PhD Fluid Web Page by Iñaki Olabarrieta

Thesis:

''Relativistic Hydrodynamics and other topics in Numerical Relativity.'' by Ignacio (Iñaki) Olabarrieta (PS, PDF)

Ideal Fluids

Notes:
- 2nd Status Report. (for committee members)
- 1st Status Report. (for committee members)
- Derivation of the EOM in 3+1 .
- Derivation of the EOM in 2+1+1 .

Simulations:
- Gaussian Ring (without gravity)
- Spherical Symmetric Initial Data (without gravity)
  - D , S_rho , S_z , tau , epsilon , v_rho , v_z .
- Shock Tube Test (without gravity)
  - P , rho_o , v_z .
- Kelvin-Helmholtz Instability (without gravity)
  - Slightly relativistic case. (5.3 Mbytes) The movie shows the density rho_o. The speed of the initial wind is 0.01c (moving leftwards).
  - Relativistic case. (1.5 Mbytes) Same as before with a speed 0.5c. The instability is kicks in much sooner. A high resolution (1.4 Mbytes) piece of the same movie. Here it is a longer evolution of the same problem.
- Relativistic Jets (without gravity)
  - D for a jet.
- One dimensional TOV solutions in maximal-isotropic coordinates.
  - P , 2M/r , v .
Ultrarelativistic Fluids
- Check out Project2 and Project 3b for the LAB of the Graduate Summer School on General Relativistic Hydrodynamics.
- 1D Notes.
- 2D Notes.
  - Jet Simulation in cartesian flatspace Energy Density (rho)
- ENO.