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Journal ArticleDOI

Dynamical analysis of interacting running vacuum models in DGP braneworld

TLDR
In this paper, the dynamical properties of varying vacuum cosmology by considering the interaction between the cosmological fluids are discussed and various functional forms (linear and non-linear) of interaction term and apply dynamical system approach.
About
This article is published in Physics of the Dark Universe.The article was published on 2021-12-01. It has received 4 citations till now. The article focuses on the topics: Inflation (cosmology) & Vacuum energy.

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Starobinsky-like inflation and running vacuum in the context of Supergravity

TL;DR: In this paper, the primeval inflationary phase of the early universe was described within a quantum field theoretical framework that can be viewed as the effective action of vacuum decay in the early times.

Phase space analysis of the accelerating multifluid Universe

TL;DR: In this paper, the phase space of a Friedmann-Robertson-Walker universe with various cosmological fluids that may or may not interact is studied, and the physical significance of the resulting fixed points is analyzed.
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Analyzing stability of five-dimensional Einstein Chern–Simons gravity through dynamical systems

TL;DR: In this paper , the cosmological solutions of various models in the realm of five-dimensional Einstein Chern-Simons cosmology were investigated in the context of the late-time accelerated universe.
References
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The Hubble Space Telescope Cluster Supernova Survey. V. Improving the Dark-energy Constraints above z > 1 and Building an Early-type-hosted Supernova Sample

Nao Suzuki, +84 more
TL;DR: In this article, Advanced Camera for Surveys, NICMOS and Keck adaptive-optics-assisted photometry of 20 Type Ia supernovae (SNe Ia) from the Hubble Space Telescope (HST) Cluster Supernova Survey was presented.
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Coupled Quintessence

Luca Amendola
- 03 Aug 1999 - 
TL;DR: The cosmological consequences of such a coupled quintessence (CQ) model, assuming an exponential potential and a linear coupling, were investigated in this article, where the authors evaluated the density perturbations on the cosmic microwave background and on the galaxy distribution at the present and derived bounds on the coupling constant.
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Exponential potentials and cosmological scaling solutions

TL;DR: In this paper, a phase-plane analysis of cosmologies containing a baryotropic fluid and a scalar field with an exponential potential was presented, and it was shown that the scaling solutions are unique late-time attractors whenever they exist.
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Properties of singularities in the (phantom) dark energy universe

TL;DR: In this paper, the properties of future singularities are investigated in the universe dominated by dark energy including the phantom-type fluid. And the authors classify the finite-time singularities into four classes and explicitly present the models which give rise to these singularities by assuming the form of the equation of state of dark energy.
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