[PDF] Top 20 Models of disformally coupled dark energy
Has 10000 "Models of disformally coupled dark energy" found on our website. Below are the top 20 most common "Models of disformally coupled dark energy".
Models of disformally coupled dark energy
... examples of scalar fields are the recently detected Higgs field [44], responsible for the mech- anism of providing mass to the particles of the Standard Model of Particle Physics, or the ... See full document
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Impact of dark energy perturbations on the growth index
... values of γ, the indication of modified gravity is not clear ...fðRÞ models, we may have γðzÞ ≲ ...clustering dark energy models. Furthermore, the slope of the growth ... See full document
7
Constraining H0 in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes
... robustness of the shift parameter has been tested by Elgaroy & Multam¨ aki [ 49 ] and compared to fits of the full CMB power spectrum (see also [ 50 ...cosmological models, and this explains why ... See full document
21
Analytic study of cosmological perturbations in a unified model of dark matter and dark energy with a sharp transition
... spite of the limits in which our unified model with piecewise constant equation of state can be obtained from other unified models (such as GCG, the arctan-UDM and the Linder-Huterer model) the fact ... See full document
19
Consequences of dark matter-dark energy interaction on cosmological parameters derived from type Ia supernova data
... mass of the DM parti- cles evolves according to some function of the dark energy field such as, for example, a linear function of the field [12–14] with a inverse power law ... See full document
7
Relaxed Astrophysical Solutions in Non-Minimally Coupled Models
... mimicked dark matter profile for the halo region of a given ...the energy conditions are satisfied under the appropriate range of values for the power law exponent ... See full document
66
Estruturas em larga escala e o Dark Energy Survey
... measurement of its spectra, in which case absorption and emission lines can be used to estimate redshifts by comparing their wavelengths with the known (laboratory) ...evolution models. However, such a ... See full document
175
Clustering dark energy and halo abundances
... amplitude of fluctuations at the redshift of CMB decoupling, clustering DE would have generated more massive clusters in comparison to homogeneous DE, therefore worsening the Planck Clusters ...DE ... See full document
20
Effects of shear and rotation on the spherical collapse model for clustering dark energy
... tens of per cent, keeping though the same qualita- tive behaviour. Models with highest differences are those with the equation-of-state parameter differing mostly from w = ...decrement of 10 ... See full document
12
Constraints on mediator-based dark matter and scalar dark energy models using $\sqrt s = 13$ TeV $pp$ collision data collected by the ATLAS detector
... support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Aus- tralia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and ... See full document
87
Using the fine structure "constant" to probe Dark Energy
... behavior of the equation of state of dark ...evolutions of the equation of states and of the dark energy density parameters we could study the corresponding ... See full document
106
Dark Matter Benchmark Models for Early LHC Run-2 Searches: Report of the ATLAS/CMS Dark Matter Forum
... component of the triplet χ b comprises the cosmological ...example of a t-channel model. Similar top-flavored models can exist, as ...such models will have to be investigate on a longer ... See full document
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Conformal Bulk Fields, Dark Energy and Brane Dynamics
... those of thick branes [29] and non-fine-tuned branes [30] may also be considered (see ...highly coupled 5-dimensional collapse dynamics has been reduced to 4-dimensional ... See full document
12
Expected constraints on dark energy parameters with euclid
... focus of this paper is not exactly the rapidly oscillatory phase that leads the present day acceleration of our ...authors of this article also identify some possible observational signatures that ... See full document
105
Cosmological dynamics of tachyonic teleparallel dark energy
... teleparallel dark energy in ...teleparallel dark energy. Such as in tele- parallel dark energy, in tachyonic teleparallel dark energy the Universe is attracted for ... See full document
8
Dynamical mutation of dark energy
... are models in which this dramatic situation is actually ...analysis of the evolution of perturbations for two gravitationally coupled fluids, dark energy and dark matter ... See full document
4
Exploring teleparallel dark energy
... field coupled to gravity and called “extended quintessence” was pro- posed in ...K-essence models non-minimally coupled to gravity were studied in ...application of the non-minimal coupling to ... See full document
85
Testing cosmological structure formation in unified dark matter-energy models
... procedure of how to test a cosmological ...view of several proposed solutions. Then studying the theoretical details of the model gave me the opportunity to understand in more detail the evolution ... See full document
111
Dark energy as a kinematic effect
... course of history geometry has undergone a remarkable evolution— from Euclid’s axioms through Riemannian manifolds to its present-day description in terms of connections on principal bundles ...theory ... See full document
118
Structure formation in inhomogeneous Early Dark Energy models
... analysis of the number density of halos initially showed that all EDE models provide fewer density of massive clusters, independently of the redshift ...For models with nearly ... See full document
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