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A constant-rate creation of dark particles in the late-time FLRW spacetime provides a cosmological model in accordance with precise observational tests. The matter creation backreaction implies in this context a vacuum energy density…

宇宙学与河外天体物理 · 物理学 2014-05-27 Saulo Carneiro

With attempts to quench the cosmological constant $\Lambda$ having so far failed, we instead investigate what could be done if $\Lambda$ is not quenched and actually gets to be as big as elementary particle physics suggests. Since the…

天体物理学 · 物理学 2007-05-23 Philip D. Mannheim

Dark energy cosmology is considered in a modified Gauss-Bonnet model of gravity with and without a scalar field. It is shown that these generalizations of General Relativity endow it with a very rich cosmological structure: it may naturally…

广义相对论与量子宇宙学 · 物理学 2015-05-18 Emilio Elizalde , Ratbay Myrzakulov , Valery V. Obukhov , Diego Sáez-Gómez

The absence of guidance from fundamental physics about the mechanism behind cosmic acceleration has given rise to a number of alternative cosmological scenarios. These are based either on modifications of general relativistic gravitation…

宇宙学与河外天体物理 · 物理学 2015-05-20 M. A. Dantas , J. S. Alcaniz , D. Mania , Bharat Ratra

The standard cosmological model, based on general relativity with an inflationary era, is very effective in accounting for a broad range of observed features of the universe. However, the ongoing puzzles about the nature of dark matter and…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Roy Maartens

The old cosmological-constant (CC) problem indicates an inconsistency of the usual formulation of semiclassical gravity. The usual formulation of semiclassical gravity also seems to be inconsistent with the conventional interpretation of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 H. Nikolic

The standard cosmological model is based on general relativity and includes dark matter and dark energy. An important prediction of this model is a fixed relationship between the gravitational potentials responsible for gravitational…

天体物理学 · 物理学 2008-11-26 Pengjie Zhang , Michele Liguori , Rachel Bean , Scott Dodelson

The creation of a quantum Universe is described by a {\em density matrix} which yields an ensemble of universes with the cosmological constant limited to a bounded range $\Lambda_{\rm min}\leq \Lambda \leq \Lambda_{\rm max}$. The domain…

高能物理 - 理论 · 物理学 2008-11-26 A. O. Barvinsky , A. Yu. Kamenshchik

Major observational efforts in the coming decade are designed to probe the equation of state of dark energy. Measuring a deviation of the equation-of-state parameter w from -1 would indicate a dark energy that cannot be represented solely…

天体物理学 · 物理学 2009-03-12 Alan Cooney , Simon DeDeo , Dimitrios Psaltis

Cosmological scenarios wherein the cumulative number of spontaneously formed, cognitively impaired, disembodied transient observers is vastly larger than the corresponding number of atypical `ordinary observers' (OOs) formed in the…

综合物理 · 物理学 2025-12-22 Meir Shimon

The pure Brans-Dicke (BD) gravity with or without the cosmological constant $\Lambda $ has been taken as a model theory for the dark matter. Indeed, there has been a consensus that unless one modifies either the standard theory of gravity,…

天体物理学 · 物理学 2007-08-21 Hongsu Kim

This paper continues the development of a discrete space-time concept that is recently used in the explanation of the cosmological constant. Instead of order estimation, a more theoretical treatment of the theory is introduced. Based on the…

综合物理 · 物理学 2007-05-23 H. M. Mok

We integrate $\Lambda_{\rm s}$CDM, a promising scenario for alleviating cosmological tensions, into VCDM, a type-II minimally modified gravity. This promotes the scenario to a fully predictive model (dubbed $\Lambda_{\rm s}$VCDM) that…

In this work we focus on the gravitationally influenced adiabatic particle creation process, a mechanism that does not need any dark energy or modified gravity models to explain the current accelerating phase of the universe. Introducing…

广义相对论与量子宇宙学 · 物理学 2018-04-10 Supriya Pan , Barun Kumar Pal , Souvik Pramanik

In the more recent literature on cosmological evolutions of the universe the cosmic vacuum energy has become a non-renouncable ingredient. The cosmological constant $\Lambda$, first invented by Einstein, but later also rejected by him,…

广义相对论与量子宇宙学 · 物理学 2016-10-28 H. J. Fahr , M. Heyl

It is shown that a first-order relativistic perturbation theory for the open, flat or closed Friedmann-Lemaitre-Robertson-Walker universe admits one, and only one, gauge-invariant quantity which describes the perturbation to the energy…

广义相对论与量子宇宙学 · 物理学 2014-03-25 P. G. Miedema

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

The well-known brane world model of cosmology is an alternative to the standard model of cosmology, called {\Lambda}CDM (Lambda Cold Dark Matter) model. However, the quadratical energy density of the brane universe requires an undesirable…

广义相对论与量子宇宙学 · 物理学 2021-11-01 Christian Henke

The DGP brane-world model provides an alternative to the standard LCDM cosmology, in which the late universe accelerates due to a modification of gravity rather than vacuum energy. The cosmological constant $\Lambda$ in LCDM is replaced by…

天体物理学 · 物理学 2009-11-13 Kazuya Koyama , Roy Maartens

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