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Phenomenological fluids from interacting tachyonic scalar fields (Q458065)

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Language	Label	Description	Also known as
English	Phenomenological fluids from interacting tachyonic scalar fields	scientific article

Statements

scholarly article

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Phenomenological fluids from interacting tachyonic scalar fields (English)

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International Journal of Theoretical Physics

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publication date

30 September 2014

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full work available at URL

https://arxiv.org/abs/1308.5364

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zbMATH Keywords

FRW cosmology

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dark energy

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phenomenology

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Martiros Khurshudyan

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Margarit Hakobyan

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MaRDI profile type

MaRDI publication profile

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Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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Interacting entropy-corrected holographic dark energy and IR cut-off length

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Viscous generalized Chaplygin gas with arbitrary \(\alpha\)

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Deflection angle and R-charged black holes

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Viscous varying generalized Chaplygin gas with cosmological constant and space curvature

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Phenomenological varying modified Chaplygin gas with variable \(G\) and \(\Lambda\): toy models for our universe

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Can an interacting varying Chaplygin gas and tachyonic matter accelerate universe?

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Effect of varying bulk viscosity on generalized Chaplygin gas

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Time-dependent density of modified cosmic Chaplygin gas with variable cosmological constant in non-flat universe

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A tachyonic scalar field with mutually interacting components

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PARAMETRIZATIONS OF THE DARK ENERGY DENSITY AND SCALAR POTENTIALS

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Phantom evolution in power-law potentials

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QUINTOM COSMOLOGY WITH GENERAL POTENTIALS

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THEORETICAL ASPECTS OF QUINTOM MODELS

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Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy

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A TRACKER SOLUTION FOR A HOLOGRAPHIC DARK ENERGY MODEL

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Holographic dark energy in braneworld models with a Gauss-Bonnet term in the bulk. Interacting behavior and the \(w=-1\) crossing

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A dark energy model characterized by the age of the Universe

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INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY

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STABLE SUPER-INFLATING COSMOLOGICAL SOLUTIONS IN f(R)-GRAVITY

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Matter bounce cosmology with the <i>f</i> ( <i>T</i> ) gravity

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Inhomogeneity-induced cosmic acceleration in a dust universe

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Cosmological Constraints on the Sign-Changeable Interactions

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Cosmological evolution of quintessence and phantom with a new type of interaction in dark sector

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Validity of the generalized second law of thermodynamics in the logamediate and intermediate scenarios of the universe

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Holographic Ricci dark energy model

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Scenario of accelerating universe: role of phenomenological \(\varLambda\) models

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Identifiers

zbMATH Open document ID

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Mathematics Subject Classification ID

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zbMATH DE Number

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10.1007/S10773-014-2025-9

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Sitelinks

Mathematics(1 entry)

mardi Publication:458065

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