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The paper proposes a novel cosmological model based on a two-field scenario, where the two fields are independently coupled with a specific invariant, based on cubic contractions of the Riemann tensor. After obtaining the modified Friedmann…

广义相对论与量子宇宙学 · 物理学 2022-07-06 Mihai Marciu

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 study the phase space dynamics of cosmological models in the theoretical formulations of non-minimal metric-torsion couplings with a scalar field, and investigate in particular the critical points which yield stable solutions exhibiting…

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

We study the interaction between dark matter and dark energy, with dark energy described by a scalar field having a double exponential effective potential. We discover conditions under which such a scalar field driven solution is a late…

广义相对论与量子宇宙学 · 物理学 2015-08-06 Vartika Gupta , Rakesh Kabir , Amitabha Mukherjee , Daksh Lohiya

We study the phase space for an scalar-tensor string inspired model of dark energy with non minimal kinetic and Gauss Bonnet couplings. The form of the scalar potential and of the coupling terms is of the exponential type, which give rise…

广义相对论与量子宇宙学 · 物理学 2016-10-12 L. N. Granda , E. Loaiza

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 a scalar field with kinetic term coupled to itself and to the curvature, as a source of dark energy, and analyze the role of this new coupling in the accelerated expansion at large times. In the case of scalar field dominance, the…

高能物理 - 理论 · 物理学 2014-11-20 L. N. Granda

The dynamical properties of a model of dark energy in which two scalar fields are coupled by a non-canonical kinetic term are studied. We show that overall the addition of the coupling has only minor effects on the dynamics of the two-field…

宇宙学与河外天体物理 · 物理学 2014-11-20 Carsten van de Bruck , Joel M. Weller

We present and examine a kinetically coupled tachyon dark energy model, where a tachyon scalar field interacts with the matter sector. More specifically, we deduce this cosmological setting from a generalised interacting dark energy model…

广义相对论与量子宇宙学 · 物理学 2024-12-31 Francesco Pace , Alberto Rozas-Fernández , Özgen Tunç Türker

This study explores the dynamics and phase-space behavior of a multi-component dark energy model, where the dark sector consists of a minimally coupled canonical scalar field and the cosmological constant, using a dynamical system analysis…

广义相对论与量子宇宙学 · 物理学 2025-05-16 Prasanta Sahoo , Nandan Roy , Himadri Shekhar Mondal

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

The main goal of this work is to propose a generalized model of interacting dark energy which allows for the kinetic term of a scalar field to couple to the matter species a priori in the action. We derive the modified field equations, and…

广义相对论与量子宇宙学 · 物理学 2019-04-01 Bruno J. Barros

We discuss the possibility of a scalar field being the fundamental description of dark energy. We focus on shift-symmetric scalar-tensor theories since this symmetry potentially avoids some fine-tuning problems. We also restrict attention…

广义相对论与量子宇宙学 · 物理学 2024-10-07 Teodor Borislavov Vasilev , Mariam Bouhmadi-López , Prado Martín-Moruno

We propose that dark energy in the form of a scalar field could effectively couple to dark matter inhomogeneities. Through this coupling energy could be transferred to/from the scalar field, which could possibly enter an accelerated regime.…

宇宙学与河外天体物理 · 物理学 2016-04-25 Valerio Marra

We present a model where a non-conventional scalar field may act like dark energy leading to cosmic acceleration. The latter is driven by an appropriate field configuration, which result in an effective cosmological constant. The potential…

高能物理 - 理论 · 物理学 2009-11-11 Alex Kehagias

This work explores the dynamical stability of cosmological models where dark matter and dark energy can non-minimally couple to spacetime (scalar) curvature. Two different scenarios are presented here. In the initial case, only dark matter…

广义相对论与量子宇宙学 · 物理学 2023-11-07 Saddam Hussain , Anirban Chatterjee , Kaushik Bhattacharya

We study the dynamical description of scalar-tensor gravity by performing the best-fit analysis for two cases of exponential and power-law form of the potential and scalar field function coupled to the curvature. The models are then tested…

广义相对论与量子宇宙学 · 物理学 2015-06-03 Hossein Farajollahi , Amin Salehi , Mohammad Nasiri

We extend the dynamical systems analysis of Scalar-Fluid interacting dark energy models performed in C. G. Boehmer et al, Phys. Rev. D 91, 123002 (2015), by considering scalar field potentials beyond the exponential type. The properties and…

广义相对论与量子宇宙学 · 物理学 2017-02-01 Jibitesh Dutta , Wompherdeiki Khyllep , Nicola Tamanini

In this work we have studied a cosmological model based on a quintom dark energy model non-minimally coupled with gravity, endowed with a specfic potential energy of the exponential squared type. For this specific type of potential energy…

广义相对论与量子宇宙学 · 物理学 2020-10-28 Mihai Marciu

We use action-angle variables to describe the basic physics of coherent scalar field oscillations in the expanding universe. These analytical mechanics methods have some advantages, like the identification of adiabatic invariants. As an…

天体物理学 · 物理学 2016-08-30 Eduard Masso , Francesc Rota , Gabriel Zsembinszki
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