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In the standard cosmological model, the Universe consists mainly of two invisible substances: vacuum energy with constant mass-density rho_v=\Lambda/(8pi G) (where Lambda is a `cosmological constant' originally proposed by Einstein and G is…

宇宙学与河外天体物理 · 物理学 2015-06-18 Matthew G. Walker , Abraham Loeb

The negative pressure accompanying gravitationally-induced particle creation can lead to a cold dark matter (CDM) dominated, accelerating Universe (Lima et al. 1996) without requiring the presence of dark energy or a cosmological constant.…

天体物理学 · 物理学 2009-07-22 G. Steigman , R. C. Santos , J. A. S. Lima

A dark-energy-free cosmological model ($\Omega_{DE} \equiv 0$) based on gravitationally induced adiabatic particle creation is proposed. The thermodynamics of particle production yields an effective negative pressure that drives both…

宇宙学与河外天体物理 · 物理学 2025-11-18 P. W. R. Lima , J. A. S. Lima

A new accelerating cosmology driven only by baryons plus cold dark matter (CDM) is proposed in the framework of general relativity. In this model the present accelerating stage of the Universe is powered by the negative pressure describing…

宇宙学与河外天体物理 · 物理学 2010-12-06 J. A. S. Lima , J. F. Jesus , F. A. Oliveira

We provide a simple analytical solution of the Friedmann equations for a universe made of stiff matter, dust matter, and dark energy. A stiff matter era is present in the cosmological model of Zel'dovich (1972) where the primordial universe…

广义相对论与量子宇宙学 · 物理学 2015-12-02 Pierre-Henri Chavanis

A new kind of accelerating flat model with no dark energy that is fully dominated by cold dark matter (CDM) is investigated. The number of CDM particles is not conserved and the present accelerating stage is a consequence of the negative…

天体物理学 · 物理学 2014-11-18 J. A. S. Lima , F. E. Silva , R. C. Santos

A simple and surprisingly realistic model of the origin of the universe can be developed using the Friedmann equation from general relativity, elementary quantum mechanics, and the experimental values of h, c, G and the proton mass. The…

广义相对论与量子宇宙学 · 物理学 2015-06-25 T. R. Mongan

A scalar-tensor theory of gravity is formulated in which $G$ and particle masses are allowed to vary. The theory yields a globally static cosmological model with no evolutionary timescales, no cosmological coincidences, and no flatness and…

综合物理 · 物理学 2015-10-01 Meir Shimon

A perfect fluid, spatially flat cosmology in a $f(T)$ model, derived from a recently proposed general Born-Infeld type theory of gravity is studied. Four dimensional cosmological solutions are obtained assuming the equation of state…

广义相对论与量子宇宙学 · 物理学 2014-12-04 Soumya Jana

Assuming that observers located inside the Universe measure a time flow which is different from the time appearing in the Friedmann-Lemaitre equation, and determining this time flow such that the Universe always appears flat to these…

宇宙学与河外天体物理 · 物理学 2012-12-24 Pierre Magain

We present a cosmological model arising from a gravitational theory with an infinite tower of higher-order curvature invariants that can reproduce the entire evolution of the Universe: from inflation to late-time acceleration, without…

广义相对论与量子宇宙学 · 物理学 2022-02-10 Luisa G. Jaime , Gustavo Arciniega

We discuss physical interpretation of {\Lambda}CDM cosmology from a Machian model of the universe containing nothing but visible matter (ordinary matter, radiation). The Friedmann equation can be derived from a Machian definition of energy,…

广义相对论与量子宇宙学 · 物理学 2016-06-28 Herman Telkamp

We show that a cosmology driven by gravitationally induced particle production of all non-relativistic species existing in the present Universe mimics exactly the observed flat accelerating $\Lambda$CDM cosmology with just one dynamical…

广义相对论与量子宇宙学 · 物理学 2016-03-23 J. A. S. Lima , R. C. Santos , J. V. Cunha

We propose an alternative, nonsingular, cosmic scenario based on gravitationally induced particle production. The model is an attempt to evade the coincidence and cosmological constant problems of the standard model ($\Lambda$CDM) and also…

宇宙学与河外天体物理 · 物理学 2015-06-05 J. A. S. Lima , S. Basilakos , F. E. M. Costa

The $\Lambda$CDM framework offers a remarkably good description of our universe with a very small number of free parameters, which can be determined with high accuracy from currently available data. However, this does not mean that the…

宇宙学与河外天体物理 · 物理学 2015-07-22 Yves Zolnierowski , Alain Blanchard

This paper deals with the cancellation mechanism, which identifies the energy density of space-time expansion in an empty universe with the zero-point energy density and avoids the scale discrepancy with the observed energy density…

综合物理 · 物理学 2018-06-12 Christian Henke

We provide preliminary quantitative evidence that a new solution to averaging the observed inhomogeneous structure of matter in the universe [gr-qc/0702082, arxiv:0709.0732], may lead to an observationally viable cosmology without exotic…

天体物理学 · 物理学 2008-11-26 Ben M. Leith , S. C. Cindy Ng , David L. Wiltshire

We generalize the fractal bubble model (FB), recently proposed in the literature as an alternative to the standard $\Lambda$CDM cosmology, to include a non-zero cosmological constant. We retain the same volume partition of voids and walls…

广义相对论与量子宇宙学 · 物理学 2012-01-30 Stefano Viaggiu

Astronomical measurements of the Omegas for mass density, cosmological constant lambda and curvature k are shown to be sufficient to produce a unique and detailed cosmological model describing dark energy influences based on the Friedman…

综合物理 · 物理学 2010-01-14 James G. Gilson

Dark energy and dark matter constitute 95% of the observable Universe. Yet the physical nature of these two phenomena remains a mystery. Einstein suggested a long-forgotten solution: gravitationally repulsive negative masses, which drive…

综合物理 · 物理学 2018-12-05 J. S. Farnes
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