Observational Constraints on Interacting Dark Matter Model Without Dark Energy
arXiv:1011.4848 · doi:10.1051/0004-6361/201016204
Abstract
The interacting dark matter (IDM) scenario allows for the acceleration of the Universe without Dark Energy. We constrain the IDM model by using the newly revised observational data including data and Union2 SNe Ia via the Markov chain Monte Carlo method. When mimicking the CDM model, we obtain a more stringent upper limit to the effective annihilation term at , and a tighter lower limit to the relevant mass of Dark Matter particles at . When mimicking the CDM model, we find that the effective equation of state of IDM is consistent with the concordance CDM model and appears to be most consistent with the effective phantom model with a constant EoS for which .
5 pages, 6 figures, 3 tables. (Astronomy & Astrophysics in press)
References in corpus (29)
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- Dark torsion as the cosmic speed-up
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- Cosmological Evolution of a Quintom Model of Dark Energy
- The Hubble Diagram to Redshift >6 from 69 Gamma-Ray Bursts
- Observational constraints on theory
- A Cosmology-Independent Calibration of Gamma-Ray Burst Luminosity Relations and the Hubble Diagram
- Constraints on Dark Matter annihilations from reionization and heating of the intergalactic gas
- Power of Observational Hubble Parameter Data: a Figure of Merit Exploration
- Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
- Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant
- Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
- Reconstruction of Deceleration Parameters from Recent Cosmic Observations
- The Weak Energy Condition and the Expansion History of the Universe
- The expansion field: The value of H_0
- Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy
- Constraints on the generalized Chaplygin gas model including gamma-ray bursts via a Markov Chain Monte Carlo approach
- Cosmological constraints combining H(z), CMB shift and SNIa observational data
- The LambdaCDM model on the lead -- a Bayesian cosmological models comparison
- Natural Phantom Dark Energy, Wiggling Hubble Parameter and Direct Data
- Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
- Exploring the Latest Union2 SNIa Dataset by Using Model-Independent Parametrization Methods
- Cosmology-Independent Distance Moduli of 42 Gamma-Ray Bursts between Redshift of 1.44 and 6.60
- Constraints on the DGP Universe Using Observational Hubble parameter
- Cosmology from Planck
- Testing the Consistence of Gamma Ray Burst Data-set and Supernovae Union2
Cited by in corpus (22)
- Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
- The Gravitational-Wave Physics II: Progress
- Observational constraints on Hubble constant and deceleration parameter in power-law cosmology
- Testing the dark energy with gravitational lensing statistics
- Testing the phenomenological interacting dark energy with observational data
- New observational constraints on cosmology from radio quasars
- Hubble parameter data constraints on dark energy
- Direct measurement of the distribution of dark matter with strongly lensed gravitational waves
- Measuring the viscosity of dark matter with strongly lensed gravitational waves
- Quintessential power-law cosmology: dark energy equation of state
- Testing the interaction model with cosmological data and gamma-ray bursts
- Interacting agegraphic dark energy model in tachyon cosmology coupled to matter
- Smooth deformations and cosmic statefinders
- Entropy of Higher Dimensional Charged Gauss-Bonnet Black hole in de Sitter Space
- Implications on the cosmic coincidence by a dynamical extrinsic curvature
- Revisiting Friedmann-like cosmology with torsion: newest constraints from high-redshift observations
- Statistical analysis with cosmic-expansion-rate measurements and two-point diagnostics
- Universe acceleration and fine structure constant variation in BSBM theory
- Fab-Four cosmography to tackle the Hubble tension
- Testing the coincidence problem with strong gravitational lens, Type Ia supernovae and Hubble parameter observational data
- Constraints on scalar-tensor theories from observations
- Thermodynamics and holography of tachyon cosmology