<div dir="ltr"><div><div><div><div><br clear="all"></div>Hello,<br></div>1) I just tried to run some of my "old" parameter files using the new ET release and I got some strange results. The parameter files which work completely fine for previous releases do not work anymore in a sense that for example for the binary neutron star simulations starting from LORENE initial data hamiltonian constraint blows up and central density become nan shortly after the beginning. Thus, I have a question are there any essential changes I need to incorporate in my par files due to the new release or the old par files should in principle work and give same results as before?<br>
<br></div>2) I'm trying to use ML_CCZ4 for the spacetime evolution and I found the example par file for BBH evolution in McLachlan/par/CCZ4/bbh_ccz4.par which does not work. I figured that this file was for the old implementation of the ccz4 inside ML_BSSN thorn and if I replace ML_BSSN with ML_CCZ4 and comment some of the parameters it works. However, I was wondering if you could provide a working example of such a file with ML_CCZ4? <br>
<br></div>Thank you. <br><div><div><div><div>-- <br><div dir="ltr"><div>Petr Tsatsin</div><div>Graduate Student - Department of Physics</div><div>Charles E. Schmidt College of Science</div><div>Florida Atlantic University</div>
<div>(561)-297-3386</div><div>cell: 1-561-299-8048</div><div><a href="mailto:ptsatin@fau.edu" target="_blank">ptsatin@fau.edu</a>, <a href="mailto:ptsatsin@gmail.com" target="_blank">ptsatsin@gmail.com</a></div><div></div>
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