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相关论文: Light scalar dark matter coupled to a trace of ene…

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We present a scenario in which a scalar field dark energy is coupled to the trace of the energy momentum tensor of the baryonic matter fields. In the slow-roll regime, this interaction could give rise to the cosmological features of dark…

宇宙学与河外天体物理 · 物理学 2011-02-02 Alejandro Aviles , Jorge L. Cervantes-Cota

We investigate scalar-tensor theories, motivated by dark energy models, in the strong gravity regime around the black hole at the centre of our galaxy. In such theories general relativity is modified since the scalar field couples to…

宇宙学与河外天体物理 · 物理学 2022-01-24 David Benisty , Anne-Christine Davis

We study the effect of an explicit interaction between two scalar fields components describing dark matter in the context of a recent proposal framework for interaction. We find that, even assuming a very small coupling, it is sufficient to…

宇宙学与河外天体物理 · 物理学 2020-10-28 Victor H. Cardenas , Samuel Lepe

In this work we investigate the evolution of a Universe consisted of a scalar field, a dark matter field and non-interacting baryonic matter and radiation. The scalar field, which plays the role of dark energy, is non-minimally coupled to…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. B. Binder , G. M. Kremer

Scalar dark matter can interact with Standard Model (SM) particles, altering the fundamental constants of Nature in the process. Changes in the fundamental constants during and prior to Big Bang nucleosynthesis (BBN) produce changes in the…

宇宙学与河外天体物理 · 物理学 2015-04-14 Y. V. Stadnik , V. V. Flambaum

Dark matter interacts gravitationally, but it presumably interacts weakly through other channels, especially with respect to regular luminous matter. We look at different ways in which dark matter may couple to other fields. We briefly…

综合物理 · 物理学 2018-09-27 Kevin J. Ludwick

In this work it is investigated the evolution of a Universe where a scalar field, non-minimally coupled to space-time curvature, plays the role of quintessence and drives the Universe to a present accelerated expansion. A non-relativistic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 J. B. Binder , G. M. Kremer

We present three distinct types of models of dark energy in the form of a scalar field which is explicitly coupled to dark matter. Our construction draws from the pull-back formalism for fluids and generalises the fluid action to involve…

宇宙学与河外天体物理 · 物理学 2013-10-11 A. Pourtsidou , C. Skordis , E. J. Copeland

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

In this work we perform some studies related to dark energy. Firstly, we propose a dynamical approach to explain the dark energy content of the universe. We assume that a massless scalar field couples to the Hubble parameter with some…

高能物理 - 唯象学 · 物理学 2009-01-07 Fei Wang , Jin Min Yang

The main aim of this work is to explore the possibility that cold dark matter (CDM) and early dark energy (EDE) can be described by canonical scalar fields that are coupled at the level of its conservation equations. The formalism covers…

宇宙学与河外天体物理 · 物理学 2024-08-02 Gabriela Garcia-Arroyo , L. Arturo Ureña-López , J. Alberto Vázquez

We propose to search for scalar dark matter via its effects on the electromagnetic fine-structure constant and particle masses. Scalar dark matter that forms an oscillating classical field produces `slow' linear-in-time drifts and…

高能物理 - 唯象学 · 物理学 2015-11-16 Yevgeny V. Stadnik , Benjamin M. Roberts , Victor V. Flambaum , Vladimir A. Dzuba

The cosmic evolution of a dark matter model which behaves relativistically in the early Universe is explored. Dark matter is described as a complex scalar field, whose earliest evolution is characterized by a stiff equation of state ($p…

宇宙学与河外天体物理 · 物理学 2015-12-11 Tanja Rindler-Daller , Bohua Li , Paul R. Shapiro , Marek Lewicki , James D. Wells

We explore unification of dark matter and dark energy in a theory containing a scalar field of non-Lagrangian type, obtained by direct insertion of a kinetic term into the energy-momentum tensor. This scalar is different from quintessence,…

宇宙学与河外天体物理 · 物理学 2013-05-29 Changjun Gao , Martin Kunz , Andrew R Liddle , David Parkinson

We consider the cosmological dynamics of a scalar field in a potential with multiple troughs and peaks. We show that the dynamics of the scalar field will evolve from light dark matter-like behaviour (such as that of a light axion) to a…

宇宙学与河外天体物理 · 物理学 2018-07-04 Takeshi Kobayashi , Pedro G. Ferreira

Quasi-constant external fields in nonlinear electromagnetism generate a contribution to the energy-momentum tensor with the form of dark energy. To provide a thorough understanding of the origin and strength of the effects, we undertake a…

高能物理 - 理论 · 物理学 2010-04-14 Lance Labun , Johann Rafelski

The nature of the cosmological dark matter remains elusive. Recent studies have advocated the possibility that dark matter could be composed of ultra-light, self-interacting bosons, forming a Bose-Einstein condensate in the very early…

宇宙学与河外天体物理 · 物理学 2014-04-22 Tanja Rindler-Daller , Paul R. Shapiro

Diverse cosmological and astrophysical observations strongly hint at the presence of dark matter and dark energy in the Universe. One of the main goals of Cosmology is to explain the nature of these two components. It may well be that both…

高能物理 - 理论 · 物理学 2023-07-10 Carsten van de Bruck , Gaspard Poulot , Elsa M. Teixeira

In this work we present a model of dark matter based on scalar-tensor theory of gravity. With this scalar field dark matter model we study the non-linear evolution of the large scale structures in the universe. The equations that govern the…

宇宙学与河外天体物理 · 物理学 2015-06-03 Mario A. Rodriguez-Meza

We investigate an interacting dark energy model which allows for the kinetic term of the scalar field to couple to dark matter via a power-law interaction. The model is characterised by scaling solutions at early times, which are of high…

宇宙学与河外天体物理 · 物理学 2022-12-06 Elsa M. Teixeira , Bruno J. Barros , Vasco M. C. Ferreira , Noemi Frusciante
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