Results 241 to 250 of about 197,812 (267)
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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,
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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
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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.
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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 ...
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Varying Newton gravitational “constant” cosmology

Annals of Physics
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Clovis Jacinto de Matos, Nicolas Lori
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Cosmological constant as integration constant

Astronomische Nachrichten, 1994
AbstractEinstein's field theory of elementary particles (Einstein 1919) yields black holes with a mass M ˜ G−1 Λ−1/2c2 and a charge Q ˜ G−1/2λ−1/2c2, their curvatu re radius is Λ−1/2. Here 4Λ is an integration constant of Einstein's ‘trace‐less’ gravitation equations.The choice λ = G−1h−1c3 for this constant defines Planckions and implies “strong ...
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Cosmological Constant And Cosmological Quintessence

Extended Study 
Philippakis, Theodore, Raptis, George
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Unveiling the Universe with emerging cosmological probes

Living Reviews in Relativity, 2022
Michele Ennio Maria Ennio Maria Moresco   +2 more
exaly  

Exponentially Small Cosmological Constant in String Theory

Physical Review Letters, 2022
Mehmet Demirtas   +2 more
exaly  

Cosmological constant—the weight of the vacuum

Physics Reports, 2003
Thanu Padmanabhan
exaly  

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