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相关论文: Unified dark sector and Hubble-tension alleviation…

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We study the cosmological dynamics of dark energy in a scalar-vector-torsion theory. The vector field is described by the cosmic triad and the scalar field is of the quintessence type with non-minimal coupling to gravity. The coupling to…

广义相对论与量子宇宙学 · 物理学 2023-07-11 Manuel Gonzalez-Espinoza , Giovanni Otalora , Yoelsy Leyva , Joel Saavedra

We describe scalar-bimetric theories where the dynamics of the Universe are governed by two separate metrics, each with an Einstein-Hilbert term. In this setting, the baryonic and dark matter components of the Universe couple to metrics…

广义相对论与量子宇宙学 · 物理学 2018-10-09 Philippe Brax , Patrick Valageas

Scalar fields coupled to dark matter by conformal or disformal transformations give rise to a general class of scalar-tensor theories which leads to a rich phenomenology in a cosmological setting. While this possibility has been studied…

广义相对论与量子宇宙学 · 物理学 2023-08-23 Gabriel Gómez

In the present work, we study a subclass of Horndeski gravity characterized by a non-minimal derivative coupling between a scalar field and the Einstein tensor, as a possible alternative to alleviate the observational tension associated…

宇宙学与河外天体物理 · 物理学 2026-03-17 M. S. Oliveira , F. A. Brito , J. A. V. Campos

I describe a tensor-vector-scalar theory that reconciles the galaxy scale success of modified Newtonian dynamics (MOND) with the cosmological scale evidence for CDM. The theory provides a cosmological basis for MOND in the sense that the…

天体物理学 · 物理学 2009-11-10 R. H. Sanders

A covariant scalar-tensor-vector gravity theory is developed which allows the gravitational constant $G$, a vector field coupling $\omega$ and the vector field mass $\mu$ to vary with space and time. The equations of motion for a test…

广义相对论与量子宇宙学 · 物理学 2021-11-22 J. W. Moffat

A family of simple and minimal extensions of the standard cosmological $\Lambda$CDM model in which dark matter experiences an additional long-range scalar interaction is demonstrated to alleviate the long lasting Hubble-tension while…

宇宙学与河外天体物理 · 物理学 2024-05-08 Jean-Philippe Uzan , Cyril Pitrou

Values of the Hubble constant between the direct measurements from various independent local observations and that inferred from the cosmic microwave background with the $\Lambda$-cold-dark-matter model are in tension with persistent…

宇宙学与河外天体物理 · 物理学 2021-06-09 Rong-Gen Cai , Zong-Kuan Guo , Li Li , Shao-Jiang Wang , Wang-Wei Yu

The discovery of cosmic acceleration motivated extensive studies of dynamical dark energy and modified gravity models. Of particular interest are the scalar-tensor theories, with a scalar field dark energy non-minimally coupled to matter.…

宇宙学与河外天体物理 · 物理学 2023-08-14 Seyed Hamidreza Mirpoorian , Zhuangfei Wang , Levon Pogosian

The presently open problem of the Hubble tension is shown to be removed in the context of a modified theory of gravity with a non-minimal coupling between curvature and matter. By evolving the cosmological parameters that match the cosmic…

广义相对论与量子宇宙学 · 物理学 2024-10-22 Miguel Barroso Varela , Orfeu Bertolami

We consider a universe with a positive effective cosmological constant and a nonminimally coupled scalar field. When the coupling constant is negative, the scalar field exhibits linear growth at asymptotically late times, resulting in a…

广义相对论与量子宇宙学 · 物理学 2015-04-06 Dražen Glavan , Tomislav Prokopec

Early dark energy solutions to the Hubble tension introduce an additional scalar field which is frozen at early times but becomes dynamical around matter-radiation equality. In order to alleviate the tension, the scalar's share of the total…

高能物理 - 唯象学 · 物理学 2025-04-01 Marc Kamionkowski , Anubhav Mathur

We explore a novel cosmological model based on coupled fields in the framework of scalar tensor theories, considering the specific interplay between gravity and scalar fields. The model further extends a recent axion-dilaton system by…

广义相对论与量子宇宙学 · 物理学 2025-11-25 Mihai Marciu

We construct a family of viable scalar-tensor models of dark energy (DE) which possess a phase of late-time acceleration preceded by a standard matter era, while at the same time satisfying the local gravity constraints (LGC). The coupling…

天体物理学 · 物理学 2008-11-26 Shinji Tsujikawa , Kotub Uddin , Shuntaro Mizuno , Reza Tavakol , Jun'ichi Yokoyama

We investigate the Hubble constant tension within $f(R)$ modified gravity in the Jordan frame, focusing on its application to the dynamics of an isotropic Universe. A scalar field, non-minimally coupled to the metric, provides an extra…

广义相对论与量子宇宙学 · 物理学 2024-11-07 Tiziano Schiavone , Giovanni Montani

The reason for the present accelerated expansion of the Universe stands as one of the most profound questions in the realm of science, with deep connections to both cosmology and fundamental physics. From a cosmological point of view,…

广义相对论与量子宇宙学 · 物理学 2024-08-22 Peixiang Ji , Lijing Shao

We study the dynamical aspects of dark energy in the context of a non-minimally coupled scalar field with curvature and torsion. Whereas the scalar field acts as the source of the trace mode of torsion, a suitable constraint on the torsion…

广义相对论与量子宇宙学 · 物理学 2017-08-18 Sourav Sur , Arshdeep Singh Bhatia

We propose a unified scalar-field framework that addresses, within standard general relativity, three current cosmological anomalies: the $H_0$ tension, the mild preference for reduced late-time clustering ($S_8$), and recent indications of…

宇宙学与河外天体物理 · 物理学 2026-03-13 Gerasimos Kouniatalis

A simple and minimal extension of the standard cosmological $\Lambda$CDM model in which dark matter experiences an additional long-range scalar interaction is demonstrated to alleviate the long lasting Hubble-tension while letting…

宇宙学与河外天体物理 · 物理学 2024-05-08 Cyril Pitrou , Jean-Philippe Uzan

A conformal coupling of the metric in the Jordan frame to the energy-momentum tensor, screens the scalar field gravitational coupling strength $G$ in modified gravity (MOG). The scalar field acquires a mass which depends on the local matter…

广义相对论与量子宇宙学 · 物理学 2014-10-14 J. W. Moffat
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