Cosmic Degeneracy with Dark Energy Equation of State
arXiv:astro-ph/0305495 · doi:10.1016/S0927-6505(03)00182-8
Abstract
We discuss a degeneracy between the geometry of the universe and the dark energy equation of state which exists in the power spectrum of the cosmic microwave background. In particular, for the case with , this degeneracy has interesting implications to a lower bound on from observations. It is also discussed how this degeneracy can be removed using current observations of type Ia supernovae.
13 pages LaTeX with five [one new] eps figures
References in corpus (27)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- An alternative to quintessence
- Exploring the Expansion History of the Universe
- A Line of Sight Approach to Cosmic Microwave Background Anisotropies
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- Essentials of k-essence
- Kinetically Driven Quintessence
- Small Scale Cosmological Perturbations: An Analytic Approach
- Cardassian Expansion: a Model in which the Universe is Flat, Matter Dominated, and Accelerating
- Anisotropies in the Cosmic Microwave Background: An Analytic Approach
- Structure Formation with Generalized Dark Matter
- Microwave Background Constraints on Cosmological Parameters
- Probing the dark side: Constraints on the dark energy equation of state from CMB, large scale structure and Type Ia supernovae
- Early-universe constraints on a Primordial Scaling Field
- Is cosmology consistent?
- Resolving the Cosmological Missing Energy Problem
- Flux-averaging Analysis of Type Ia Supernova Data
- How to Test Stringy Dark Energy?
- The Fate of Dark Energy
- Modified Dispersion Relations from Closed Strings in Toroidal Cosmology
- The magnification of SN 1997ff, the farthest known Supernova
- Discriminating between models for the dark energy
- Cosmic Background Radiation Temperature Anisotropy: Position of First Doppler Peak
Cited by in corpus (19)
- The phantom menaced: constraints on low-energy effective ghosts
- Interacting holographic dark energy
- Nonflat time-variable dark energy cosmology
- Dark Energy Evolution and the Curvature of the Universe from Recent Observations
- Planck 2015 constraints on the non-flat XCDM inflation model
- Inflation in a closed universe
- Implication of Dark Energy Parametrizations on the Determination of the Curvature of the Universe
- Observational constraints on non-flat dynamical dark energy cosmological models
- Dark Energy Parametrizations and the Curvature of the Universe
- Observational constraints on Horava-Lifshitz cosmology
- Horava-Lifshitz cosmology with generalized Chaplygin gas
- Overall observational constraints on the running parameter λof Horava-Lifshitz gravity
- Bigger Rip with No Dark Energy
- Constraints from growth-rate data on some coupled dark energy models mimicking a expansion
- The Hubble constant and dark energy from cosmological distance measures
- Late-time acceleration driven by shift-symmetric Galileon in the presence of Torsion
- Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
- On the Determination of Neutrino Masses and Dark Energy Evolution from the Cross Correlation of CMB and LSS
- Tilted non-spatially-flat inflation