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Thermodynamics of relativistic fluids P. Ván Department of Theoretical Physics Research Institute of Particle Thermodynamics of relativistic fluids P. Ván Department of Theoretical Physics Research Institute of Particle and Nuclear Physics, Budapest, Hungary – Introduction Internal energy: –Thermodynamics and stability – Non-relativistic fluids – Stability paradox of dissipative relativistic fluids – About the temperature of moving bodies – Conclusions common work with T. S. Bíró and E. Molnár

Introduction – role of the Second Law: Non-equilibrium thermodynamics: basic variables evolution equations (basic Introduction – role of the Second Law: Non-equilibrium thermodynamics: basic variables evolution equations (basic balances) Second Law Stability of homogeneous equilibrium Entropy ~ Lyapunov function Homogeneous systems (equilibrium thermodynamics): dynamic reinterpretation – ordinary differential equations clear, mathematically strict - Finite time thermodynamics …. - Matolcsi T. : Ordinary thermodynamics (Academic Publishers, 2005)

Continuum systems partial differential equations – Lyapunov theorem is more technical Linear stability (of Continuum systems partial differential equations – Lyapunov theorem is more technical Linear stability (of homogeneous equilibrium) Example: non-relativistic fluid mechanics local equilibrium, Fourier-Navier-Stokes n vi e qi Pij pi Thermodynamics p particle number density relative (3 -)velocity internal energy density internal energy (heat) flux pressure momentum density

Fourier-Navier-Stokes linear constitutive relations, <> is symmetric, traceless part Equilibrium: Linearization, …, Routh-Hurwitz criteria: Fourier-Navier-Stokes linear constitutive relations, <> is symmetric, traceless part Equilibrium: Linearization, …, Routh-Hurwitz criteria: Thermodynamic stability (concave entropy) Hydrodynamic stability

Dissipative relativistic fluids Nonrelativistic Relativistic Local equilibrium (1 st order) Fourier+Navier-Stokes Eckart (1940) Beyond Dissipative relativistic fluids Nonrelativistic Relativistic Local equilibrium (1 st order) Fourier+Navier-Stokes Eckart (1940) Beyond local equilibrium (2 nd order) Cattaneo-Vernotte, gen. Navier-Stokes Israel-Stewart (1969 -72), Müller-Ruggieri, Öttinger, Carter, etc. Eckart: Israel-Stewart:

Special relativistic fluids (Eckart): energy-momentum density particle density vector General representations by local rest Special relativistic fluids (Eckart): energy-momentum density particle density vector General representations by local rest frame quantities. Eckart term

Stability of homogeneous equilibrium Eckart theory: instable – due to heat conduction water Israel-Stewart Stability of homogeneous equilibrium Eckart theory: instable – due to heat conduction water Israel-Stewart theory: stability is conditional: complicated conditions relaxation to the first order theory? (Geroch 1995, Lindblom 1995)

Second Law as a constrained inequality (Liu procedure): 1) 2) Ván: under publication in Second Law as a constrained inequality (Liu procedure): 1) 2) Ván: under publication in JMMS, (ar. Xiv: 07121437)

Modified relativistic irreversible thermodynamics: Internal energy: Eckart term Modified relativistic irreversible thermodynamics: Internal energy: Eckart term

Dissipative hydrodynamics < > symmetric traceless spacelike part Þ linear stability of homogeneous equilibrium Dissipative hydrodynamics < > symmetric traceless spacelike part Þ linear stability of homogeneous equilibrium CONDITION: thermodynamic stablity

Thermodynamics: Temperatures and other intensives are doubled: Different roles: Equations of state: Constitutive functions: Thermodynamics: Temperatures and other intensives are doubled: Different roles: Equations of state: Constitutive functions: Θ, M T, μ

About the temperature of moving bodies: moving body CRETE inertial observer About the temperature of moving bodies: moving body CRETE inertial observer

About the temperature of moving bodies: Body v K 0 K translational work Einstein-Planck: About the temperature of moving bodies: Body v K 0 K translational work Einstein-Planck: entropy is invariant, energy is vector

Body v K 0 K Ott - hydro: entropy is vector, energy-presssure are from Body v K 0 K Ott - hydro: entropy is vector, energy-presssure are from a tensor Our:

Summary – energy ≠ internal energy → generic stability without extra conditions - relativistic Summary – energy ≠ internal energy → generic stability without extra conditions - relativistic thermodynamics: there is no local equilibrium - different temperatures in Fourier-law (equilibration) and in state functions out of local equilibrium. - causality /Ván and Bíró, EPJ, (2007), 155, p 201 -212, (ar. Xiv: 0704. 2039 v 2)/ - hyperbolic(-like) extensions, solutions /Bíró, Molnár and Ván: under publication in PRC, (ar. Xiv: 0805. 1061)/

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