Classical and quantum gravity with Ashtekar variables

This thesis is a study of classical and quantum gravity with Ashtekar variables. The Ashtekar constraints are shown to capture the essence of the constraints and constraint algebra of General Relativity in four dimensions. A classification scheme of the solution space of the Ashtekar constraints is...

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Main Author: Soo, Chopin
Other Authors: Physics
Format: Others
Language:en
Published: Virginia Tech 2014
Subjects:
Online Access:http://hdl.handle.net/10919/38626
http://scholar.lib.vt.edu/theses/available/etd-06192006-125720/
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spelling ndltd-VTETD-oai-vtechworks.lib.vt.edu-10919-386262021-12-15T05:57:34Z Classical and quantum gravity with Ashtekar variables Soo, Chopin Physics LD5655.V856 1992.S671 Gravity Quantum gravity This thesis is a study of classical and quantum gravity with Ashtekar variables. The Ashtekar constraints are shown to capture the essence of the constraints and constraint algebra of General Relativity in four dimensions. A classification scheme of the solution space of the Ashtekar constraints is proposed and the corresponding physics is investigated. The manifestly covariant equations of motion for the Ashtekar variables are derived. Explicit examples are discussed and new classical solutions of General Relativity are constructed by exploiting the properties of the Ashtekar variables. Non-perturbative canonical quantization of the theory is performed. The ordering of the quantum constraints as well as the formal closure of the quantum constraint algebra are explored. A detailed Becchi-Rouet-Stora-Tyutin (BRST) analysis of the theory is given. The results demonstrate explicitly that in quantum gravity, fluctuations in topology can occur and there are strong evidences of phases in the theory. There is a phase which is described by a topological quantum field theory (TQFT) of the Donaldson-Witten type and an Abelian antiinstanton phase wherein self-interactions of the gravitational fields produce symmetry breaking from SO(3) to U(1). The full theory is much richer and includes fluctuations which bring the system out of the various restricted sectors while preserving diffeomorphism invariance. Invariants of the quantum theory with are constructed through BRST descents. They provide a clear and systematic characterization of non-local observables in quantum gravity, and can yield further differential invariants of four-manifolds. Ph. D. 2014-03-14T21:15:05Z 2014-03-14T21:15:05Z 1992 2006-06-19 2006-06-19 2006-06-19 Dissertation Text etd-06192006-125720 http://hdl.handle.net/10919/38626 http://scholar.lib.vt.edu/theses/available/etd-06192006-125720/ en OCLC# 27379287 LD5655.V856_1992.S671.pdf In Copyright http://rightsstatements.org/vocab/InC/1.0/ vii, 102 leaves BTD application/pdf application/pdf Virginia Tech
collection NDLTD
language en
format Others
sources NDLTD
topic LD5655.V856 1992.S671
Gravity
Quantum gravity
spellingShingle LD5655.V856 1992.S671
Gravity
Quantum gravity
Soo, Chopin
Classical and quantum gravity with Ashtekar variables
description This thesis is a study of classical and quantum gravity with Ashtekar variables. The Ashtekar constraints are shown to capture the essence of the constraints and constraint algebra of General Relativity in four dimensions. A classification scheme of the solution space of the Ashtekar constraints is proposed and the corresponding physics is investigated. The manifestly covariant equations of motion for the Ashtekar variables are derived. Explicit examples are discussed and new classical solutions of General Relativity are constructed by exploiting the properties of the Ashtekar variables. Non-perturbative canonical quantization of the theory is performed. The ordering of the quantum constraints as well as the formal closure of the quantum constraint algebra are explored. A detailed Becchi-Rouet-Stora-Tyutin (BRST) analysis of the theory is given. The results demonstrate explicitly that in quantum gravity, fluctuations in topology can occur and there are strong evidences of phases in the theory. There is a phase which is described by a topological quantum field theory (TQFT) of the Donaldson-Witten type and an Abelian antiinstanton phase wherein self-interactions of the gravitational fields produce symmetry breaking from SO(3) to U(1). The full theory is much richer and includes fluctuations which bring the system out of the various restricted sectors while preserving diffeomorphism invariance. Invariants of the quantum theory with are constructed through BRST descents. They provide a clear and systematic characterization of non-local observables in quantum gravity, and can yield further differential invariants of four-manifolds. === Ph. D.
author2 Physics
author_facet Physics
Soo, Chopin
author Soo, Chopin
author_sort Soo, Chopin
title Classical and quantum gravity with Ashtekar variables
title_short Classical and quantum gravity with Ashtekar variables
title_full Classical and quantum gravity with Ashtekar variables
title_fullStr Classical and quantum gravity with Ashtekar variables
title_full_unstemmed Classical and quantum gravity with Ashtekar variables
title_sort classical and quantum gravity with ashtekar variables
publisher Virginia Tech
publishDate 2014
url http://hdl.handle.net/10919/38626
http://scholar.lib.vt.edu/theses/available/etd-06192006-125720/
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