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相关论文: Particle Production Scenario in an Algebraically C…

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We present a new approach to build models of quintessence interacting with dark or baryonic matter. We use a variational approach for relativistic fluids to realize an effective description of matter fields at the Lagrangian level. The…

广义相对论与量子宇宙学 · 物理学 2015-06-10 Christian G. Boehmer , Nicola Tamanini , Matthew Wright

The description of dark matter as a pressure-less fluid and of dark energy as a cosmological constant, both minimally coupled to gravity, constitutes the basis of the concordance $\Lambda\text{CDM}$ model. However, the concordance model is…

宇宙学与河外天体物理 · 物理学 2024-09-27 Amin Aboubrahim , Pran Nath

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

Particle creation (or annihilation) mechanisms, described by either quantum field theoretical models, or by the thermodynamics of irreversible processes, play an important role in the evolution of the early Universe, like, for example, in…

广义相对论与量子宇宙学 · 物理学 2022-11-03 T. Harko , K. Asadi , H. Moshafi , H. Sheikhahmadi

In this work we present the cosmological dynamics of interacting dark energy models in the framework of particle creation mechanism. The particle creation mechanism presented here describes the true non equilibrium thermodynamics of the…

广义相对论与量子宇宙学 · 物理学 2017-06-07 Sujay Kr. Biswas , Wompherdeiki Khyllep , Jibitesh Dutta , Subenoy Chakraborty

We consider a cosmological scenario endowed with an interaction between the universe's dark components $-$ dark matter and dark energy. Specifically, we assume the dark matter component to be a pressure-less fluid, while the dark energy…

广义相对论与量子宇宙学 · 物理学 2021-08-03 Andronikos Paliathanasis , Genly Leon , Wompherdeiki Khyllep , Jibitesh Dutta , Supriya Pan

We investigate an interacting quintessence dark energy - dark matter scenario and its impact on structure formation by analyzing the evolution of scalar perturbations. The interaction is introduced by incorporating a non-zero source term…

广义相对论与量子宇宙学 · 物理学 2025-02-06 Anirban Chatterjee , Abhijit Bandyopadhyay , Debasish Majumdar

Gravitational particle production has been investigated by using Einstein's gravitational field equations in the presence of a cosmological constant. To study the mechanism of particle creation, the Universe has been considered as a…

广义相对论与量子宇宙学 · 物理学 2020-04-07 Z. Safari , B. Malekolkalami , H. Moshafi

We consider an original variational approach for building new models of quintessence interacting with dark or baryonic matter. The coupling is introduced at the Lagrangian level using a variational formulation for relativistic fluids, where…

广义相对论与量子宇宙学 · 物理学 2015-06-10 Christian G. Boehmer , Nicola Tamanini , Matthew Wright

We entertain the possibility that the phenomena typically attributed to dark matter may have a fundamentally emergent nature, rather than arising from new particle degrees of freedom. To illustrate this idea, we consider a field-theoretic…

高能物理 - 唯象学 · 物理学 2025-11-13 Christian Canete , Archil Kobakhidze

We introduce a new class of interacting dark sector models that couple the intrinsic entropy of dark matter to scalar field dark energy. Using the Lagrangian formulation for relativistic perfect fluids, we construct consistent covariant…

宇宙学与河外天体物理 · 物理学 2026-03-12 Erik Jensko , Elsa M. Teixeira , Vivian Poulin

We discuss how to formulate a quantum field theory of dark energy interacting with dark matter. We show that the proposals based on the assumption that dark matter is made up of heavy particles with masses which are very sensitive to the…

高能物理 - 理论 · 物理学 2017-03-09 Guido D'Amico , Teresa Hamill , Nemanja Kaloper

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

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 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

This study examines interacting quintessence dark energy models and their observational constraints for a general parameterization of the quintessence potential, which encompasses a broad range of popular potentials. Four different forms of…

宇宙学与河外天体物理 · 物理学 2023-07-25 Nandan Roy

We add Dark Matter Dark Energy terms with a quintessence field interacting with a Dark Matter field to a MSSM EW Lagrangian previously used to calculate the magnetic field created during the EWPT. From the expectation value of the…

宇宙学与河外天体物理 · 物理学 2014-04-29 Leonard S. Kisslinger , Steven Casper

We study nonequilibrium thermodynamic properties of a driven one-dimensional quantum fluid by combining nonlinear Luttinger liquid theory with the quantum kinetic equation. In particular, we derive an entropy production consistent with the…

介观与纳米尺度物理 · 物理学 2019-10-09 Edvin G. Idrisov , Thomas L. Schmidt

We investigate how entanglement entropy can drive particle creation, deriving explicit relations between entropy and the radiated particle spectrum, the total number of particles, and the total energy. Particle production is computed for…

量子物理 · 物理学 2026-02-04 Michael R. R. Good , Evgenii Ievlev , Eric V. Linder

Models with dark energy decaying into dark matter have been proposed to solve the coincidence problem in cosmology. We study the effect of such coupling in the matter power spectrum. Due to the interaction, the growth of matter density…

天体物理学 · 物理学 2008-11-26 G. Olivares , F. Atrio-Barandela , D. Pavon
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