中文
相关论文

相关论文: Cosmological constraints on a dark matter -- dark …

200 篇论文

The paper deals with a theoretical model for interacting dark energy. The interaction between the cold dark matter (dust) and the dark energy has been assumed to be non-gravitational in nature. Exact analytic cosmological solutions are…

广义相对论与量子宇宙学 · 物理学 2015-07-31 Supriya Pan , Subhra Bhattacharya , Subenoy Chakraborty

In the proposed model with interaction between dark energy and dark matter, we consider cosmological scenarios with different equations of state ($w_d$) for dark energy. For both constant and variable equation of state, we analyze solutions…

广义相对论与量子宇宙学 · 物理学 2017-10-18 Supriya Pan , German S. Sharov

Interactions inside the cosmological dark sector influence the cosmological dynamics. As a consequence, the future evolution of the Universe may be different from that predicted by the $\Lambda$CDM model. We review main features of several…

宇宙学与河外天体物理 · 物理学 2014-04-30 W. Zimdahl

We consider a set of non-linear interactions between dark matter and dark energy which comprises couplings proportional to products of (powers of) the energy densities of both dark components and of the total energy. We demonstrate that…

宇宙学与河外天体物理 · 物理学 2015-06-03 Fabiola Arévalo , Anna Paula Ramos Bacalhau , Winfried Zimdahl

We investigate a class of interacting dark energy and dark matter (DM) models, where dark energy is modeled as a $k$-essence scalar field with an inverse-square potential. Two general forms of interaction are considered: one proportional to…

宇宙学与河外天体物理 · 物理学 2026-04-14 Saddam Hussain , Qiang Wu , Tao Zhu

We discuss how to formulate a quantum field theory of dark energy interacting with dark matter. We show that the proposals based on the assumption that dark matter is made up of heavy particles with masses which are very sensitive to the…

高能物理 - 理论 · 物理学 2017-03-09 Guido D'Amico , Teresa Hamill , Nemanja Kaloper

If dark energy interacts with dark matter, there is a change in the background evolution of the universe, since the dark matter density no longer evolves as a^{-3}. In addition, the non-gravitational interaction affects the growth of…

宇宙学与河外天体物理 · 物理学 2009-07-24 Gabriela Caldera-Cabral , Roy Maartens , Bjoern Malte Schaefer

We discuss a model of the universe where dark energy is replaced by electrically-charged extremely-massive dark matter. The cosmological constant has a value of the same order as the mean matter density, consistent with observations, and is…

综合物理 · 物理学 2026-01-26 Paul H. Frampton

We study the effect of an explicit interaction between two scalar fields components describing dark matter in the context of a recent proposal framework for interaction. We find that, even assuming a very small coupling, it is sufficient to…

宇宙学与河外天体物理 · 物理学 2020-10-28 Victor H. Cardenas , Samuel Lepe

In standard cosmologies, dark energy interacts only gravitationally with dark matter. An extension to this picture is interacting quintessence (IQ) model, where scalar field coupled directly to cold dark matter. The percentage deviation is…

宇宙学与河外天体物理 · 物理学 2019-10-23 Azam Hussain

We investigate the characteristic modifications in the evolving cosmological perturbations when dark energy interacts with dust-like matter, causing the latter's background energy density fall off with time faster than usual. Focusing in…

宇宙学与河外天体物理 · 物理学 2022-04-06 Mohit Kumar Sharma , Sourav Sur

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

Progress in observational cosmology over the past five years has established that the Universe is dominated dynamically by dark matter and dark energy. Both these new and apparently independent forms of matter-energy have properties that…

天体物理学 · 物理学 2009-11-10 J. M. Overduin , P. S. Wesson

Dark matter interactions with electrons or protons during the early Universe leave imprints on the cosmic microwave background and the matter power spectrum, and can be probed through cosmological and astrophysical observations. These…

宇宙学与河外天体物理 · 物理学 2022-04-06 Manuel A. Buen-Abad , Rouven Essig , David McKeen , Yi-Ming Zhong

We consider the cosmological system with two interacting fluids: dark energy and dark matter, in a homogeneous and isotropic universe with dissipation. The modified gravitational equation for dark matter is solved. The analytic…

广义相对论与量子宇宙学 · 物理学 2015-08-19 I. Brevik , V. V. Obukhov , A. V. Timoshkin

We consider scalar field models of dark energy interacting with dark matter through a coupling proportional to the contraction of the four-derivative of the scalar field with the four-velocity of the dark matter fluid. The coupling is…

广义相对论与量子宇宙学 · 物理学 2018-02-07 Jibitesh Dutta , Wompherdeiki Khyllep , Nicola Tamanini

A cosmological model of dark energy interacting with dark matter and another general component of the universe is considered. The evolution equations for coincidence parameters r and s, which represent the ratios between the dark energy and…

广义相对论与量子宇宙学 · 物理学 2009-10-08 Norman Cruz , Samuel Lepe , Francisco Pena

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

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 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