[Users] McLachlan crash
Vassilios Mewes
vassilios.mewes at uv.es
Wed Feb 27 07:53:51 CST 2013
Hello all,
still no success with the full evolution of BH+torus...
i have attached the par file i have been using lately, in which i added two
more levels of mesh refinement, as Roland suggested, increased the
Dissipation order to 5th and removed the parameter
ML_BSSN::dt_lapse_shift_method = "noLapseShiftAdvection"..
this has improved things a bit, but the L_inf norm of the hamiltonian
constraint still starts growing at around t=200 (after having decreased and
then having been rather constant up to that point) and then the simulation
will crash later (either due to the shift being nan at the puncture or by
detecting nans)
in the meantime, i have evolved a single puncture, the bondi accretion onto
a puncture and an "inverse cowling" (setting up the spacetime and hydro
variables of the BH+torus system but only evolving the spacetime), all
using the same parameters, and all of those work...its only the full system
of BH+torus when i run into problems...this is using the ET 2012.11.
release..
do you have any ideas what might go wrong with the spacetime evolution when
evolving the full system?
best wishes,
Vassili
On Tue, Feb 12, 2013 at 2:07 AM, Roland Haas <roland.haas at physics.gatech.edu
> wrote:
> Hello Vassilios,
>
> > as mentioned earlier in the ET phone call, i have attached the par file
> > used in the run...
> >
> > i tried checking for the nans in the output, but the last hdf5 output was
> > too many iterations earlier and they aren't visible in 1D ascii output
> > either
> >
> > as said, the puncture tracker actually aborted the run, not the nan
> > checker...
> Thank you for the parameter file. As a unsubstantiated guess, I would
> try what happens if you move the outer boundary further out. Right now
> it sits at 50M which I would find uncomfortably close if there is any
> say "junk" radiation (eg from setting up a BH with spin in flat
> background) present. I'd move it to at least 200M (ie two more levels of
> mesh refinement). Not sure how likely this explanation is since your
> NaNs appear after many (9) light crossing times.
>
> Yours,
> Roland
>
> --
> My email is as private as my paper mail. I therefore support encrypting
> and signing email messages. Get my PGP key from http://keys.gnupg.net.
>
>
> _______________________________________________
> Users mailing list
> Users at einsteintoolkit.org
> http://lists.einsteintoolkit.org/mailman/listinfo/users
>
>
-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists.einsteintoolkit.org/pipermail/users/attachments/20130227/bbda6ec7/attachment.html
-------------- next part --------------
A non-text attachment was scrubbed...
Name: tori_AN1_cc.par
Type: application/octet-stream
Size: 15700 bytes
Desc: not available
Url : http://lists.einsteintoolkit.org/pipermail/users/attachments/20130227/bbda6ec7/attachment.obj
More information about the Users
mailing list