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Relativistic Smoothed Particle Hydrodynamics. C.E. Aguiar, T. Kodama U.F. Rio de Janeiro T. Osada,Y. Hama U. São Paulo. Outline Relativistic hydrodynamics Relativistic SPH Entropy-based SPH Shocks and artificial viscosity. Relativistic Hydrodynamics. Energy-momentum conservation.
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Relativistic Smoothed Particle Hydrodynamics C.E. Aguiar, T. Kodama U.F. Rio de Janeiro T. Osada,Y. Hama U. São Paulo • Outline • Relativistic hydrodynamics • Relativistic SPH • Entropy-based SPH • Shocks and artificial viscosity
Relativistic Hydrodynamics Energy-momentum conservation Baryon-number conservation
Baryon number conservation: comoving derivative:
enthalpy per baryon: Energy-momentum conservation:
Momentum equation: Energy equation:
Entropy conservation: s = entropy density (rest frame)
SPH • Developed to study gas dynamics in astrophysical systems. • Lagrangian method. • No grids. • Arbitrary geometries. • Equally applicable in 1, 2 and 3 space • dimensions. - L.Lucy, Astron.J. 82, 1013 (1977) - R.Gingold, J.Monaghan, MNRAS 181, 378 (1977) Reviews: - J. Monaghan, Annu. Rev. Astron. Astrophys. 30, 543 (1992) - L. Hernquist, N. Katz, Ap. J. Suppl. 70, 419 (1989)
Smoothing h x 0 Error:
Particles "Monte-Carlo" sampling nb = baryon number of ''particle'' b
Different ways of writing SP estimates (we omit the SP subscript from now on):
Derivatives No need for finite differences and grids: D D i+1 i-1 i
Momentum equation Energy equation
? Particle Velocity equation for g:
Pion Gas Rarefaction Wave
Pion Gas Landau Solution
numerical calculation shock wave x Shock Waves
Pion Gas Shock Wave
Second Law of Thermodynamics: Thermodynamically normal matter: Thermodynamically anomalous matter:
Pion Gas Shock Wave
Pion Gas Rankine - Hugoniot:
QGP + Pions Rarefaction Shock
QGP + Pions Rarefaction Shock
QGP + Pions Rarefaction Shock