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In certain two-dimensional models, collapsing matter forms a black hole if and only if the incoming energy flux exceeds the Hawking radiation rate. Near the critical threshold, the black hole mass is given by a universal formula in terms of…

高能物理 - 理论 · 物理学 2009-09-17 A. Strominger , L. Thorlacius

(abbreviated) We study quantized solutions of WdW equation describing a closed FRW universe with a $\Lambda $ term and a set of massless scalar fields. We show that when $\Lambda \ll 1$ in the natural units and the standard $in$-vacuum…

广义相对论与量子宇宙学 · 物理学 2015-09-23 P. Ivanov , S. V. Chernov

It is fair to say that the deepest mystery in our understanding of nature is the birth of our universe. Much of the dilemma over the last decades comes from the extraordinarily small probability that the universe started with the high…

高能物理 - 理论 · 物理学 2008-09-25 Laura Mersini-Houghton

Wheeler-DeWitt equation is applied to $k > 0$ Friedmann Robertson Walker metric with various types of matter. It is shown that if the Universe ends in the matter dominated era (e.g., radiation or pressureless gas) with zero cosmological…

高能物理 - 理论 · 物理学 2010-11-01 Jong Hyun Kung

The wave function of the universe is usually taken to be a functional of the three-metric on a spacelike section, Sigma, which is measured. It is sometimes better, however, to work in the conjugate representation, where the wave function…

高能物理 - 理论 · 物理学 2014-11-18 Raphael Bousso , Stephen Hawking

In the background of Friedmann-Robertson-Walker Universe, there exists Hawking radiation which comes from the cosmic apparent horizon due to quantum effect. Although the Hawking radiation on the late time evolution of the universe could be…

广义相对论与量子宇宙学 · 物理学 2012-08-02 Changjun Gao

We consider two quantum cosmological models with a massive scalar field: an ordinary Friedmann universe and a universe containing primordial black holes. For both models we discuss the complex solutions to the Euclidean Einstein equations.…

广义相对论与量子宇宙学 · 物理学 2009-10-28 R. Bousso , S. W. Hawking

The basic scaling laws for structures in a fractal universe require that the characteristic quantity of action associated with astronomical bodies should be of order near the maximum possible action allowed by the holographic upper bound.…

综合物理 · 物理学 2008-08-13 Scott Funkhouser

Wheeler-Dewitt equation for the wave function of the universe appeared long ago in an approach to quantization of gravity. Presently, the universe considered as the microuniverse, very tiny universe compared to the outer universe to which…

综合物理 · 物理学 2020-02-07 S S De , Farook Rahaman , Antara Mapdar

The early universe according to the big bang and the grand unified theories is discussed. The shortcomings of big bang are summarized together with their resolution by inflationary cosmology. Inflation, the subsequent oscillation and decay…

高能物理 - 唯象学 · 物理学 2007-05-23 George Lazarides

In this paper we propose a mechanism of natural preheating of our universe by introducing an inflaton field dependent mass term for the gravitational wave for a specific class of massive gravity theory. For any single field inflationary…

高能物理 - 理论 · 物理学 2016-08-03 Debaprasad Maity

In this note we show that vector perturbations exhibit growing mode solutions in a contracting Universe, such as the contracting phase of the Pre Big Bang or the Cyclic/Ekpyrotic models of the Universe. This is not a gauge artifact and will…

高能物理 - 理论 · 物理学 2007-05-23 Thorsten Battefeld , Robert Brandenberger

Within the framework of an eternal inflationary scenario, a natural question regarding the production of eternal bubbles is the essential condition requires to have a universe capable of generating life. In either an open or a closed…

宇宙学与河外天体物理 · 物理学 2017-08-30 Sohrab Rahvar

We propose a picture, within the pre-big-bang approach, in which the universe emerges from a bath of plane gravitational and dilatonic waves. The waves interact gravitationally breaking the exact plane symmetry and lead generically to…

高能物理 - 理论 · 物理学 2014-11-18 A. Feinstein , K. E. Kunze , M. A. Vazquez-Mozo

When the semi-positive cosmological constant is dynamical, the naive Euclidean Einstein action is unbounded from below and the Hartle-Hawking wavefunction of the universe is not normalizable. With the inclusion of back-reaction (a crucial…

高能物理 - 理论 · 物理学 2007-05-23 Saswat Sarangi , S. -H. Henry Tye

How is the universe organized on large scales? How did this structure evolve from the unknown initial conditions of a rather smooth early universe to the present time? The answers to these questions will shed light on the cosmology we live…

天体物理学 · 物理学 2007-05-23 Neta A. Bahcall

We study the classical dynamics of the universe undergoing a transition from contraction to expansion through a big bang singularity. The dynamics is described by a system of differential equations for a set of physical quantities, such as…

广义相对论与量子宇宙学 · 物理学 2015-04-14 BingKan Xue , Edward Belbruno

The Hawking minisuperspace model (closed FRW geometry with a homogeneous massive scalar field) provides a fairly non-trivial testing ground for fundamental problems in quantum cosmology. We provide evidence that the Wheeler-DeWitt equation…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Franz Embacher

We propose that at the beginning of the universe gravity existed in a limbo either because it was switched off or because it was only conformally coupled to all particles. This picture can be reverse-engineered from the requirement that the…

广义相对论与量子宇宙学 · 物理学 2015-12-09 Giovanni Amelino-Camelia , Michele Arzano , Giulia Gubitosi , Joao Magueijo

We argue that the topological string partition function, which has been known to correspond to a wave-function, can be interpreted as an exact ``wave-function of the universe'' in the mini-superspace sector of physical superstring theory.…

高能物理 - 理论 · 物理学 2009-09-17 Hirosi Ooguri , Cumrun Vafa , Erik Verlinde