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A huge amount of good quality astrophysical data converges towards the picture of a spatially flat universe undergoing the today observed phase of accelerated expansion. This new observational trend is commonly addressed as Precision…

天体物理学 · 物理学 2009-06-23 S. Capozziello

A dark energy component is responsible for the present stage of acceleration of our universe. If no fine tuning is assumed on the dark energy potential then it will end up dominating the universe at late times and the universe will not stop…

天体物理学 · 物理学 2008-11-26 A. de la Macorra

A huge amount of good quality data converges towards the picture of a spatially flat universe undergoing the today observed phase of accelerated expansion. This new observational trend is commonly addressed as Precision Cosmology. Despite…

广义相对论与量子宇宙学 · 物理学 2008-12-02 S. Capozziello

A pressureless dark matter component fits well with several cosmological observations. However, there are indications that cold dark matter may encounter challenges in explaining observations at small scales, particularly at galactic…

宇宙学与河外天体物理 · 物理学 2025-04-17 Weiqiang Yang , Supriya Pan , Eleonora Di Valentino , Olga Mena , David F. Mota , Subenoy Chakraborty

The introduction of an interaction for dark energy to the standard cosmology offers a potential solution to the cosmic coincidence problem. We examine the conditions on the dark energy density that must be satisfied for this scenario to be…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Micheal S. Berger , Hamed Shojaei

We outline a dynamical dark energy scenario whose signatures may be simultaneously tested by astronomical observations and laboratory experiments. The dark energy is a field with slightly sub-gravitational couplings to matter, a logarithmic…

天体物理学 · 物理学 2009-06-23 Nemanja Kaloper

I briefly review our current understanding of dark matter and dark energy. The first part of this paper focusses on issues pertaining to dark matter including observational evidence for its existence, current constraints and the `abundance…

天体物理学 · 物理学 2022-07-19 Varun Sahni

In this talk I will firstly review on the current constraints on the equation of state of the dark energy from observational data, then present a new scenario of dark energy dubbed {\it Quintom}. The recent fits to the type Ia supernova…

高能物理 - 唯象学 · 物理学 2016-09-06 Xinmin Zhang

The coupling between the dark components provides a new approach to mitigate the coincidence problem of cosmological standard model. In this paper, dark energy is treated as a fluid with a constant equation of state, whose coupling with…

宇宙学与河外天体物理 · 物理学 2014-08-18 Weiqiang Yang , Lixin Xu

In this paper, we explore the cosmological implications of interacting dark energy model in a torsion based gravity namely $f(T)$. Assuming dark energy interacts with dark matter and radiation components, we examine the stability of this…

综合物理 · 物理学 2012-03-27 Mubasher Jamil , D. Momeni , Ratbay Myrzakulov

Modern Cosmology offers us a great understanding of the universe with striking precision, made possible by the modern technologies of the newest generations of telescopes. The standard cosmological model, however, is not absent of…

宇宙学与河外天体物理 · 物理学 2016-10-06 Rafael J. F. Marcondes

Cosmological models involving an interaction between dark matter and dark energy have been proposed in order to solve the so-called coincidence problem. Different forms of coupling have been studied, but there have been claims that…

天体物理学 · 物理学 2009-06-23 Miguel Quartin , Mauricio O. Calvao , Sergio E. Joras , Ribamar R. R. Reis , Ioav Waga

In this study, we will look at an interacting dark energy model. In the framework of Friedmann-Robertson-Walker (FRW) space-time, we have made the hypothesis of an interacting scheme between two fields (dark matter (DM) and dark energy…

广义相对论与量子宇宙学 · 物理学 2023-11-27 J. K. Singh , Ritika Nagpal

The interaction between dark matter and dark energy can be incorporated into field theory models of dark energy that have proved successful in alleviating the coincidence problem. We review recent advances in this field, including new…

宇宙学与河外天体物理 · 物理学 2024-02-02 B Wang , E Abdalla , F Atrio-Barandela , D Pavón

I briefly review the cosmological constant problem and the issue of dark energy (or quintessence). Within the framework of quantum field theory, the vacuum expectation value of the energy momentum tensor formally diverges as $k^4$. A cutoff…

天体物理学 · 物理学 2008-11-26 Varun Sahni

Motivated by results implying that the constituents of dark matter (DM) might be collisional, we consider a cosmological (toy-) model, in which the DM itself possesses some sort of thermodynamic properties. In this case, not only can the…

广义相对论与量子宇宙学 · 物理学 2015-03-19 Kostas Kleidis , Nicholas K. Spyrou

The recent observational evidence for the current cosmic acceleration have stimulated renewed interest in alternative cosmologies, such as scenarios with interaction in the dark sector (dark matter and dark energy). In general, such models…

宇宙学与河外天体物理 · 物理学 2009-10-22 R. S. Goncalves , J. S. Alcaniz , A. Dev , D. Jain

We study some properties of the dark degeneracy, which is the fact that what we measure in gravitational experiments is the energy momentum tensor of the total dark sector, and any split into components (as in dark matter and dark energy)…

宇宙学与河外天体物理 · 物理学 2011-10-17 Alejandro Aviles , Jorge L. Cervantes-Cota

Models where Dark Matter and Dark Energy interact with each other have been proposed to solve the coincidence problem. We review the motivations underlying the need to introduce such interaction, its influence on the background dynamics and…

宇宙学与河外天体物理 · 物理学 2016-08-24 B. Wang , E. Abdalla , F. Atrio-Barandela , D. Pavon

A model for a flat homogeneous and isotropic Universe composed of dark energy, dark matter, neutrinos, radiation and baryons is analyzed. The fields of dark matter and neutrinos are supposed to interact with the dark energy. The dark energy…

广义相对论与量子宇宙学 · 物理学 2008-11-26 G. M. Kremer
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