#2119: The binary neutron star gallery example gives different results with the release candiate. ----------------------+----------------------------------------------------- Reporter: diener | Owner: Type: defect | Status: new Priority: blocker | Milestone: ET_2018_02 Component: Other | Version: development version Resolution: | Keywords: ----------------------+-----------------------------------------------------
Comment (by roberto.depetri@…):
Quite likely the new run use the c++ code instead of the fortran one (that was the default at that time) and small difference can be present. A better comparison (for the post-merger phase) should be to consider (also) the module of psi_4 instead of just the real part. In the post merger phase there are more than one modes with diffrent constructive-distructive interference) and a small phase differnce on the two-three excited mode may show up. Running the Gallery example on Marconi.