Results 261 to 270 of about 202,532 (277)

Hawking-Type Singularity Theorems for Worldvolume Energy Inequalities. [PDF]

open access: yesAnn Henri Poincare
Graf M   +3 more
europepmc   +1 more source

Decaying Cosmological Constant and Cosmology

open access: yesDecaying Cosmological Constant and Cosmology
openaire  

ANOTHER “COSMOLOGICAL” CONSTANT

International Journal of Modern Physics A, 1992
Capovilla, Jacobson and Dell have found a one-parameter family of field equations which coincides with Einstein’s equations when the parameter is set to zero. The basic variable is an SO(3) vector potential. For generic values of the parameter, we show that the solutions of the field equations may be interpreted in terms of Riemannian geometry.
Bengtsson, Ingemar, Peldán, Peter
openaire   +2 more sources

EFFECTIVE COSMOLOGICAL CONSTANT IN BRANE COSMOLOGY

International Journal of Modern Physics D, 2006
We consider a brane-world of co-dimension one without reflection symmetry. Through it, we give a possible explanation of the great discrepancy between the vacuum energy and the observed cosmological constant without contradiction to the knowledge we have about our Universe. We also show the gravity observed will be standard four-dimensional gravity as
Hu, Sen, Wang, Jing-Rong
openaire   +2 more sources

Cosmology ‘without’ Constants

Astrophysics and Space Science, 2003
We review varying speed of light (VSL) theories, in a cosmological and astrophysical setting, and as phenomenological descriptions of quantum gravity. We first introduce two observational puzzles, and explain how they may related to VSL. We then catalogue the various theoretical efforts associated with VSL. We focus on recent VSL theories rendering the
openaire   +1 more source

The Cosmological Constants

Nature, 1937
THE fundamental constants of physics, such as c the velocity of light, h Planck's constant, e the charge and m mass of the electron, and so on, provide for us a set of absolute units for measurement of distance, time, mass, etc. There are, however, more of these constants than are necessary for this purpose, with the result that certain dimensionless ...
openaire   +2 more sources

The cosmological constant and cosmological change

Physics Today, 1977
Is the Universe of infinite extent, or is it a finite system? Will it expand forever, or will it reach some maximum size before turning and collapsing upon itself like an inverse Big Bang? Just a few years ago, models of the conventional Friedman types were showing consistent, albeit tentative, evidence for an open, ever-expanding Universe. Since then,
openaire   +1 more source

Inhomogeneous cosmologies with cosmological constant

Physics Letters A, 1984
Abstract We give a new class of exact inhomogeneous solutions to Einstein's equations with non-zero cosmological constant and zero pressure. They generalize the de Sitter space-time and evolve towards a state that is stationary inside the event horizon of any future inextendible time-like curve and confirm the cosmic “no hair” conjecture.
John D. Barrow, J. Stein-Schabes
openaire   +1 more source

THE COSMOLOGICAL CONSTANT PROBLEM

International Journal of Modern Physics D, 1992
The cosmological constant is a macroscopic parameter which controls the large-scale structure of the Universe. All observations to date have shown that it is very small. However, our modern microscopic theory of particle physics and gravity suggests that the cosmological constant should be very large.
openaire   +1 more source

Cosmological constant

2017
Abstract The contribution of vacuum fluctuations to the cosmological constant is reconsidered studying the dependence on the used regularisation scheme. Then alternative explanations for the observed accelerated expansion of the universe in the present epoch are introduced which either modify gravity or add a new component of matter ...
openaire   +1 more source

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