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相关论文: Field Theories and Fluids for an Interacting Dark …

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We consider an interacting field theory model that describes the dark energy - dark matter interaction. Only for a specific interaction term, this interacting field theory description has an equivalent interacting fluid description. For…

宇宙学与河外天体物理 · 物理学 2022-01-26 Joseph P Johnson , Archana Sangwan , S. Shankaranarayanan

There is no unique way to describe the dark energy-dark matter interaction, as we have little information about the nature and dynamics of the dark sector. Hence, in many of the phenomenological dark matter fluid interaction models in the…

广义相对论与量子宇宙学 · 物理学 2021-01-13 Joseph P Johnson , S. Shankaranarayanan

The strange behaviour of the universe's dark sector offers us the flexibility to address cosmological problems with different approaches. Using this flexibility, we consider a possible exchange of energy among the dark sector components as…

广义相对论与量子宇宙学 · 物理学 2023-02-14 Trupti Patil , Sukanta Panda , Manabendra Sharma , Ruchika

We study the dynamics of Dirac-Born-Infeld (DBI) dark energy interacting with dark matter. The DBI dark energy model considered here has a scalar field with a nonstandard kinetic energy term, and has potential and brane tension that are…

广义相对论与量子宇宙学 · 物理学 2013-01-07 Chakkrit Kaeonikhom , Douglas Singleton , Sergey V. Sushkov , Nattapong Yongram

In this paper, we will deepen the understanding of some fluid models proposed by other authors for the description of dark energy. Specifically, we will show that the so-called (Modified) Berthelot fluid is the hydrodynamic realization of…

广义相对论与量子宇宙学 · 物理学 2023-01-31 Muhsin Aljaf , Daniele Gregoris , Martiros Khurshudyan

In Cosmology, when dissipative effects are minimal, the energy content of the Universe can be effectively described as a sum of perfect fluids. Perfect fluid descriptions ensure thermal equilibrium since they equilibrate immediately.…

宇宙学与河外天体物理 · 物理学 2024-12-16 Pulkit Bansal , Joseph P Johnson , S. Shankaranarayanan

We consider theories which break the invariance under diffeomorphisms (Diff) down to transverse diffeomorphisms (TDiff) in the matter sector, consisting of multiple scalar fields. In particular, we regard shift-symmetric models with two…

广义相对论与量子宇宙学 · 物理学 2025-01-17 Diego Tessainer , Antonio L. Maroto , Prado Martín-Moruno

A dynamical system analysis related to Dirac Born Infeld (DBI) cosmological model has been investigated in this present work. For spatially flat FRW space time, the Einstein field equation for DBI scenario has been used to study the…

广义相对论与量子宇宙学 · 物理学 2015-01-20 Nilanjana Mahata , Subenoy Chakraborty

Anisotropic dark energy cosmological models are constructed in the frame work of generalised Brans-Dicke theory with a self interacting potential. Wet dark fluid characterized by a linear equation of state is considered as the source of…

综合物理 · 物理学 2017-05-10 Sunil K. Tripathy , Dipanjali Behera , Bivudutta Mishra

We investigate the interaction between the dark sectors from the point of view of a dynamical system analysis. A general setup for interacting dark energy models that incorporates both quintessence and phantom fields through a switch…

广义相对论与量子宇宙学 · 物理学 2025-05-16 Chonticha Kritpetch , Nandan Roy , Narayan Banerjee

Motivated by cosmological applications for interacting matters, an extension of the action functional for relativistic fluids is proposed to incorporate the physics of non-adiabatic processes and chemical reactions. The former are…

广义相对论与量子宇宙学 · 物理学 2025-01-30 Damianos Iosifidis , Erik Jensko , Tomi S. Koivisto

This article examines the foundation of the recently developed relativistic variational formalism[1]. Our work is heavily based on [2, 27] which extends this approach to the multi-fluid theory and examines its utility in astrophysics and…

广义相对论与量子宇宙学 · 物理学 2019-05-22 Bob Osano , Timothy Oreta

Some dark energy cosmological models are constructed in the framework of a generalised Brans-Dicke theory which contains a self interacting potential and a dynamical coupling parameter. The dark sector of the universe is considered through…

广义相对论与量子宇宙学 · 物理学 2022-07-19 S. K. Tripathy , Sasmita K Pradhan , Z. Naik , D. Behera , B. Mishra

Perfect fluids are modeled by using an effective field theory approach which naturally gives a self-consistent and unambiguous description of the intrinsic non-adiabatic contribution to pressure variations. We study the impact of intrinsic…

广义相对论与量子宇宙学 · 物理学 2018-03-28 Marco Celoria , Denis Comelli , Luigi Pilo

In this paper it is shown that in non-minimally coupled Brans-Dicke theory containing a self-interacting potential, a suitable conformal transformation can automatically give rise to an interaction between the normal matter and the…

广义相对论与量子宇宙学 · 物理学 2015-06-18 Sudipta Das , Abdulla Al Mamon

We study observational signatures of non-gravitational interactions between the dark components of the cosmic fluid, which can be either due to creation of dark particles from the expanding vacuum or an effect of the clustering of a…

宇宙学与河外天体物理 · 物理学 2019-12-10 Micol Benetti , Welber Miranda , Humberto A. Borges , Cassio Pigozzo , Saulo Carneiro , Jailson S. Alcaniz

Analogue gravity offers an approach for testing the universality and robustness of quantum field theories in curved spacetimes and validating them using down-to-earth, laboratory-based experiments. Fluid interfaces are a promising framework…

广义相对论与量子宇宙学 · 物理学 2023-06-27 Vitor S. Barroso , Cameron R. D. Bunney , Silke Weinfurtner

I consider couplings between the dark energy and dark matter sectors. I describe how the existence of an adiabatic regime, in which the dark energy field instantaneously tracks the minimum of its effective potential, opens the door for a…

宇宙学与河外天体物理 · 物理学 2009-10-16 Mark Trodden

We propose a field theory model for dark energy and dark matter in interaction. Comparing the classical solutions of the field equations with the observations of the CMB shift parameter, BAO, lookback time and Gold supernovae sample, we…

广义相对论与量子宇宙学 · 物理学 2009-07-30 Sandro Micheletti , Elcio Abdalla , Bin Wang

We consider scalar field models of dark energy interacting with dark matter through a coupling proportional to the contraction of the four-derivative of the scalar field with the four-velocity of the dark matter fluid. The coupling is…

广义相对论与量子宇宙学 · 物理学 2018-02-07 Jibitesh Dutta , Wompherdeiki Khyllep , Nicola Tamanini
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