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Recently it has been argued that a possible source for the dark energy may arise due to the contribution to the vacuum energy of the QCD ghost in a time-dependent background. In this paper we establish a connection between interacting ghost…

High Energy Physics - Theory · Physics 2012-04-10 A. Sheykhi , M. Sadegh Movahed , E. Ebrahimi

In the teleparallel framework of cosmology, a quintessence with non-minimal couplings to the scalar torsion and a boundary term is considered. A conformal coupling to matter density is also taken into account. It is shown that the model can…

General Relativity and Quantum Cosmology · Physics 2017-06-13 H. Mohseni Sadjadi

Interactions between dark matter and dark energy, allowing both conformal and and disformal couplings, are studied in detail. We discuss the background evolution, anisotropies in the cosmic microwave background and large scale structures.…

General Relativity and Quantum Cosmology · Physics 2015-06-23 C. van de Bruck , J. Morrice

We consider a cosmological scenario where the dark sector is described by two perfect fluids that interact through a velocity-dependent coupling. This coupling gives rise to an interaction in the dark sector driven by the relative velocity…

Cosmology and Nongalactic Astrophysics · Physics 2021-04-14 Jose Beltrán Jiménez , Dario Bettoni , David Figueruelo , Florencia A. Teppa Pannia , Shinji Tsujikawa

We consider a cosmological model with an interaction between dark matter and dark energy which leaves the background cosmology unaffected and only affects the evolution of the perturbations. This is achieved by introducing a coupling given…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-21 Mahnaz Asghari , Jose Beltran Jimenez , Shahram Khosravi , David F. Mota

It has been proposed recently the existence of a non-minimal coupling between a canonical scalar field (quintessence) and gravity in the framework of teleparallel gravity, motivated by similar constructions in the context of General…

General Relativity and Quantum Cosmology · Physics 2013-09-06 G. Otalora

We investigate an interacting quintessence dark energy - dark matter scenario and its impact on structure formation by analyzing the evolution of scalar perturbations. The interaction is introduced by incorporating a non-zero source term…

General Relativity and Quantum Cosmology · Physics 2025-02-06 Anirban Chatterjee , Abhijit Bandyopadhyay , Debasish Majumdar

We place observational constraints on a dark energy (DE) model in which a quintessence scalar field $\phi$ is coupled to dark matter (DM) through momentum and energy exchanges.The momentum transfer is weighed by an interaction between the…

Cosmology and Nongalactic Astrophysics · Physics 2024-03-12 Xiaolin Liu , Shinji Tsujikawa , Kiyotomo Ichiki

In this paper a possibility to accelerated the expansion of the large scale universe due to interacting varying Chaplygin gas of a specific form and a tachyonic matter is considered. A specific form of the potential and appropriate values…

General Physics · Physics 2017-08-16 Martiros Khurshudyan

We suggest a scalar model of dark energy with the SO(1,1) symmetry. The model may be reformulated in terms of a real scalar field $\Phi$ and the scale factor $a$ so that the Lagrangian may be decomposed as that of the real quintessence…

General Relativity and Quantum Cosmology · Physics 2009-11-10 Yi-Huan Wei , Yu Tian

We present evidence that a special class of gravitationally-coupled hidden sectors, in which conformal invariance is dynamically broken in a controlled way, exhibit the properties of dark energy. Such quantum field theories may appear while…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 I. Mocioiu , R. Roiban

We consider a model of interacting cosmological constant/quintessence, where dark matter and dark energy behave as, respectively, two coexisting phases of a fluid, a thermally excited Bose component and a condensate, respectively. In a…

Astrophysics · Physics 2009-11-07 G. Mangano , G. Miele , V. Pettorino

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…

Cosmology and Nongalactic Astrophysics · Physics 2016-08-24 B. Wang , E. Abdalla , F. Atrio-Barandela , D. Pavon

We explore a cosmological model in which dark matter is non-minimally coupled to gravity at the fluid level. While typically subdominant compared to Standard Model forces, such couplings may dominate dark matter dynamics. We show that this…

General Relativity and Quantum Cosmology · Physics 2025-10-14 Samuele Silveravalle , Andrea Lapi , Francesco Benetti , Stefano Liberati

In a recent paper we showed that a quintessence scalar field plus a dissipative matter fluid can drive late cosmic accelerated expansion and simultaneously solve the coincidence problem [1]. In this brief report we extend this result to the…

Astrophysics · Physics 2009-11-07 Luis P. Chimento , Alejandro S. Jakubi , Diego Pavon

Interacting dark energy models may play a crucial role in explaining several important observational issues in modern cosmology and also may provide a solution to current cosmological tensions. Since the phenomenology of the dark sector…

Cosmology and Nongalactic Astrophysics · Physics 2023-12-06 Weiqiang Yang , Supriya Pan , Olga Mena , Eleonora Di Valentino

In this paper we put forward a running coupling scenario for describing the interaction between dark energy and dark matter. The dark sector interaction in our scenario is free of the assumption that the interaction term $Q$ is proportional…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-19 Yun-He Li , Xin Zhang

We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark matter and the dark energy components of the cosmic fluid. The kind of coupling chosen is inspired in scalar-tensor theories of gravity. We…

Astrophysics · Physics 2007-05-23 Tame Gonzalez , Genly Leon , Israel Quiros

We present a type of dark energy models where the particles of dark energy phi are dynamically produced via a quantum transition at very low energies. The scale where the transition takes places depends on the strength g of the interaction…

Cosmology and Nongalactic Astrophysics · Physics 2009-10-12 A. de la Macorra , F. Briscese

In this work, we study two scalar field driven dark energy models characterized by the axion potential and the inverse power law potential, each coupled to dark matter through a momentum exchange interaction. By formulating the dynamics as…

Cosmology and Nongalactic Astrophysics · Physics 2025-06-27 Prasanta Sahoo , Nandan Roy , Himadri Shekhar Mondal
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