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This work is focused on the exploration of the thermodynamics foundations of the matter creation scenario when a generalized form of the second law of thermodynamics for this scheme is implemented. In this scenario we consider an expanding…

广义相对论与量子宇宙学 · 物理学 2024-07-23 Víctor H. Cárdenas , Miguel Cruz , Samuel Lepe

We perform a study both statistical and theoretical for cosmological models of matter creation and their ability to describe effective phantom models of dark energy. Such models are beyond the $\Lambda$CDM model since the resulting cosmic…

广义相对论与量子宇宙学 · 物理学 2020-04-23 Víctor H. Cárdenas , Miguel Cruz , Samuel Lepe , Shin'ichi Nojiri , Sergei D. Odintsov

In the context of thermodynamics we discuss the way inevitable emerge an interaction between dark components, and in this way, provide a mechanism to understand the limits of the LCDM model and the class of interaction models between dark…

宇宙学与河外天体物理 · 物理学 2019-05-22 Víctor H. Cárdenas , Daniela Grandón , Samuel Lepe

We investigate the cosmological evolution of mimetic matter model with arbitrary scalar potential. The cosmological reconstruction, which is the way to construct a model for arbitrary evolutions of the scale factor, is explicitly done for…

广义相对论与量子宇宙学 · 物理学 2015-04-01 Jiro Matsumoto , Sergei D. Odintsov , Sergey V. Sushkov

We examine an extension of the quintom scenario of dark energy, in which a canonical scalar field and a phantom field are coupled through a kinetic interaction. We perform a phase space analysis and show that the kinetic coupling gives rise…

高能物理 - 理论 · 物理学 2014-11-20 Emmanuel N. Saridakis , Joel M. Weller

We consider a model where both dark energy and dark matter originate from the coupling of a scalar field with a non-conventional kinetic term to, both, a metric measure and a non-metric measure. An interacting dark energy/dark matter…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Stefano Ansoldi , Eduardo I. Guendelman

Recent results from the Dark Energy Spectroscopic Instrument (DESI) provide evidence for a dynamical dark-energy component, whose equation of state appears to have recently crossed the phantom divide. In this Letter, we present an…

宇宙学与河外天体物理 · 物理学 2026-05-20 E. Abdalla , O. P. F. Piedra , A. A. Escobal , A. M. Vicente , F. B. Abdalla , B. Wang , A. Marins

We revise the cosmological interaction between dark energy and dark matter. More precisely, we focus on models that support compartmentalization or co-existence in the dark sector of the universe. Within the framework of a homogeneous and…

广义相对论与量子宇宙学 · 物理学 2024-11-25 Andronikos Paliathanasis , Kevin Duffy , Amlan Halder , Amare Abebe

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

The cosmological abundance of dark matter can be significantly influenced by the temperature dependence of particle masses and vacuum expectation values. We illustrate this point in three simple freeze-in models. The first one, which we…

高能物理 - 唯象学 · 物理学 2019-07-08 Michael J. Baker , Moritz Breitbach , Joachim Kopp , Lukas Mittnacht

Non-conservation of dark matter can lead to late-time cosmic acceleration. This mechanism is known as the matter creation theory and this replaces the need of dark energy and modified gravity theories. We consider a two-fluid system…

广义相对论与量子宇宙学 · 物理学 2025-12-02 Sudip Halder , Jaume de Haro , Supriya Pan , Tapan Saha , Subenoy Chakraborty

An interacting dark energy model with interaction term $Q= \lambda_m H\rho_m+\lambda_dH\rho_d$ is considered. By studying the model near the transition time, in which the system crosses the w=-1 phantom-divide-line, the conditions needed to…

广义相对论与量子宇宙学 · 物理学 2008-11-26 H. Mohseni Sadjadi , M. Alimohammadi

We argue that interactions in the dark sector may have a crucial impact on the cosmological dynamics. In particular, the future cosmic evolution may be very different from that predicted by the LCDM model. An example is a scenario in which…

宇宙学与河外天体物理 · 物理学 2013-02-07 W. Zimdahl , C. Z. Vargas , W. S. Hipólito-Ricaldi

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 perform a detailed phase-space analysis of various phantom cosmological models, where the dark energy sector interacts with the dark matter one. We examine whether there exist late-time scaling attractors, corresponding to an…

广义相对论与量子宇宙学 · 物理学 2009-12-04 Xi-ming Chen , Yungui Gong , Emmanuel N. Saridakis

The existence of dark matter and dark energy in cosmology is implied by various observations, however, they are still unclear because they have not been directly detected. In this Letter, an unified model of dark energy and dark matter that…

宇宙学与河外天体物理 · 物理学 2016-10-27 Jiro Matsumoto

Dark matter may be coupled to dark radiation: light degrees of freedom that mediate forces between dark sector particles. Cosmological constraints favor dark radiation that is colder than Standard Model radiation. In models with fixed…

高能物理 - 唯象学 · 物理学 2016-10-12 Matthew Reece , Thomas Roxlo

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

Models in which dark energy interacts with dark matter have been proposed in the literature to help explain why dark energy should only come to dominate in recent times. In this paper, we present a dynamical framework to calculate…

天体物理学 · 物理学 2009-03-12 Sirichai Chongchitnan

We analyse three cosmological scenarios with interaction in the dark sector, which are particular cases of a general expression for the energy flux from vacuum to matter. In the first case the interaction leads to a transition from an…

宇宙学与河外天体物理 · 物理学 2015-03-31 L. P. Chimento , S. Carneiro
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