Reconstruction of cosmic history from a simple parametrization of H
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Publication:5370975
DOI10.1142/S0219887817501110zbMath1376.83034arXiv1609.02801MaRDI QIDQ5370975
S. K. J. Pacif, Shynaray Myrzakul, Ratbay Myrzakulov
Publication date: 20 October 2017
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1609.02801
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
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Cites Work
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- LRS Bianchi type-I perfect fluid cosmological model with modified generalized chaplygin gas equation of state
- Cosmological models with linearly varying deceleration parameter
- Bouncing cosmology in modified Gauss-Bonnet gravity
- An exact Chameleon cosmological model unifying phantom inflation with late-time acceleration
- A new variable modified Chaplygin gas model interacting with a scalar field
- Cosmological models with variable cosmological and gravitational ``constants and bulk viscous models
- Scenario of inflationary cosmology from the phenomenological \(\Lambda \) models
- Viscous inflationary universe models
- A critical density cosmological model with varying gravitational and cosmological ``constants
- Generalized Chaplygin gas model: dark energy -- dark matter unification and CMBR con\-straints
- Quantum de Sitter cosmology and phantom matter
- FRW-type universe with vacuum energy density
- Singular inflation from generalized equation of state fluids
- Role of deceleration parameter and interacting dark energy in singularity avoidance
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Acceleration of the universe with a simple trigonometric potential
- Consequences on variable Λ-models from distant type Ia supernovae and compact radio sources
- Anisotropic dark energy model with a hybrid scale factor
- A divergence-free parametrization of deceleration parameter for scalar field dark energy
- CHAMELEON COSMOLOGY MODEL DESCRIBING THE PHANTOM DIVIDE LINE CROSSING
- The cosmological constant and dark energy
- Late-time cosmic acceleration: ABCD of dark energy and modified theories of gravity
- Exact scalar field cosmologies
- DYNAMICS OF DARK ENERGY
- A Machian approach to general relativity
- CONSTRAINTS TO DECELERATION PARAMETERS BY RECENT COSMIC OBSERVATIONS
- Role of modified Chaplygin gas in accelerated universe
- A programme for a problem-free cosmology within the framework of a rich class of scalar-tensor theories
- THEORETICAL MODELS OF DARK ENERGY
- Unification of inflation and dark energyà laquintessential inflation
- FIELD THEORY OF TACHYON MATTER
- QUINTOM COSMOLOGY WITH GENERAL POTENTIALS
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Cosmological Imprint of an Energy Component with General Equation of State
- The cosmological constant problem
- \(k\)-inflation
- An alternative to quintessence
- Study of the magnitude-redshift relation for type Ia supernovae in a model resulting from a Ricci-symmetry
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