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相关论文: Exploring the Possibility of Interacting Quintesse…

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We consider two models of interacting dark energy, both of which interact only through momentum exchange. One is a phenomenological one-parameter extension to $w$CDM, and the other is a coupled quintessence model described by a Lagrangian…

宇宙学与河外天体物理 · 物理学 2022-09-07 Mark S. Linton , Robert Crittenden , Alkistis Pourtsidou

In this paper we consider two models of quintessence scalar fields with different potentials. Interaction with generalized cosmic Chaplygin gas is also investigated. Cosmological parameters are studied and graphical behavior is analyzed. We…

广义相对论与量子宇宙学 · 物理学 2014-07-08 M. Khurshudyan , E. Chubaryan , B. Pourhassan

We perform a detailed analysis of a theoretically motivated dark energy quintessence model which interacts with the dark matter sector of the universe. Utilising the current observational datasets from the Cosmic Microwave Background,…

广义相对论与量子宇宙学 · 物理学 2025-09-12 Atul Ashutosh Samanta , Abhijith Ajith , Sukanta Panda

We study the interacting quintessence model with two different types of interaction by introducing a general parameterization of the quintessence potentials. The form of the quintessence potentials is arbitrary as the recent cosmological…

宇宙学与河外天体物理 · 物理学 2019-06-27 Nandan Roy , Kazuharu Bamba

We derive two field theory models of interacting dark energy, one in which dark energy is associated with the quintessence and another in which it is associated with the tachyon. In both, instead of choosing arbitrarily the potential of…

广义相对论与量子宇宙学 · 物理学 2020-07-10 Sandro M. R. Micheletti

We consider a quintessence model for dark energy interacting with dark matter via a Yukawa interaction. To put constraints on this model we use the CMB measurements from the Planck satellite together with BAO, SNIa and $H_0$ data. We…

宇宙学与河外天体物理 · 物理学 2016-08-08 André A. Costa , Lucas C. Olivari , E. Abdalla

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

We do a detailed analysis of a well-theoretically motivated interacting dark energy scalar field model with a time-varying interaction term. Using current cosmological datasets from CMB, BAO, Type Ia Supernova, $H(z)$ measurements from…

宇宙学与河外天体物理 · 物理学 2024-06-11 Trupti Patil , Ruchika , Sukanta Panda

We investigate the scenario of interacting dark energy through a detailed confrontation with various observational datasets. We quantify the interaction in a general way, through the deviation from the standard scaling of the dark matter…

宇宙学与河外天体物理 · 物理学 2026-01-28 Supriya Pan , Sivasish Paul , Emmanuel N. Saridakis , Weiqiang Yang

In this note, we extend our previous work [Phys. Lett. B 644, 7 (2007), astro-ph/0609597], and compare eleven interacting dark energy models with different couplings to the observational $H(z)$ data. However, none of these models is better…

天体物理学 · 物理学 2008-11-26 Hao Wei , Shuang Nan Zhang

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

Interacting dark energy models have been suggested as alternatives to the standard cosmological model, $\Lambda$CDM. We focus on a phenomenologically interesting class of dark scattering models that is characterised by pure momentum…

宇宙学与河外天体物理 · 物理学 2023-02-08 Maria Tsedrik , Chiara Moretti , Pedro Carrilho , Federico Rizzo , Alkistis Pourtsidou

We employ a ghost model of interacting dark energy to obtain the equation of state \omega for ghost energy density in an FRW universe in complex quintessence theory. We reconstruct the potential and study the dynamics of the scalar field…

高能物理 - 理论 · 物理学 2022-01-04 Yang Liu

Since physics of the dark sector components of the Universe is not yet well-understood, the phenomenological studies of non-minimal interaction in the dark sector could possibly pave the way to theoretical and experimental progress in this…

宇宙学与河外天体物理 · 物理学 2021-08-03 Suresh Kumar

The Standard Model of cosmology, $\Lambda$CDM, while enormously successful, is currently unable to account for several cosmological anomalies the most prominent of which are in the measurements of the Hubble parameter and $S_8$.…

宇宙学与河外天体物理 · 物理学 2025-03-14 Amin Aboubrahim , Pran Nath

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

Cosmological models describing the non-gravitational interaction between dark matter and dark energy are based on some phenomenological choices of the interaction rates between dark matter and dark energy. There is no such guiding rule to…

宇宙学与河外天体物理 · 物理学 2020-06-10 Supriya Pan , German S. Sharov , Weiqiang Yang

We study the global dynamics of the universe within the framework of the Interacting Dark Matter (IDM) scenario. Assuming that the dark matter obeys the collisional Boltzmann equation, we can derive analytical solutions of the global…

天体物理学 · 物理学 2015-05-13 S. Basilakos , M. Plionis

Cosmological models involving an interaction between dark matter and dark energy have been proposed in order to solve the so-called coincidence problem. Different forms of coupling have been studied, but there have been claims that…

天体物理学 · 物理学 2009-06-23 Miguel Quartin , Mauricio O. Calvao , Sergio E. Joras , Ribamar R. R. Reis , Ioav Waga

We determine the range of parameter space of an interacting quintessence (IQ) model that best fits the luminosity distance of type Ia supernovae data and the recent WMAP measurements of Cosmic Microwave Background temperature anisotropies.…

天体物理学 · 物理学 2009-11-13 German Olivares , Fernando Atrio-Barandela , Diego Pavon
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