Cosmic viscosity as a remedy for tension between PLANCK and LSS data
arXiv:1708.07030 · doi:10.1088/1475-7516/2017/11/005
Abstract
Measurements of from large scale structure observations show a discordance with the extrapolated from Planck CMB parameters using CDM cosmology. Similar discordance is found in the value of and . In this paper, we show that the presence of viscosity in cold dark matter, shear or bulk or combination of both, can remove the above mentioned conflicts simultaneously. This indicates that the data from Planck CMB observation and different LSS observations prefer small but non-zero amount of viscosity in cold dark matter fluid.
16 pages, 13 figs, matches accepted version in JCAP
References in corpus (10)
- The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview
- Indications of a late-time interaction in the dark sector
- Viscous Cosmology for Early- and Late-Time Universe
- Tension between the power spectrum of density perturbations measured on large and small scales
- Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation
- Residual Non-Abelian Dark Matter and Dark Radiation
- A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
- Hidden Charged Dark Matter and Chiral Dark Radiation
- Structure formation in a CDM universe
- Baryon Acoustic Oscillations
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- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Cosmological discordances II: Hubble constant, Planck and large-scale-structure data sets
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- Accelerated and decelerated expansion in a causal dissipative cosmology
- Growth of matter perturbations in the extended viscous dark energy models
- Microphysical manifestations of viscosity and consequences for anisotropies in the very early universe
- Can the Hubble tension be resolved by bulk viscosity?
- A new Parametrization for Bulk Viscosity Cosmology as Extension of the CDM Model
- Linearized propagation equations for metric fluctuations in a general (non-vacuum) background geometry
- Study of a viscous WDM model: Near equilibrium condition, entropy production, and cosmological constraints
- Global 21-cm brightness temperature in viscous dark energy models
- Dark Matter Cosmology with Varying Viscosity: a Possible Resolution to the Tension
- Viscous attenuation of gravitational waves propagating through an inhomogeneous background
- Gravitational Wave luminosity distance in viscous cosmological models
- Exploring thermodynamics inconsistencies in unimodular gravity: a comparative study of two energy diffusion functions
- Scalar field unification of interacting viscous dark fluid from a geometrical scalar-tensor theory of gravity
- Ricci cosmology in light of astronomical data
- Singularities and Soft-Big Bang in a viscous CDM model