Perturbations In Some Dark Energy Models
arXiv:2110.02666
Abstract
Dark energy is the candidate that can produce effective negative pressure and make the galaxies and galaxy clusters move away from each other in an accelerated way. The structures of the Universe have evolved from some initial primordial fluctuations and depend on the background dynamics of different components of the Universe like dark matter, dark energy and others. The motivation of this thesis is to investigate how some of the dark energy models manifest themselves in the formation of the structures in the Universe.
arXiv commentThesis accepted for the award of PhD degree of IISER Kolkata, September 2021
References in corpus (254)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- Efficient Computation of CMB anisotropies in closed FRW models
- f(R) Theories Of Gravity
- Modified Gravity and Cosmology
- The World as a Hologram
- Cosmological Imprint of an Energy Component with General Equation of State
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The Case for a Positive Cosmological Lambda-term
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- Cosmology and the Fate of Dilatation Symmetry
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- The Cosmological Constant
- An alternative to quintessence
- Exploring the Expansion History of the Universe
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- 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
- Dark Energy and the Accelerating Universe
- A Model of Holographic Dark Energy
- The galileon as a local modification of gravity
- Coupled Quintessence
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
- Chameleon Cosmology
- Cosmological Tracking Solutions
- The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Cur vature of the Universe Using Type Ia Supernovae
- f(T) teleparallel gravity and cosmology
- Exponential potentials and cosmological scaling solutions
- Kinetically Driven Quintessence
- Curvature Quintessence
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Disappearing cosmological constant in f(R) gravity
- Dark Energy Constraints from the Cosmic Age and Supernova
- Can the dark energy equation-of-state parameter w be less than -1?
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Rolling Tachyon
- Beyond the Cosmological Standard Model
- Quintessence and the Rest of the World
- Accelerated expansion of the universe driven by tachyonic matter
- Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
- Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
- Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic
- Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
- Cosmology with a Primordial Scaling Field
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Brane-World Gravity
- A Covariant Entropy Conjecture
- Entropy Bounds and Dark Energy
- Cosmic Microwave Background Anisotropies
- Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress tensors
- Conditions for the cosmological viability of f(R) dark energy models
- Cosmological Tests of Modified Gravity
- Holographic dark energy and cosmic coincidence
- CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments
- Cosmological perturbations
- Transition of the dark energy equation of state in an interacting holographic dark energy model
- Scaling solutions in general non-minimal coupling theories
- The Cosmology of Generalized Modified Gravity Models
- Unifying inflation with LambdaCDM epoch in modified f(R) gravity consistent with Solar System tests
- Quintessence arising from exponential potentials
- Efficient sampling of fast and slow cosmological parameters
- Curvature quintessence matched with observational data
- Cosmology with tachyon field as dark energy
- Structure formation with a self-tuning scalar field
- A New Cosmological Model of Quintessence and Dark Matter
- Are f(R) dark energy models cosmologically viable ?
- Do consistent models mimic General Relativity plus ?
- Calibrator Design for the COBE Far Infrared Absolute Spectrophotometer (FIRAS)
- New physics in light of the tension: an alternative view
- Probing the dark energy: methods and strategies
- Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
- A Holographic Dark Energy Model from Ricci Scalar Curvature
- Cosmological scaling solutions of non-minimally coupled scalar fields
- Can the clustered dark matter and the smooth dark energy arise from the same scalar field ?
- Anisotropies in the Cosmic Microwave Background: An Analytic Approach
- Prospects for probing the dark energy via supernova distance measurements
- Supersymmetric World-volume Action for Non-BPS D-branes
- Can interacting dark energy solve the tension?
