[ET Trac] #2599: nsnstohmns cannot be reproduced using LORENE2

Ken Hui trac-noreply at einsteintoolkit.org
Fri Mar 11 01:03:42 CST 2022


#2599: nsnstohmns cannot be reproduced using LORENE2

 Reporter: Ken Hui
   Status: open
Milestone: ET_2021_05
  Version: ET_2021_05
     Type: bug
 Priority: minor
Component: Cactus

Comment (by Ken Hui):

The definition of those 3 physical constants do not match between LORENE1 and LORENE2. The initial data of the gallery simulation nsnstohmns is \(I supposed\) taken from [https://lorene.obspm.fr/data/binNS.html](https://lorene.obspm.fr/data/binNS.html), which should have been generated with an older LORENE version. That’s why I tried to change the physical constants in LORENE2, to recover their old values. 

```
--- lorene1_unites.h.ori	2022-03-11 13:14:02.810753230 +0800
+++ lorene2_unites.h.ori	2022-03-11 02:08:27.660497092 +0800
@@ -26,8 +26,20 @@
 
 
 /*
- * $Id: unites.h,v 1.4 2004/12/01 12:28:32 p_grandclement Exp $
+ * $Id: unites.h,v 1.8 2015/03/17 14:20:00 j_novak Exp $
  * $Log: unites.h,v $
+ * Revision 1.8  2015/03/17 14:20:00  j_novak
+ * New class Hot_eos to deal with temperature-dependent EOSs.
+ *
+ * Revision 1.7  2014/10/13 08:52:37  j_novak
+ * Lorene classes and functions now belong to the namespace Lorene.
+ *
+ * Revision 1.6  2014/06/30 14:34:57  j_novak
+ * Update of the values of some constants (G, M_sol and MeV).
+ *
+ * Revision 1.5  2014/05/13 10:06:12  j_novak
+ * Change of magnetic units, to make the Lorene unit system coherent. Magnetic field is now expressed in Lorene units. Improvement on the comments on units.
+ *
  * Revision 1.4  2004/12/01 12:28:32  p_grandclement
  * Include math.h in unite.h
  *
@@ -47,50 +59,55 @@
  * Initial revision
  *
  *
- * $Header: /cvsroot/Lorene/C++/Include/unites.h,v 1.4 2004/12/01 12:28:32 p_grandclement Exp $
+ * $Header: /cvsroot/Lorene/C++/Include/unites.h,v 1.8 2015/03/17 14:20:00 j_novak Exp $
```

Indeed I have tried to update the values of G, M\_sol and MeV in LORENE1 according to the 2014 revision, recompile ET and run the nsnstohmns simulations. The Carpet errors came up again at the exact same time step.

For the plot of the grids, I am having problem visualising it in gnuplot. Allow me to attach the raw output here for the moment, I will also try to see if I can plot them using other methods later.  
[https://drive.google.com/drive/folders/1iutL\_5avKqVTQxDCvqb8dIY5QwB6A\_PN?usp=sharing](https://drive.google.com/drive/folders/1iutL_5avKqVTQxDCvqb8dIY5QwB6A_PN?usp=sharing)

‌

--
Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2599/nsnstohmns-cannot-be-reproduced-using
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