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相关论文: Induced Gravity and the Attractor Dynamics of Dark…

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We study the cosmological evolution of an induced gravity model with a scale symmetry breaking potential for the scalar field. The radiation to matter transition, following inflation and reheating, influences the dynamics of such a field…

广义相对论与量子宇宙学 · 物理学 2015-06-04 Alexander Y. Kamenshchik , Alessandro Tronconi , Giovanni Venturi

Modern astrophysical and cosmological models are faced with two severe theoretical difficulties, that can be summarized as the dark energy and the dark matter problems. Relative to the former, it has been stated that cosmology has entered a…

广义相对论与量子宇宙学 · 物理学 2013-08-23 Francisco S. N. Lobo

Observations provide increasingly strong evidence that the universe is accelerating. This revolutionary advance in cosmological observations confronts theoretical cosmology with a tremendous challenge, which it has so far failed to meet.…

天体物理学 · 物理学 2008-11-26 Ruth Durrer , Roy Maartens

We present a model where a non-conventional scalar field may act like dark energy leading to cosmic acceleration. The latter is driven by an appropriate field configuration, which result in an effective cosmological constant. The potential…

高能物理 - 理论 · 物理学 2009-11-11 Alex Kehagias

We study the cosmological evolution of an induced gravity model with a self-interacting scalar field $\sigma$ and in the presence of matter and radiation. Such model leads to Einstein Gravity plus a cosmological constant as a stable…

天体物理学 · 物理学 2008-11-26 F. Finelli , A. Tronconi , G. Venturi

The reason for the present accelerated expansion of the Universe stands as one of the most profound questions in the realm of science, with deep connections to both cosmology and fundamental physics. From a cosmological point of view,…

广义相对论与量子宇宙学 · 物理学 2024-08-22 Peixiang Ji , Lijing Shao

Cosmic acceleration can be achieved not only with a sufficiently flat scalar field potential but through kinetic terms coupled to gravity. These derivative couplings impose a shift symmetry on the scalar field, aiding naturalness. We write…

宇宙学与河外天体物理 · 物理学 2011-11-29 Giulia Gubitosi , Eric V. Linder

Astrophysical observations are pointing out huge amounts of dark matter and dark energy needed to explain the observed large scale structures and cosmic accelerating expansion. Up to now, no experimental evidence has been found, at…

天体物理学 · 物理学 2009-11-11 S. Capozziello , V. F. Cardone , A. Troisi

We propose that dark energy in the form of a scalar field could effectively couple to dark matter inhomogeneities. Through this coupling energy could be transferred to/from the scalar field, which could possibly enter an accelerated regime.…

宇宙学与河外天体物理 · 物理学 2016-04-25 Valerio Marra

I review the problem of dark energy focusing on the cosmological constant as the candidate and discuss its implications for the nature of gravity. Part 1 briefly overviews the currently popular `concordance cosmology' and summarises the…

广义相对论与量子宇宙学 · 物理学 2008-11-26 T. Padmanabhan

A model of induced gravity with a Higgs potential is investigated in detail in view of the pressure components related to the scalar-field excitations. The physical consequences emerging as an artifact due to the presence of these pressure…

广义相对论与量子宇宙学 · 物理学 2010-11-29 Nils M. Bezares-Roder , Hemwati Nandan , Heinz Dehnen

In this article, we examine a model which proposes a common explanation for the presence of additional attractive gravitational effects -- generally considered to be due to dark matter -- in galaxies and in clusters, and for the presence of…

天体物理学 · 物理学 2007-05-23 Alexandre Arbey

A global scale-invariant Dark Energy model based on Induced Gravity with the addition of a small $R^2$ contribution is examined. The scalar field (quintessence), playing the role of Dark Energy, has a quartic potential and generates…

广义相对论与量子宇宙学 · 物理学 2025-02-14 Alessandro Tronconi , Giovanni Venturi

We use action-angle variables to describe the basic physics of coherent scalar field oscillations in the expanding universe. These analytical mechanics methods have some advantages, like the identification of adiabatic invariants. As an…

天体物理学 · 物理学 2016-08-30 Eduard Masso , Francesc Rota , Gabriel Zsembinszki

Explanations of the late-time cosmic acceleration within the framework of general relativity are plagued by difficulties. General relativistic models are mostly based on a dark energy field with fine-tuned, unnatural properties. There is a…

天体物理学 · 物理学 2010-04-22 Ruth Durrer , Roy Maartens

We study the interaction between dark matter and dark energy, with dark energy described by a scalar field having a double exponential effective potential. We discover conditions under which such a scalar field driven solution is a late…

广义相对论与量子宇宙学 · 物理学 2015-08-06 Vartika Gupta , Rakesh Kabir , Amitabha Mukherjee , Daksh Lohiya

Cosmologists are just beginning to probe the properties of the cosmic vacuum and its role in reversing the attractive pull of gravity to cause an acceleration in the expansion of the cosmos. The cause of this acceleration is given the…

宇宙学与河外天体物理 · 物理学 2016-11-15 Eric V. Linder

The discovery of accelerated cosmic expansion implies that, in addition to the attractive gravity of matter, there exists in our universe some other form of energy (dark energy or cosmological constant) producing a repulsive force. The…

综合物理 · 物理学 2013-03-26 Ti-Pei Li

The origin of the observed acceleration of the expansion of the universe is a major problem of modern cosmology and theoretical physics. Simple estimations of the contribution of vacuum to the density energy of the universe in quantum field…

宇宙学与河外天体物理 · 物理学 2013-06-11 Arnaud Dupays , Brahim Lamine , Alain Blanchard

It is argued that the discovery of cosmic acceleration could have been anticipated on thermodynamic grounds, namely, the generalized second law and the approach to equilibrium at large scale factor. Therefore, the existence of dark energy…

广义相对论与量子宇宙学 · 物理学 2015-05-20 Ninfa Radicella , Diego Pavón
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