This is the first of two papers examining the critical collapse of spherically symmetric perfect fluids with the equation of state P = ( -1) . Here we present the equations of motion and describe a computer code capable of simulating the extremely relativistic flows encountered in critical solutions for 2. The fluid equations are solved using a high-resolution shock-capturing scheme based on a linearized Riemann solver.
No takes yet. Share an insight, caveat, or question.
Neilsen et al. (2000) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: