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相关论文: Cosmological model with interactions in the dark s…

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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

Basic cosmology describes the universe as a Robertson-Walker model filled with black-body radiation and no barionic matter, and as observational data it uses only the value of the speed of light, the Hubble and deceleration parameters and…

综合物理 · 物理学 2014-03-25 Ll. Bel

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 cosmological consequences of an interacting model in which vacuum decay law is deducted from the effect that vacuum decay has on the dark matter evolution are investigated. Here, the baryonic matter is also considered as a fluid…

宇宙学与河外天体物理 · 物理学 2017-11-27 H. T. C. M. Souza , N. Pires , F. E. M. Costa , F. C. Carvalho , E. P. Bento

We investigate the interaction between dark energy and dark matter in the framework of irreversible thermodynamics of open systems with matter creation/annihilation. We consider dark energy and dark matter as an interacting two component…

广义相对论与量子宇宙学 · 物理学 2013-02-08 Tiberiu Harko , Francisco S. N. Lobo

In this paper we exploit the theory of the dynamical systems to study the dynamics of the standard cosmological model of the universe, which is known as the $\Lambda$CDM model. We assume that the matter content in our universe consists of…

综合物理 · 物理学 2022-09-07 Danijela Branković , Žarko Mijajlović

It may well happen that the two main components of the dark sector of the Universe, dark matter and dark energy, do not evolve separately but interact nongravitationally with one another. However, given our current lack of knowledge on the…

广义相对论与量子宇宙学 · 物理学 2015-07-02 Sergio del Campo , Ramon Herrera , Diego Pavon

This work focuses on two linear interaction models between dark matter and dark energy, which are proposed as key factors in explaining cosmic history, specifically the latetime accelerating expansion of the universe. Both models are…

宇宙学与河外天体物理 · 物理学 2024-12-13 Robert Rugg , Shambel Sahlu , Amare Abebe

Interacting dark energy models are widely renowned for giving an explanation to the cosmic coincidence problem as well as several observational issues. According to the recent observational data, and so far we are concerned with the…

宇宙学与河外天体物理 · 物理学 2020-07-07 Supriya Pan , Weiqiang Yang , Andronikos Paliathanasis

Two exotic elements have been introduced into the standard cosmological model: non-baryonic dark matter and dark energy. The success in converting a hypothesis into a solid theory depends strongly on whether we are able to solve the…

宇宙学与河外天体物理 · 物理学 2020-01-08 Martin Lopez-Corredoira

Models proposing a non-gravitational interaction between dark energy (DE) and dark matter (CDM) have been extensively studied as alternatives to the standard cosmological model. A common approach to describing the DE-CDM coupling assumes it…

宇宙学与河外天体物理 · 物理学 2025-04-22 Jaelsson S. Lima , Rodrigo von Marttens , Luciano Casarini

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

In this study, we explore the impact of the interacting parameter on dark matter in a model resulting from a parametrization of dark energy density. To ensure a model-independent approach, we treat \( r_d \) as a free parameter, avoiding…

广义相对论与量子宇宙学 · 物理学 2025-03-11 Ritika Nagpal , S. K. J. Pacif , Farruh Atamurotov , Rasmikanta Pati

We consider interacting dark matter-dark energy models arising out of a general interaction term $Q=f(\rho_{m},\rho_{d},\dot{\rho}_{m},\dot{\rho}_{d}).$ Here $f$ is a functional relation connecting the energy densities $\rho_{m}$ and…

广义相对论与量子宇宙学 · 物理学 2024-05-24 Subhra Bhattacharya

So far, there have been no theories or observational data that deny the presence of interaction between dark energy and dark matter. We extend naturally the holographic dark energy (HDE) model, proposed by Granda and Oliveros, in which the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Fei Yu , Jingfei Zhang , Jianbo Lu , Wei Wang , Yuanxing Gui

We investigate a phenomenological non-gravitational coupling between dark energy and dark matter, where the interaction in the dark sector is parameterized as an energy transfer either from dark matter to dark energy or the opposite. The…

宇宙学与河外天体物理 · 物理学 2016-04-11 Riccardo Murgia , Stefano Gariazzo , Nicolao Fornengo

The distribution of the non-luminous matter in galaxies of different luminosity and Hubble type is much more than a proof of the existence of dark particles governing the structures of the Universe. Here, we will review the complex but…

星系天体物理 · 物理学 2019-02-25 Paolo Salucci

We have re-investigated Cosmology involving interaction between Dark matter and Dark Energy in the light of a new parametrization. The new parametrization is based on the hypothesis that when Dark matter and Dark Energy will interact, Dark…

宇宙学与河外天体物理 · 物理学 2023-09-20 Arkajit Aich

We examine the evolution of a holographic cosmological model with future event horizon as the infrared cut-off and dark matter and dark energy do not evolve independently $-$ there is interaction between them. The basic evolution equations…

广义相对论与量子宇宙学 · 物理学 2011-06-24 Ritabrata Biswas , Nairwita Mazumder , Subenoy Chakraborty

In models where dark matter and dark energy interact non-minimally, the total amount of matter in a fixed comoving volume may vary from the time of recombination to the present time due to energy transfer between the two components. This…

宇宙学与河外天体物理 · 物理学 2012-10-16 P. P. Avelino , H. M. R. da Silva