Viscosity bound for anisotropic superfluids with dark matter sector

Marek Rogatko and Karol I. Wysokiński
Phys. Rev. D 96, 026015 – Published 17 July 2017

Abstract

The shear viscosity to the entropy density ratio η/s of the anisotropic superfluid has been calculated by means of the gauge/gravity duality in the presence of the dark matter sector. The dark matter has been described by the Yang-Mills field analogous to the one describing the visible matter sector, and it is assumed to interact with the visible field with coupling constant α. Close to the superfluid transition temperature (Tc), the analytical solution has been given up to the leading order in a symmetry breaking parameter and the ratio of the gravitational constant and Yang-Mils coupling. The tensor element of ratio η/s remains unaffected by the dark matter for the viscosity tensor in the plane perpendicular to the symmetry breaking direction (here, yz). The temperature dependence and the linear correction in (1α) in the plane containing this direction (here, xy) was also revealed. The correction linearly vanishes for temperature tending to the critical one TTc.

  • Received 9 May 2017

DOI:https://doi.org/10.1103/PhysRevD.96.026015

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Marek Rogatko*

  • Institute of Physics, Maria Curie-Sklodowska University, 20-031 Lublin, Polish square Marii Curie-Sklodowskiej 1, Poland

Karol I. Wysokiński

  • Institute of Physics, Maria Curie-Sklodowska University, 20-031 Lublin, Polish square Marii Curie-Sklodowskiej 1, Poland

  • *marek.rogatko@poczta.umcs.lublin.pl, rogat@kft.umcs.lublin.pl
  • karol.wysokinski@umcs.pl

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Issue

Vol. 96, Iss. 2 — 15 July 2017

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