Dynamical analysis of -essence cosmology in the light of Supernova Ia observations
arXiv:2108.12186 · doi:10.1140/epjp/s13360-022-02747-y
Abstract
In this paper, we analyse the JLA data on Supernova observations in the context of essence dark energy model with Lagrangian , with a constant potential and the dynamical term for a homogeneous scalar field , in a flat FRW spacetime background. Scaling relations are used to extract temporal behaviour of different cosmological quantities and the form of the function from the data. We explore how the parameters of the model, viz. value of the constant potential and a constant appearing in the emergent scaling relation, control the dynamics of the model in the context of JLA data, by setting up and analysing an equivalent dynamical system described by a set of autonomous equations.
arXiv comment22 pages, 7 figures, 3 tables; Accepted for publication in European Physical Journal Plus
References in corpus (64)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- 4D Gravity on a Brane in 5D Minkowski Space
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Accelerating Universes with Scaling Dark Matter
- The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- k-Inflation
- Essentials of k-essence
- The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
- Curvature Quintessence
- The Pan-STARRS1 Photometric System
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
- A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder
- Braneworld models of dark energy
- First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters
- Scaling solutions in general non-minimal coupling theories
- Purely kinetic k-essence as unified dark matter
- Curvature quintessence matched with observational data
- CfA3: 185 Type Ia Supernova Light Curves from the CfA
- Dynamical systems applied to cosmology: dark energy and modified gravity
- The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary
- Cosmological scaling solutions of non-minimally coupled scalar fields
- SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes
- WMAP constraints on low redshift evolution of dark energy
- Extended Quintessence
- The Carnegie Supernova Project: First Photometry Data Release of Low-Redshift Type Ia Supernovae
- The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae
- Quintessence, the Gravitational Constant, and Gravity
- Scalar-Tensor Gravity and Quintessence
- The Carnegie Supernova Project: Second Photometry Data Release of Low-Redshift Type Ia Supernovae
- Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
- Tracking K-essence
- Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data
- First-Year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Constraints on Non-Standard Cosmological Models
- Uncorrelated Measurements of the Cosmic Expansion History and Dark Energy from Supernovae
- Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample
- First-year Sloan Digital Sky Survey-II (SDSS-II) supernova results: consistency and constraints with other intermediate-redshift datasets
- Flux-averaging Analysis of Type Ia Supernova Data
- Cosmology with Photometrically-Classified Type Ia Supernovae from the SDSS-II Supernova Survey
- Constraints on dark energy with the LOSS SN Ia sample
- A generalized equation of state for dark energy
- Dynamics of cosmological scalar fields
- Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds
- Scaling solutions and weak gravity in dark energy with energy and momentum couplings
- Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
- Reconstructing the dark energy potential
- Cosmological dynamics of scalar fields with kinetic corrections: Beyond the exponential potential
- A Comparative Study of Dark Energy Constraints from Current Observational Data
- Probing the time dependence of dark energy
- Phase-space analysis of a class of k-essence cosmology
- Dynamical stability of K-essence field interacting non-minimally with a perfect fluid
- Distance Measurements from Supernovae and Dark Energy Constraints
- General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter
- Anisotropic k-essence cosmologies
- Kinetically coupled dark energy
- Dynamical Systems Analysis of K-essence Model
- Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
- Implications of JLA data for essence model of dark energy with given equation of state