Steady asymptotic equilibria in conformal relativistic fluids

Esteban Calzetta
Phys. Rev. D 105, 036013 – Published 23 February 2022

Abstract

When one considers a shock wave in the frame where the shock is at rest, on either side one has a steady flow which converges to equilibrium away from the shock. However, hydrodynamics is unable to describe this flow if the asymptotic velocity is higher than the characteristic speed of the theory. We obtain an exact solution for the decay rate to equilibrium for a conformal fluid in kinetic theory under the relaxation time approximation, and compare it to two hydrodynamic schemes, one accounting for the second moments of the distribution function and thus equivalent, in the small deviations from equilibrium limit, to an Israel-Stewart framework, and another accounting for both second and third moments. While still having a finite characteristic speed, the second model is a significant improvement on the first.

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  • Received 4 January 2022
  • Accepted 7 February 2022

DOI:https://doi.org/10.1103/PhysRevD.105.036013

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Fluid DynamicsParticles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Esteban Calzetta*

  • Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires and IFIBA, CONICET, Cuidad Universitaria, Buenos Aires 1428, Argentina

  • *calzetta@df.uba.ar

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Vol. 105, Iss. 3 — 1 February 2022

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