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Fundamental aspects of the expansion of the universe and cosmic horizons /Davis, Tamara M. January 2003 (has links)
Thesis (Ph. D.)--University of New South Wales, 2003. / Also available online.
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Variational results and solutions in gauge gravity and a bifurcation analysis of black hole orbital dynamicsDean, Bruce H. January 1999 (has links)
Thesis (Ph. D.)--West Virginia University, 1999. / Title from document title page. Document formatted into pages; contains ix, 223 p. : ill. (some col.). Includes abstract. Includes bibliographical references (p. 214-223) and index.
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Relativity and the critical philosophy ...Kassel, Frank, January 1926 (has links)
Thesis (Ph. D.)--University of Pennsylvania, 1926. / Bibliography: p. 48.
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Rotating relativistic models of the universe construction and interpretation /Sviestins, Egils. January 1983 (has links)
Thesis (doctoral)--Stockholm University, 1983. / Includes bibliographical references.
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Spacetime conformal fluctuations and quantum dephasingBonifacio, Paolo. January 2009 (has links)
Thesis (Ph.D.)--Aberdeen University, 2009. / Title from web page (viewed on Oct. 8, 2009). Includes bibliographical references.
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Kosmologia Alberta Einsteina i jej filozoficzne uwarunkowaniaTurek, Józef. January 1982 (has links)
Thesis (doctoral)--Katolicki Uniwersytet Lubelski. / On p. facing t.p.: Wydział Filozofii Chrześcijańskiej. Includes bibliographical references (p. 101-[109]).
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Relationship between mental maturity and the level of understanding of concepts of relativity in grades 4-8Haddid, Wadi. January 1968 (has links)
Thesis (Ph. D.)--University of Wisconsin--Madison, 1968. / Typescript. Vita. eContent provider-neutral record in process. Description based on print version record.
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Electromagnetism in axisymmetric gravitational collapse /Skinfill, Craig Ernest, January 2006 (has links) (PDF)
Thesis (M.S.)--Brigham Young University. Dept. of Physics and Astronomy, 2006. / Includes bibliographical references (p. 83-84).
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Contribution to the quantum theory of gravitationFreeman, Michael James January 1967 (has links)
A quantum theory of gravitation is constructed, by considering the gravitational field in the linear approximation to be a rank II tensor field, which has imposed upon it the auxiliary conditions of symmetry, transversality, and tracelessness. Extensive use is made of the close analogy between the electromagnetic field as a special case of a vector field, and the gravitational field as a special case of a tensor field. This analogy includes the necessity of introducing an indefinite
metric in order to make the auxiliary conditions compatible with the commutation relations.
A complete theory of gravitation must take into account the gravitating nature of gravitation and hence must be a nonlinear
theory. A method proposed by Gupta of iterating the linear field equations for this purpose is investigated, and it is shown that this method fails, because the Lagrangian for the second order equations does not exist. An alternative method of iteration is proposed which avoids this problem, and which yields a functional equation for the Lagrangian of the full nonlinear theory.
Finally, the problem of photon-photon scattering due to the gravitational interaction is investigated. This is done by constructing an interaction Hamiltonian by using the principle
of the compensating field and then applying the standard methods of quantum electrodynamics. It is found that for
sufficiently high frequencies this process dominates the purely
electrodynamic scattering of photons by photons. / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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Spin-two fields and general covarianceHeiderich, Karen Rachel January 1991 (has links)
It has long been presumed that any consistent nonlinear theory of a spin-two field must be generally covariant. Using Wald's consistency criteria, we exhibit classes of nonlinear theories of a spin-two field that do not have general covariance. We consider four alternative formulations of the spin-two equations. As a first example, we consider a conformally invariant theory of a spin-two field coupled to a scalar field. In the next two cases, the usual symmetric rank-two tensor field, γab, is chosen as the potential. In the fourth case, a traceless symmetric rank-two tensor field is used as the potential. We find that consistent nonlinear generalization of these different formulations leads to theories of a spin-two field that are not generally covariant. In particular, we find types of theories which, when interpreted in terms of a metric, are invariant under the infinitesimal gauge transformation γab→γab + ∇ (a∇[symbol omitted]K[symbol omitted]), where Kab is an arbitrary two-form field. In addition, we find classes of theories that are conformally invariant.
As a related problem, we compare the types of theories obtained from the nonlinear extension of a divergence- and curl-free vector field when it is described in terms of two of its equivalent formulations. We find that nonlinear extension of the theory is quite different in each case. Moreover, the resulting types of nonlinear theories may not necessarily be equivalent. A similar analysis is carried out for three-dimensional electromagnetism. / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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