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相关论文: Non-linear Phenomenology of Disformally Coupled Qu…

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This paper is concerned with theories of gravity that contain a scalar coupled both conformally and disformally to matter through the metric. By systematically deriving the non-relativistic limit, it is shown that no new non-linear…

宇宙学与河外天体物理 · 物理学 2014-12-10 Jeremy Sakstein

The late-time cosmological dynamics of disformal gravity are investigated using dynamical systems methods. It is shown that in the general case there are no stable attractors that screen fifth-forces locally and simultaneously describe a…

宇宙学与河外天体物理 · 物理学 2015-06-23 Jeremy Sakstein

In Einstein's General Relativity (GR), the gravitational interactions are described by the spacetime curvature. Recently, other alternative geometric formulations and representations of GR have emerged in which the gravitational…

广义相对论与量子宇宙学 · 物理学 2023-08-16 A. Hanin , M. Koussour , Z. Sakhi , M. Bennai

In this work we consider a cosmological model in which dark energy is portrayed by a canonical scalar field which is allowed to couple to the other species by means of a disformal transformation of the metric. We revisit the current…

广义相对论与量子宇宙学 · 物理学 2020-04-06 Elsa M. Teixeira , Ana Nunes , Nelson J. Nunes

Brans--Dicke scalar--tensor theory provides a conformally coupling of the scalar field with gravity in Einstein's frame. This model is equivalent to an interacting quintessence in which dark matter is coupled to dark energy. This provides a…

广义相对论与量子宇宙学 · 物理学 2015-05-30 Fatimah Shojai , Ali Shojai

We consider a cosmology in which dark matter and a quintessence scalar field responsible for the acceleration of the Universe are allowed to interact. Allowing for both conformal and disformal couplings, we perform a global analysis of the…

宇宙学与河外天体物理 · 物理学 2017-02-22 Carsten van de Bruck , Jurgen Mifsud , Jack Morrice

One of the main technical obstacles in constructing a consistent theory of quantum gravity is that the metric itself defines the causal structure required for quantization. This motivates implementing quantum aspects of gravity through an…

广义相对论与量子宇宙学 · 物理学 2025-12-16 Johas Morales , Yuri Bonder

The coupled quintessence model with disformal couplings is treated here to mimic the $\Lambda$CDM background. Using this approach, the quintessence potential does not have to be specified. The model considers a generic fluid coupled to the…

广义相对论与量子宇宙学 · 物理学 2021-03-16 Avishek Dusoye , Alvaro de la Cruz-Dombriz , Peter Dunsby , Nelson J. Nunes

We discuss some of the issues which we encounter when we try to invoke the scalar-tensor theories of gravitation as a theoretical basis of quintessence. One of the advantages of appealing to these theories is that they allow us to implement…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Yasunori Fujii

We investigate statistical properties of the distribution of matter at redshift zero in disformal gravity by using N-body simulations. The disformal model studied here consists of a conformally coupled symmetron field with an additional…

宇宙学与河外天体物理 · 物理学 2015-12-15 R. Hagala , C. Llinares , D. F. Mota

We consider a model of Quantum Gravity phenomenology, based on the idea that space-time may have some unknown granular structure that respects the Lorentz symmetry. The proposal involves non-trivial couplings of curvature to matter fields…

广义相对论与量子宇宙学 · 物理学 2008-01-21 Y. Bonder

Dynamical vacuum energy or quintessence, a slowly varying and spatially inhomogeneous component of the energy density with negative pressure, is currently consistent with the observational data. One potential difficulty with the idea of…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Takeshi Chiba

We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark matter and the dark energy components of the cosmic fluid. The kind of coupling chosen is inspired in scalar-tensor theories of gravity. We…

天体物理学 · 物理学 2009-11-13 Tame Gonzalez , Genly Leon , Israel Quiros

We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark matter and the dark energy components of the cosmic fluid. The kind of coupling chosen is inspired in scalar-tensor theories of gravity. We…

天体物理学 · 物理学 2007-05-23 Tame Gonzalez , Genly Leon , Israel Quiros

In this paper we present a cosmological model arising from a non-conservative gravitational theory proposed in [PRD 95, 101501(R) (2017)]. The novel feature where comparing with previous implementations of dissipative effects in gravity is…

广义相对论与量子宇宙学 · 物理学 2018-05-28 Júlio C. Fabris , Hermano Velten , Thiago R. P. Caramês , Matheus J. Lazo , Gastão S. F. Frederico

These notes summarize a set of lectures on phenomenological quantum gravity which one of us delivered and the other attended with great diligence. They cover an assortment of topics on the border between theoretical quantum gravity and…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Dagny Kimberly , Joao Magueijo

In this mini-review we discuss first why we should investigate cosmological models beyond LCDM. We then show how to describe dark energy or modified gravity models in a fluid language with the help of one background and two perturbation…

宇宙学与河外天体物理 · 物理学 2012-09-24 Martin Kunz

We show how the scalar field, a candidate of quintessence, in a proposed model of the scalar-tensor theories of gravity provides a way to understand a small but nonzero cosmological constant as indicated by recent observations. A particular…

广义相对论与量子宇宙学 · 物理学 2009-09-25 Yasunori Fujii

We describe a refined version of a previous proposal for the exploration of quantum gravity phenomenology. Unlike the original scheme, the one presented here is free from sign ambiguities while it shares with the previous one the essential…

广义相对论与量子宇宙学 · 物理学 2015-05-13 Yuri Bonder , Daniel Sudarsky

It is shown that a disformally coupled theory in which the gravitational sector has the Einstein-Hilbert form is equivalent to a quartic DBI Galileon Lagrangian, possessing non-linear higher derivative interactions, and hence allowing for…

宇宙学与河外天体物理 · 物理学 2013-05-02 Miguel Zumalacarregui , Tomi S. Koivisto , David F. Mota
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