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Titlebook: Quantum Gravity; M. A. Markov,P. C. West Book 1984 Plenum Press, New York 1984 cosmology.gauge theory.general relativity.geometry.law of t

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樓主: ODE
21#
發(fā)表于 2025-3-25 03:56:12 | 只看該作者
22#
發(fā)表于 2025-3-25 11:13:01 | 只看該作者
The Loss of Quantum Coherence due to Virtual Black Holes. In this paper it is shown how such loss of quantum coherence occurs on a microscopic, elementary particle level. A series of axioms are presented for the asymptotic Green’s Functions for quantum gravity in asymptotically flat space. These axioms are the same as for Quantum Field Theory in flat spa
23#
發(fā)表于 2025-3-25 15:11:11 | 只看該作者
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發(fā)表于 2025-3-25 16:23:06 | 只看該作者
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發(fā)表于 2025-3-25 23:24:29 | 只看該作者
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發(fā)表于 2025-3-26 01:57:25 | 只看該作者
27#
發(fā)表于 2025-3-26 04:50:59 | 只看該作者
Nonsingular Model of the Universe with the Quantum-Gravitational de Sitter Stage and its Observatione, but it encounters a fundamental difficulty, namely, the existence of a singularity at some finite moment of time t = 0 in the past. The Friedman solution cannot be analytically continued to the region t < 0 where, strictly speaking, there is no space and no time. So, in the scope of classical gen
28#
發(fā)表于 2025-3-26 08:54:21 | 只看該作者
Can De Sitter Spacetime be a Final State of the Contracting Universe?d to take into account these non-equilibrium processes by introducing a new additional thermodynamic variable, namely explicit time dependence of all thermodynamic potentials into the thermodynamic relations. It is shown that this trick leads to “softening” of the equation of state. It is demonstrat
29#
發(fā)表于 2025-3-26 16:06:31 | 只看該作者
Self-Consistent Treatment of Vacuum Quantum Effects in Isotropic Cosmology discovery of the black holes quantum evaporation and the complete analysis of vacuum quantum effects in isotropic Universes. It was often pointed out that quantum theory may yield the resolution of one of the main problems of modern theoretical physics — the problem of gravitational singularities.
30#
發(fā)表于 2025-3-26 18:40:02 | 只看該作者
Quantum Field Theories with Spontaneous Symmetry Breaking in External Gravitational Fields of Cosmole extrapolated back in time according to the Friedmann expansion law a(t) ~ t. (or a(t) ~ t.). In this way one is able to describe the physical processes in the early Universe at least up to the “hadronic stage” characterized by the temperature T ~ 1 GeV. However, within this theory one has to postu
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