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Introduction to Relativistic Hydrodynamics

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<strong>Relativistic</strong> viscous hydrodynamics<br />

Basic equations<br />

◮ allow dissipative terms, but no charge in the system<br />

◮ assume entropy current has additional linear dissipative terms (first-order<br />

theory)<br />

S µ = su µ + αV µ<br />

◮ phenomenological definitions resp. so called constitutive equations for the<br />

shear stress tensor π µν and for the bulk pressure Π<br />

π µν <br />

1<br />

<br />

= 2η ∆<br />

2<br />

µ α∆ ν β + ∆µ<br />

β∆ν <br />

α − 1<br />

3 ∆µν <br />

∆αβ ∆ ακ ∂κu β<br />

Π = −ξ∂µu µ<br />

◮ transport coefficients: η shear viscosity, ξ bulk viscosity, ...<br />

◮ characterize deviation from thermal equilibrium<br />

November 22nd, 2012 | TUD - IKP | D. Nowakowski | 17

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