1 / 37

Relativistic Smoothed Particle Hydrodynamics

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.

zclayton
Download Presentation

Relativistic Smoothed Particle Hydrodynamics

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. 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

  2. Relativistic Hydrodynamics Energy-momentum conservation Baryon-number conservation

  3. Baryon number conservation: comoving derivative:

  4. enthalpy per baryon: Energy-momentum conservation:

  5. Momentum equation: Energy equation:

  6. Entropy conservation: s = entropy density (rest frame)

  7. Lagrangian Equations

  8. 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)

  9. Smoothing h x 0 Error:

  10. Particles "Monte-Carlo" sampling nb = baryon number of ''particle'' b

  11. Different ways of writing SP estimates (we omit the SP subscript from now on):

  12. Derivatives No need for finite differences and grids: D D i+1 i-1 i

  13. More than one way of calculating derivatives:

  14. Moving the Particles

  15. Momentum equation Energy equation

  16. Energy and Momentum

  17. Entropy equation

  18. ? Particle Velocity equation for g:

  19. RSPH Equations

  20. Baryon-Free Matter

  21. Lagrangian equations:

  22. Entropy-based RSPH

  23. Ultrarelativistic Pion Gas

  24. Pion Gas Rarefaction Wave

  25. Pion Gas Landau Solution

  26. numerical calculation shock wave x Shock Waves

  27. Pion Gas Shock Wave

  28. Artificial Viscosity

  29. Second Law of Thermodynamics: Thermodynamically normal matter: Thermodynamically anomalous matter:

  30. Dissipative RSPH

  31. Pion Gas Shock Wave

  32. Pion Gas Rankine - Hugoniot:

  33. QGP + Pion Gas

  34. QGP + Pions Rarefaction Shock

  35. QGP + Pions Rarefaction Shock

  36. QGP + Pions Rarefaction Shock

More Related