CONSTRAINING THE PROPERTIES OF DARK MATTER WITH OBSERVATIONS OF THE COSMIC MICROWAVE BACKGROUND

ABSTRACT We examine how the properties of dark matter, parameterized by an equation-of-state parameter w and two perturbative generalized dark matter (GDM) parameters, c2s (the sound speed) and (the viscosity), are constrained by existing cosmological data, particularly the Planck 2015 data release....

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Bibliographic Details
Published in:The Astrophysical journal 2016-10, Vol.830 (2), p.155
Main Authors: Thomas, Daniel B., Kopp, Michael, Skordis, Constantinos
Format: Article
Language:English
Subjects:
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Big Bang theory
Cold dark matter
Confidence intervals
Constraining
Constraints
cosmic background radiation
Cosmic microwave background
cosmological parameters
COSMOLOGY
cosmology: observations
Dark matter
DENSITY
EQUATIONS OF STATE
INCLUSIONS
NONLUMINOUS MATTER
Parameters
RELICT RADIATION
UNIVERSE
VELOCITY
VISCOSITY
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Summary:ABSTRACT We examine how the properties of dark matter, parameterized by an equation-of-state parameter w and two perturbative generalized dark matter (GDM) parameters, c2s (the sound speed) and (the viscosity), are constrained by existing cosmological data, particularly the Planck 2015 data release. We find that the GDM parameters are consistent with zero, and are strongly constrained, showing no evidence for extending the model of dark matter beyond the cold dark matter (CDM) paradigm. The equation of state of dark matter is constrained to be within at the 99.7% confidence level (CL), which is several times stronger than constraints found previously using WMAP data. The parameters c2s and are constrained to be less than and 6.06 × 10−6 respectively at the 99.7% CL. The inclusion of the GDM parameters does significantly affect the error bars on several ΛCDM parameters, notably the dimensionless dark matter density g and the derived parameters 8 and H0. This can be partially alleviated with the inclusion of data constraining the expansion history of the universe.
ISSN:0004-637X
1538-4357
DOI:10.3847/0004-637X/830/2/155