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Duality invariant formulations of string and M-theoryMalek, Emanuel January 2015 (has links)
No description available.
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Investigation on the holographic principleJiang, Li, Fischler, Willy, January 2003 (has links) (PDF)
Thesis (Ph. D.)--University of Texas at Austin, 2003. / Supervisor: Willy Fischler. Vita. Includes bibliographical references. Also available from UMI.
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Investigation on the holographic principleJiang, Li 28 August 2008 (has links)
Not available / text
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FIELD THEORIES INVOLVING TENSOR AND CONNECTION FIELDSMcKellar, Robert James January 1978 (has links)
No description available.
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MATHEMATICAL FOUNDATIONS OF THE EINSTEIN FIELD EQUATIONSAnderson, Ian, 1952- January 1976 (has links)
No description available.
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Hellmann-Feynman theorem in some classical field theories by François Bégin.Bégin, François. January 1986 (has links)
No description available.
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On a class of completely integrable classical field theoriesDavid, Daniel. January 1982 (has links)
No description available.
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The philosophical significance of unitarily inequivalent representations in quantum field theoryLupher, Tracy Alexander. January 1900 (has links)
Thesis (Ph. D.)--University of Texas at Austin, 2008. / Vita. Includes bibliographical references.
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A cosmological field theoryStarkovich, Steven Paul 04 July 2018 (has links)
Field theory is used to describe the material content of the universe throughout
its entire history, and an oscillating cosmological model without a singularity
is presented. In our theory, the “cosmological fluid” is described by a classical
scalar field that undergoes a series of phase transitions over the lifetime of the
universe. Each transition corresponds to a discontinuous change in the equation
of state of the field. In general, for an FRW universe and a given equation of
state, we show that the field potential V(Φ) may be derived from the solution of
Piccati’s equation. The resulting expression for V(Φ) includes parameters whose
values are determined from the boundary conditions. In our theory, we employ the
standard cosmological model and the fundamental Planck quantities to provide
these boundary conditions. We thereby determine the scalar field Lagrangian for
the entire history of the universe. The resulting cosmological model is free of any
singularities, and includes an early inflationary epoch. Inflation arises in our theory
as a consequence of the initial conditions. The theory describes a universe that
is very cold at its minimum radius, although it heats rapidly during the initial inflationary
era. This increase in the temperature of the scalar field during inflation
is a direct consequence of applying classical thermodynamics under the assumed
conditions for the early universe, and does not depend on the fine-tuning of free
parameters. Inflation continues until a maximum possible physical temperature
(the Planck temperature) is attained, at which point a phase transition occurs
and the standard model era begins. By relating the temperature of the scalar
field in our theory to the radiation temperature in the standard model universe,
it is possible to establish a thermodynamic constraint on a more complete theory
of matter for the early universe. Although, in principle, inflation occurs for any
equation of state where p < -(1/3)p, we find that the initial equation of state
must be p ≈ -p if the later epochs of the universe are to resemble the standard
model. In particular, we find that Ho = 33 - 44 km sec-1 Mpc-1 is the value
of the Hubble parameter a t the current epoch that is least sensitive to the initial
equation of state. / Graduate
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Renormalization of cavity field theoriesStoddart, A J January 1990 (has links)
Bibliography: pages 95-97. / A major obstacle to calculating Feynman diagrams in field theories, confined to a cavity, has always been the divergent loop diagrams. So far, only the quantum chromodynamic and electrodynamic self-energies of a ls1/2 quark, confined to a static spherical cavity, have been accurately calculated. These quantities are of immediate interest in the M.I.T. bag model. The existing methods to calculate loop diagrams are based on the multiple reflection scheme, in which the zero reflection term is separated out analytically, and evaluated separately. Thus far, there are some indications that this method is unsuitable for the quadratically divergent one loop vacuum polarization. In this thesis we firstly develop a set of Fourier transforms, appropriate to a discussion of renormalization in a cavity. Using these, we renormalize the cavity propagators to one loop for scalar, Dirac, and gauge fields. We then introduce a new computational method to subtract out the divergences, based on dimensional regularization. Using this method, we present results for various loop diagrams. The scalar φ⁴ theory is used as a pedagogical example. We then present the quark self-energy for several low lying cavity modes. Finally we tackle the long standing and hitherto unresolved question of the vacuum polarization. For this we give a detailed discussion of surface divergences, and present results for scalar quantum electrodynamics. We make a suggestion for the implementation of the running coupling constant in the cavity.
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