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相关论文: Cosmological constraints on interacting dark energ…

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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…

宇宙学与河外天体物理 · 物理学 2019-08-21 Mahnaz Asghari , Jose Beltran Jimenez , Shahram Khosravi , David F. Mota

The local measurement of $H_0$ is in tension with the prediction of $\Lambda$CDM model based on the Planck data. This tension may imply that dark energy is strengthened in the late-time Universe. We employ the latest cosmological…

宇宙学与河外天体物理 · 物理学 2016-10-25 Dong-Mei Xia , Sai Wang

It is possible that there exist some interactions between dark energy (DE) and dark matter (DM), and a suitable interaction can alleviate the coincidence problem. Several phenomenological interacting forms are proposed and are fitted with…

宇宙学与河外天体物理 · 物理学 2010-05-25 Rong-Gen Cai , Qiping Su

The interacting and holographic dark energy models involve two important quantities. One is the characteristic size of the holographic bound and the other is the coupling term of the interaction between dark energy and dark matter. Rather…

高能物理 - 理论 · 物理学 2008-11-26 Bo Hu , Yi Ling

We explore an interacting dark sector model in trace-free Einstein gravity where dark energy has a constant equation of state, $w=-1$, and the energy-momentum transfer potential is proportional to the cold dark matter density. Compared to…

宇宙学与河外天体物理 · 物理学 2025-03-21 Yuejia Zhai , Marco de Cesare , Carsten van de Bruck , Eleonora Di Valentino , Edward Wilson-Ewing

We present improved constraints on an interacting vacuum model using updated astronomical observations including the first data release from Planck. We consider a model with one dimensionless parameter, $\alpha$, describing the interaction…

宇宙学与河外天体物理 · 物理学 2014-07-09 Yuting Wang , David Wands , Gong-Bo Zhao , Lixin Xu

Dark energy might interact with dark matter in a direct, non-gravitational way, which can help remedy several theoretical defects. In order to find out the properties of interacting dark energy models, it is necessary to investigate the…

宇宙学与河外天体物理 · 物理学 2019-05-15 Ji-Ping Dai , Junqing Xia

We investigate interacting scenarios which belong to a wider class, since they include a dynamical dark energy component whose equation of state follows various one-parameter parametrizations. We confront them with the latest observational…

宇宙学与河外天体物理 · 物理学 2019-11-20 Supriya Pan , Weiqiang Yang , Eleonora Di Valentino , Emmanuel N. Saridakis , Subenoy Chakraborty

Models of interacting dark energy and dark matter offer a possible solution to cosmological tensions. In this work, we examine a pure momentum-exchange model with a time-dependent coupling strength $\xi(z)$ that could help to alleviate the…

宇宙学与河外天体物理 · 物理学 2025-10-28 Nathan Cruickshank , Robert Crittenden , Kazuya Koyama , Marco Bruni

We use the latest compilation of observational Hubble parameter measurements estimated with the differential evolution of cosmic chronometers, in combination with the local value of the Hubble constant recently measured with 2.4% precision,…

宇宙学与河外天体物理 · 物理学 2016-07-13 Rafael C. Nunes , Supriya Pan , Emmanuel N. Saridakis

We reconsider the dynamics of the Universe in the presence of interactions in the cosmological dark sector. A class of interacting models is introduced via a real function $f\left(r\right)$ of the ratio $r$ between the energy densities of…

宇宙学与河外天体物理 · 物理学 2019-01-09 R. von Marttens , L. Casarini , D. F. Mota , W. Zimdahl

Modern Cosmology offers us a great understanding of the universe with striking precision, made possible by the modern technologies of the newest generations of telescopes. The standard cosmological model, however, is not absent of…

宇宙学与河外天体物理 · 物理学 2016-10-06 Rafael J. F. Marcondes

We study the dynamical behaviour of the interacting holographic dark energy model whose interaction term is $Q=3H(\lam_d\rho_d + \lam_c\rho_c)$, where $\rho_d$ and $\rho_c$ are the energy density of dark energy and CDM respectively. To…

天体物理学 · 物理学 2008-11-26 Khamphee Karwan

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

In this work the observational constraints on interaction coupling parameter between dynamical dark energy and cold dark matter were obtained using CMB, BAO and SN Ia data. The dark energy in considered models is dynamical and evolution of…

宇宙学与河外天体物理 · 物理学 2025-12-17 Roman Neomenko

We show that an interaction between dark matter and dark energy generically results in an effective dark energy equation of state of w<-1. This arises because the interaction alters the redshift-dependence of the matter density. An observer…

天体物理学 · 物理学 2010-03-26 Subinoy Das , Pier Stefano Corasaniti , Justin Khoury

Assuming a non-gravitational interaction amongst the dark fluids of our universe namely, the dark matter and dark energy, we study a specific interaction model in the background of a spatially flat Friedmann-Lema\^itre-Robertson-Walker…

广义相对论与量子宇宙学 · 物理学 2018-08-29 Weiqiang Yang , Supriya Pan , Ramón Herrera , Subenoy Chakraborty

We revisit a class of coupled dark energy models where dark energy interacts with dark matter via phenomenological energy exchange terms. We include the perturbation of the Hubble rate in the interaction term, which was absent in previous…

宇宙学与河外天体物理 · 物理学 2025-07-16 Gabriel A. Hoerning , Ricardo G. Landim , Luiza O. Ponte , Raphael P. Rolim , Filipe B. Abdalla , Elcio Abdalla

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

The recent observational evidence for the current cosmic acceleration have stimulated renewed interest in alternative cosmologies, such as scenarios with interaction in the dark sector (dark matter and dark energy). In general, such models…

宇宙学与河外天体物理 · 物理学 2009-10-22 R. S. Goncalves , J. S. Alcaniz , A. Dev , D. Jain