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相关论文: Coupled Dark Energy field variation

200 篇论文

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

We introduce a new form of coupling between dark energy and dark matter that is quadratic in their energy densities. Then we investigate the background dynamics when dark energy is in the form of exponential quintessence. The three types of…

广义相对论与量子宇宙学 · 物理学 2010-04-14 Christian G. Boehmer , Gabriela Caldera-Cabral , Nyein Chan , Ruth Lazkoz , Roy Maartens

We present a scenario in which a scalar field dark energy is coupled to the trace of the energy momentum tensor of the baryonic matter fields. In the slow-roll regime, this interaction could give rise to the cosmological features of dark…

宇宙学与河外天体物理 · 物理学 2011-02-02 Alejandro Aviles , Jorge L. Cervantes-Cota

We consider the interaction between dark matter and dark energy in the framework of holographic dark energy, and propose a natural and physically plausible form of interaction, in which the interacting term is proportional to the product of…

宇宙学与河外天体物理 · 物理学 2014-05-27 Yin-zhe Ma , Yan Gong , Xuelei Chen

The cosmological model with an interaction between dynamical quintessence dark energy and cold dark matter is considered. Evolution of a dark energy equation of state parameter is defined by a dark energy adiabatic sound speed and a dark…

宇宙学与河外天体物理 · 物理学 2023-11-08 Roman Neomenko

We present new constraints on coupled dark energy from the recent measurements of the Cosmic Microwave Background Anisotropies from the Planck satellite mission. We found that a coupled dark energy model is fully compatible with the Planck…

宇宙学与河外天体物理 · 物理学 2013-09-02 Valentina Salvatelli , Andrea Marchini , Laura Lopez-Honorez , Olga Mena

We study CMB constraints on a model with a cosmological constant and a fraction of dark matter non-minimally coupled to a massless scalar field. In this scenario, there is an extra gravity-like fifth force which can affect the evolution of…

宇宙学与河外天体物理 · 物理学 2018-05-09 Sophie C. F. Morris , Anne M. Green

Cosmological dark energy is a natural source of variation of the fine structure constant. Using a model-independent approach we show that once general assumptions about the alpha-varying interactions are made, astronomical probes of its…

天体物理学 · 物理学 2015-06-24 David Parkinson , Bruce A. Bassett , John D. Barrow

The existence of dark energy is essential to explain the cosmic accelerated expansion. We consider a homogenous interacting tachyonic scalar field as a possible candidate for the dynamical dark energy. The interaction between the tachyonic…

广义相对论与量子宇宙学 · 物理学 2023-05-02 V K Ojha , Adithya A Rao , S D Pathak

I consider couplings between the dark energy and dark matter sectors. I describe how the existence of an adiabatic regime, in which the dark energy field instantaneously tracks the minimum of its effective potential, opens the door for a…

宇宙学与河外天体物理 · 物理学 2009-10-16 Mark Trodden

We discuss the coupling between dark energy and matter by considering a homogeneous tachyonic scalar field as a candidate for dark energy. We obtained the functional form of scale factor by assuming that the coupling strength depends…

广义相对论与量子宇宙学 · 物理学 2021-01-27 A Kundu , S D Pathak , V K Ojha

We investigate an interacting dark energy model which allows for the kinetic term of the scalar field to couple to dark matter via a power-law interaction. The model is characterised by scaling solutions at early times, which are of high…

宇宙学与河外天体物理 · 物理学 2022-12-06 Elsa M. Teixeira , Bruno J. Barros , Vasco M. C. Ferreira , Noemi Frusciante

We assess the viability of successful reconstruction of the evolution of the dark energy equation of state using varying fundamental couplings, such as the fine structure constant or the proton-to-electron mass ratio. We show that the same…

宇宙学与河外天体物理 · 物理学 2015-06-03 P. P. Avelino , L. Losano , R. Menezes , J. C. R. E. Oliveira

Cosmological observations have revealed the existence of a dark matter sector, which is commonly assumed to be made up of one particle species only. However, this sector might be more complicated than we currently believe: there might be…

天体物理学 · 物理学 2008-11-26 A. W. Brookfield , C. van de Bruck , L. M. H. Hall

We investigate the model where electrons and dark matter interact with dark energy through the rolling of a scalar field which comes from extra dimensional theories such as the braneworld theory and Brans-Dicke theory. In this model, dark…

宇宙学与河外天体物理 · 物理学 2023-05-01 Kouki Hoshiya , Yo Toda

We investigate the impact on the classical dynamics of dark matter particles and dark energy of a non-minimal coupling in the dark sector, assuming that the mass of the dark matter particles is coupled to a dark energy scalar field. We show…

宇宙学与河外天体物理 · 物理学 2015-05-06 P. P. Avelino

We briefly discuss the intriguing case of a phenomenological non-gravitational coupling in the dark sector, where the interaction is parameterized as an energy transfer either from dark matter to dark energy or the opposite. We show that a…

宇宙学与河外天体物理 · 物理学 2017-07-04 Riccardo Murgia

Dark energy and dark matter are only indirectly measured via their gravitational effects. It is possible that there is an exchange of energy within the dark sector, and this offers an interesting alternative approach to the coincidence…

广义相对论与量子宇宙学 · 物理学 2009-03-24 Gabriela Caldera-Cabral , Roy Maartens , L. Arturo Urena-Lopez

Under the assumption that the variations of parameters of nature and the current acceleration of the universe are related and governed by the evolution of a single scalar field, we show how information can be obtained on the nature of dark…

宇宙学与河外天体物理 · 物理学 2009-10-27 N. J. Nunes , T. Dent , C. J. A. P. Martins , G. Robbers

The today estimated value of dark energy can be achieved by the vacuum condensate induced by neutrino mixing phenomenon. Such a tiny value is recovered for a cut-off of the order of Planck scale and it is linked to the sub eV neutrino mass…

高能物理 - 理论 · 物理学 2014-11-18 A. Capolupo , S. Capozziello , G. Vitiello