Central value of Ricci scalar for near-critical scalar collapse
- ln R(0,T_0) [ PS | data ]. T_0 is central proper time.
- ln R(0,-tau) [ PS | data ]. tau is ln | T_0 - T_0^star |
Central value of scalar field for near-critical scalar collapse
Note: The above data sets were generated from DIFFERENT critical solutions.
Maintained by choptuik@physics.ubc.ca.
Supported by CIAR,
CFI, NSERC and NSF.