- Large-scale instability in interacting dark energy and dark matter fluids
- Reconstructing the Cosmic Equation of State from Supernova distances
- Probing the Coupling between Dark Components of the Universe
- 1/R Curvature Corrections as the Source of the Cosmological Acceleration
- CFHTLenS: Combined probe cosmological model comparison using 2D weak gravitational lensing
- Phenomenology of a realistic accelerating universe using only Planck-scale physics
- Probing dark energy perturbations: the dark energy equation of state and speed of sound as measured by WMAP
- Dynamics of dark energy with a coupling to dark matter
- Statefinder diagnostic for holographic dark energy model
- Indications of a late-time interaction in the dark sector
- A Lower Growth Rate from Recent Redshift Space Distortion Measurements than Expected from Planck
- Scalar-Tensor Gravity and Quintessence
- Teleparallel equivalent of Gauss-Bonnet gravity and its modifications
- Testing cosmological structure formation using redshift-space distortions
- A kinematical approach to dark energy studies
- Constraints on the interacting holographic dark energy model
- The shape of the SDSS DR5 galaxy power spectrum
- Dynamics of interacting dark energy
- WMAP and the Generalized Chaplygin Gas
- Proposal for non-BPS D-brane action
- Cosmic flows in the nearby universe from Type Ia Supernovae
- The Robustness of Quintessence
- Generalized Chaplygin gas and CMBR constraints
- A measurement of gravitational lensing of the microwave background using South Pole Telescope data
- What is needed of a tachyon if it is to be the dark energy?
- Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
- Cosmic acceleration without quintessence
- Cosmic Complementarity: H_0 and Omega_m from Combining CMB Experiments and Redshift Surveys
- The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at
- Effects of the interaction between dark energy and dark matter on cosmological parameters
- Le Chatelier-Braun principle in cosmological physics
- Evolution of the tension with the Planck15/CDM determination and implications for modified gravity theories
- Interactions in Scalar Field Cosmology
- Tension and constraints on modified gravity parametrizations of from growth rate and Planck data
- Thawing quintessence with a nearly flat potential
- Reconciling CMB and structure growth measurements with dark energy interactions
- Cosmological dynamics of the tachyon with an inverse power-law potential
- Linear and nonlinear interactions in the dark sector
- Hubble Sinks In The Low-Redshift Swampland
- Reconstruction of the deceleration parameter and the equation of state of dark energy
- A new cosmological tracker solution for Quintessence
- Dark coupling
- Constraining Dark Energy Dynamics in Extended Parameter Space
- Large-scale curvature and entropy perturbations for multiple interacting fluids
- Solving the Coincidence Problem: Tracking Oscillating Energy
- Testing the viability of the interacting holographic dark energy model by using combined observational constraints
- Local Gravity versus Local Velocity: Solutions for and nonlinear bias
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- Interacting Dark Energy -- constraints and degeneracies
- Statefinder Diagnosis for Ricci Dark Energy
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples
- Constraining Interactions in Cosmology's Dark Sector
- New constraints on interacting dark energy from cosmic chronometers
- Testing the Interaction between Dark Energy and Dark Matter with Planck Data
- The growth rate of cosmic structure from peculiar velocities at low and high redshifts
- Tracking solutions in tachyon cosmology
- Challenges for scaling cosmologies
- Quintessence: a mini-review
- Thermodynamical description of the interaction between holographic dark energy and dark matter
- On the stability of Dark Energy with Mass-Varying Neutrinos
- Probing interaction and spatial curvature in the holographic dark energy model
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering
- Holographic dark energy in Brans-Dicke theory
- A Low CMB Quadrupole from Dark Energy Isocurvature Perturbations
- Cosmic Duality in Quintom Universe
- Statefinder diagnosis for the interacting model of holographic dark energy
- Late time acceleration in Brans Dicke Cosmology
- The influence of cosmological transitions on the evolution of density perturbations
- Exhaustive Study of Cosmic Microwave Background Anisotropies in Quintessential Scenarios
- Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
- Brans-Dicke Scalar Field as a Chameleon
- Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation
- Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
- Cosmological window onto the string axiverse and the supersymmetry breaking scale
- Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
- Planck Constraints on Holographic Dark Energy
- Constraints on the interacting vacuum -- geodesic CDM scenario
- A String-Inspired Quintom Model Of Dark Energy
- Adiabatic initial conditions for perturbations in interacting dark energy models
- Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter
- Constraining Inverse Curvature Gravity with Supernovae
- Cosmographic Hubble fits to the supernova data
- Comprehensive cosmographic analysis by Markov Chain Method
- Constraint on Coupled Dark Energy Models from Observations
- Cosmological Constraints from Multiple Probes in the Dark Energy Survey
- Dark Energy Model with Spinor Matter and Its Quintom Scenario
- Scalar-field-dominated cosmology with a transient accelerating phase
- On the large-scale instability in interacting dark energy and dark matter fluids
