Imperfect Dark Matter
Abstract
We consider cosmology of the recently introduced mimetic matter with higher derivatives (HD). Without HD this system describes irrotational dust—Dark Matter (DM) as we see it on cosmologically large scales. DM particles correspond to the shiftcharges—Noether charges of the shifts in the field space. Higher derivative corrections usually describe a deviation from the thermodynamical equilibrium in the relativistic hydrodynamics. Thus we show that mimetic matter with HD corresponds to an imperfect DM which: i) renormalises the Newton's constant in the Friedmann equations, ii) has zero pressure when there is no extra matter in the universe, iii) survives the inflationary expansion which puts the system on a dynamical attractor with a vanishing shiftcharge, iv) perfectly tracks any external matter on this attractor, v) can become the main (and possibly the only) source of DM, provided the shiftsymmetry in the HD terms is broken during some small time interval in the radiation domination époque. In the second part of the paper we present a hydrodynamical description of general anisotropic and inhomogeneous configurations of the system. This imperfect mimetic fluid has an energy flow in the field's rest frame. We find that in the Eckart and in the LandauLifshitz frames the mimetic fluidmore »
 Authors:
 Arnold Sommerfeld Center for Theoretical Physics, Ludwig Maximilian University Munich, Theresienstr. 37, Munich, D80333 Germany (Germany)
 Publication Date:
 OSTI Identifier:
 22525769
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2015; Journal Issue: 06; Other Information: Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ANISOTROPY; ATTRACTORS; CORRECTIONS; COSMOLOGY; EQUILIBRIUM; FLUIDS; GRAVITATIONAL COLLAPSE; HYDRODYNAMICS; INFLATIONARY UNIVERSE; NONLUMINOUS MATTER; PARTICLE TRACKS; RELATIVISTIC RANGE; SPACE; UNIVERSE
Citation Formats
Mirzagholi, Leila, and Vikman, Alexander, Email: l.mirzagholi@physik.unimuenchen.de, Email: alexander.vikman@lmu.de. Imperfect Dark Matter. United States: N. p., 2015.
Web. doi:10.1088/14757516/2015/06/028.
Mirzagholi, Leila, & Vikman, Alexander, Email: l.mirzagholi@physik.unimuenchen.de, Email: alexander.vikman@lmu.de. Imperfect Dark Matter. United States. doi:10.1088/14757516/2015/06/028.
Mirzagholi, Leila, and Vikman, Alexander, Email: l.mirzagholi@physik.unimuenchen.de, Email: alexander.vikman@lmu.de. Mon .
"Imperfect Dark Matter". United States.
doi:10.1088/14757516/2015/06/028.
@article{osti_22525769,
title = {Imperfect Dark Matter},
author = {Mirzagholi, Leila and Vikman, Alexander, Email: l.mirzagholi@physik.unimuenchen.de, Email: alexander.vikman@lmu.de},
abstractNote = {We consider cosmology of the recently introduced mimetic matter with higher derivatives (HD). Without HD this system describes irrotational dust—Dark Matter (DM) as we see it on cosmologically large scales. DM particles correspond to the shiftcharges—Noether charges of the shifts in the field space. Higher derivative corrections usually describe a deviation from the thermodynamical equilibrium in the relativistic hydrodynamics. Thus we show that mimetic matter with HD corresponds to an imperfect DM which: i) renormalises the Newton's constant in the Friedmann equations, ii) has zero pressure when there is no extra matter in the universe, iii) survives the inflationary expansion which puts the system on a dynamical attractor with a vanishing shiftcharge, iv) perfectly tracks any external matter on this attractor, v) can become the main (and possibly the only) source of DM, provided the shiftsymmetry in the HD terms is broken during some small time interval in the radiation domination époque. In the second part of the paper we present a hydrodynamical description of general anisotropic and inhomogeneous configurations of the system. This imperfect mimetic fluid has an energy flow in the field's rest frame. We find that in the Eckart and in the LandauLifshitz frames the mimetic fluid possesses nonvanishing vorticity appearing already at the first order in the HD. Thus, the structure formation and gravitational collapse should proceed in a rather different fashion from the simple irrotational DM models.},
doi = {10.1088/14757516/2015/06/028},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 06,
volume = 2015,
place = {United States},
year = {Mon Jun 01 00:00:00 EDT 2015},
month = {Mon Jun 01 00:00:00 EDT 2015}
}

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