Relativistic dissipative hydrodynamics with spontaneous symmetry breaking

Abstract

In this paper we consider dissipative hydrodynamic equations for systems with continuous broken symmetries. We first present the case of superfluidity, in which the symmetry U(1) is broken and then generalize to the chiral symmetry $SU(2{)}_L\times SU(2{)}_R$. The corresponding new transport coefficients are introduced.

5 pages, RevTeX Minor changes, version accepted for publication

References in corpus (2)

• Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions
• Hydrodynamics of relativisic systems with broken continuous symmetries

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