- Density perturbations for running vacuum: a successful approach to structure formation and to the -tension
- Physical approximations for the nonlinear evolution of perturbations in dark energy scenarios
- Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
- Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
- Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
- Dynamics of Interacting Quintessence Models: Observational Constraints
- High-Redshift Cosmography
- Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
- The First Public Release of South Pole Telescope Data: Maps of a 95-square-degree Field from 2008 Observations
- Acceleration of the universe with a simple trigonometric potential
- Interacting dark matter and modified holographic Ricci dark energy induce a relaxed Chaplygin gas
- Observational constraints on the tilted spatially-flat and the untilted nonflat CDM dynamical dark energy inflation models
- Internal Robustness of Growth Rate data
- Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
- Quintessence Model With Double Exponential Potential
- Thermodynamics second law and crossing(s) in interacting holographic dark energy model
- Slow-Roll Thawing Quintessence
- Searching for dark matter - dark energy interactions: going beyond the conformal case
- Constraints on coupled dark energy using CMB data from WMAP and SPT
- A Comparison of Thawing and Freezing Dark Energy Parametrizations
- Testing coupled dark energy models with their cosmological background evolution
- Direct reconstruction of the quintessence potential
- Phantom Dark Energy Models with a Nearly Flat Potential
- Structure formation in inhomogeneous Early Dark Energy models
- Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
- Tension of the statistic and RSD data with Planck/CDM and implications for weakening gravity
- Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
- Interacting dark matter and modified holographic Ricci dark energy plus a noninteracting cosmic component
- Slowly varying tachyon and tachyon potential
- Quintessence reconstructed: new constraints and tracker viability
- Curvature driven acceleration : a utopia or a reality ?
- Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
- Testing coupled dark energy with next-generation large-scale observations
- Cosmography beyond standard candles and rulers
- In search of the dark matter dark energy interaction: a kinematic approach
- Post- constraints on interacting vacuum energy
- Reconstruction and constraining of the jerk parameter from OHD and SNe Ia observations
- Coupled dark energy with perturbed Hubble expansion rate
- Cosmological perturbations in coherent oscillating scalar field models
- Toward a Possible Solution to the Cosmic Coincidence Problem
- How clustering dark energy affects matter perturbations
- A parametric reconstruction of the cosmological jerk from diverse observational data sets
- Fitting Type Ia supernovae with coupled dark energy
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 LRG sample: structure growth rate measurement from the anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0
- Late universe dynamics with scale-independent linear couplings in the dark sector
- Cosmological Scaling Solutions of Multiple Tachyon Fields with Inverse Square Potentials
- What do we know about cosmography
- CMB constraints on interacting cosmological models
- Scalar Field Dark Energy Perturbations and their Scale Dependence
- An interacting scalar field and the recent cosmic acceleration
- Updated observational constraints on quintessence dark energy models
- Cosmological Perturbations in Models of Coupled Dark Energy
- Growth of matter perturbations in clustered holographic dark energy cosmologies
- Low redshift observational constraints on tachyon models of dark energy
- Interacting dark sector with variable vacuum energy
- Large-scale inhomogeneities may improve the cosmic concordance of supernovae
- Reconstructing the interaction rate in holographic models of dark energy
- Model selection and constraints from Holographic dark energy scenarios
- New tracker models of dark energy
- Reconstruction of interacting dark energy models from parameterizations
- Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
- BAO cosmography
- Clustering dark energy and halo abundances
- Holographic dark energy: constraints on the interaction from diverse observational data sets
- New general parametrization of quintessence fields and its observational constraints
- A comparison of perturbations in fluid and scalar field models of dark energy
- Growth of structure in interacting vacuum cosmologies
- A late time acceleration of the universe with two scalar fields : many possibilities
- Cosmological Perturbation Theory and Structure Formation
- English and Spanish Translation of Zwicky's (1933) The Redshift of Extragalactic Nebulae
- Tachyon Field in Cosmology
- Holographic Dark Energy and Present Cosmic Acceleration
- Growth of perturbations in dark energy parametrization scenarios
- Evolution of perturbations in distinct classes of canonical scalar field models of dark energy
- Cosmological Perturbations in an Inflationary Universe
- Interacting Dark Energy
- Matter Perturbations in Scaling Cosmology
- Reconstruction of cosmological matter perturbations in Modified Gravity
- Scalar field dark energy perturbations and the Integrated Sachs Wolfe effect
- Linear perturbations in a universe with a cosmological constant
- Cosmology and the Origin of the Universe: Historical and Conceptual Perspectives
- On the Reconstruction of Dark Energy Models