找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

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

[复制链接]
楼主: ODE
发表于 2025-3-25 03:56:12 | 显示全部楼层
发表于 2025-3-25 11:13:01 | 显示全部楼层
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
发表于 2025-3-25 15:11:11 | 显示全部楼层
发表于 2025-3-25 16:23:06 | 显示全部楼层
发表于 2025-3-25 23:24:29 | 显示全部楼层
发表于 2025-3-26 01:57:25 | 显示全部楼层
发表于 2025-3-26 04:50:59 | 显示全部楼层
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
发表于 2025-3-26 08:54:21 | 显示全部楼层
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
发表于 2025-3-26 16:06:31 | 显示全部楼层
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.
发表于 2025-3-26 18:40:02 | 显示全部楼层
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
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-2 06:10
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表