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In a new model that we proposed, nonperturbative vacuum contributions to the effective action of a free quantized massive scalar field lead to a cosmological solution in which the scalar curvature becomes constant after a time $t_j$ (when…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Leonard Parker , Alpan Raval

In this work, I develop an alternative explanation for the acceleration of the cosmic expansion, which seems to be a result of recent high redshift Supernova data. In the current interpretation, this cosmic acceleration is explained by…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. -F. Pascual-Sánchez

In this essay, I present an alternative explanation for the cosmic acceleration which appears as a consequence of recent high redshift Supernova data. In the usual interpretation, this cosmic acceleration is explained by the presence of a…

广义相对论与量子宇宙学 · 物理学 2009-10-31 J. -F. Pascual-Sánchez

Within the Quantum Field Theory context the idea of a "cosmological constant" (CC) evolving with time looks quite natural as it just reflects the change of the vacuum energy with the typical energy of the universe. In the particular frame…

高能物理 - 唯象学 · 物理学 2008-11-26 Cristina Espana-Bonet , Pilar Ruiz-Lapuente , Ilya L. Shapiro , Joan Sola

The current observations are usually explained by an accelerating expansion of the present universe. However, with the present quality of the supernovae Ia data, the allowed parameter space is wide enough to accommodate the decelerating…

天体物理学 · 物理学 2009-11-07 R. G. Vishwakarma

The "standard" model of cosmology is founded on the basis that the expansion rate of the universe is accelerating at present --- as was inferred originally from the Hubble diagram of Type Ia supernovae. There exists now a much bigger…

宇宙学与河外天体物理 · 物理学 2016-10-24 Jeppe Trøst Nielsen , Alberto Guffanti , Subir Sarkar

The observation that Type Ia supernovae are fainter than expected given their red shifts has led to the conclusion that the expansion of the universe is accelerating. The widely accepted hypothesis is that this acceleration is caused by a…

宇宙学与河外天体物理 · 物理学 2010-07-09 Rutger Dungan , Harrison B. Prosper

In the late 1990s, observations of type Ia supernovae led to the astounding discovery that the universe is expanding at an accelerating rate. The explanation of this anomalous acceleration has been one of the great problems in physics since…

综合物理 · 物理学 2015-11-09 Wun-Yi Shu

The discovery that the cosmic expansion is accelerating has been followed by an intense theoretical and experimental response in physics and astronomy. The discovery implies that our most basic notions about how gravity work are violated on…

宇宙学与河外天体物理 · 物理学 2010-01-15 Robert R. Caldwell , Marc Kamionkowski

We present a new model based on General Relativity in where a subtle change of curvature at late times is able to produce the observed Universe acceleration and an oscillating behavior in the effective equation of state. This model aims to…

宇宙学与河外天体物理 · 物理学 2025-02-18 A. Esteban-Gutiérrez , Miguel A. García-Aspeitia , A. Hernández-Almada , Juan Magaña , V. Motta

We trace the origin of the cosmological constant problem to the assumption that Newton's constant $G$ sets the scale for cosmology. And then we show that once this assumption is relaxed, the very same cosmic acceleration which has served to…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Philip D. Mannheim

The principles of General Relativity allow for a non-vanishing cosmological constant, which can possibly be interpreted at least partially in terms of quantum-fluctuations of matter fields. Depending on sign and magnitude it can cause…

天体物理学 · 物理学 2007-05-23 Domenico Giulini , Norbert Straumann

The novel idea is that the undergoing accelerated expansion of the universe happens due to infrared quantum gravity modifications at intermediate astrophysical scales of galaxies or galaxy clusters, within the framework of Asymptotically…

广义相对论与量子宇宙学 · 物理学 2021-02-16 Fotios K. Anagnostopoulos , Georgios Kofinas , Vasilios Zarikas

A fundamental property of an expanding universe is that any time dependent characteristic of distant objects must appear to scale by the factor $(1+z$). This is called time dilation. Light curves of type Ia supernovae and the duration of…

高能天体物理现象 · 物理学 2019-03-06 David F. Crawford

Cosmic acceleration may be the result of unknown physical processes involving either new fields in high energy physics or modifications of gravitation theory. In the latter case, such modifications are usually related to the existence of…

天体物理学 · 物理学 2009-11-10 J. S. Alcaniz , N. Pires

It is generally argued that the present cosmological observations support the accelerating models of the universe, as driven by the cosmological constant or `dark energy'. We argue here that an alternative model of the universe is possible…

天体物理学 · 物理学 2009-11-07 J. V. Narlikar , R. G. Vishwakarma , G. Burbidge

The quantum field theory prediction of the cosmological constant is 120 orders of magnitude higher than the observed value. This is known as the cosmological constant problem. Here, we deal with the cosmological constant as a scalar field…

高能物理 - 理论 · 物理学 2010-11-29 Nicolas Avilan V. , Jose Rolando Roldan

We have probed a cosmological model in $f(R)$-gravity, which is a cubic equation in scalar curvature $R$. The terms arise due to nonlinear $f(R)$ function are treated as energy due to curvature inspired geometry. As a result, we find…

广义相对论与量子宇宙学 · 物理学 2023-05-03 G. K. Goswami , Rita Rani , Harshna Balhara , J. K. Singh

We investigate the possibility that the late acceleration observed in the rate of expansion of the universe is due to vacuum quantum effects arising in curved spacetime. The theoretical basis of the vacuum cold dark matter (VCDM), or vacuum…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Leonard Parker , Daniel A. T. Vanzella

Recent investigations seem to favor a cosmological dynamics according to which the accelerated expansion of the Universe may have already peaked and is now slowing down again \cite{sastaro}. As a consequence, the cosmic acceleration may be…

宇宙学与河外天体物理 · 物理学 2015-03-13 Julio C. Fabris , Bernardo Fraga , Nelson Pinto-Neto , Winfried Zimdahl
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