldcat.org/fast", valueURI="http://id.worldcat.org/fast/01794284")
Topic
Theoretical physics
Subject (fast) (authorityURI="http://id.worldcat.org/fast", valueURI="http://id.worldcat.org/fast/01085110")
Topic
Quantum gravity
Language
Language Term (ISO639-2B)
English
Record Information
Record Content Source (marcorg)
RPB
Record Creation Date (encoding="iso8601")
20220706