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Re: [charm] AMR performance, for cosmology


Chronological Thread 
  • From: "Casey W. Stark" <caseywstark AT gmail.com>
  • To: Akhil langer <akhilanger AT gmail.com>
  • Cc: charm AT cs.uiuc.edu
  • Subject: Re: [charm] AMR performance, for cosmology
  • Date: Sun, 25 Sep 2011 19:32:28 -0700
  • List-archive: <http://lists.cs.uiuc.edu/pipermail/charm>
  • List-id: CHARM parallel programming system <charm.cs.uiuc.edu>

Hi Akhil.

I'm still in the early stages of learning charm, but where should I look in the git repo to start contributing to the AMR work? I'm very much interested in the solvers and such.

Best,
Casey


On Wed, Sep 21, 2011 at 2:03 PM, Akhil langer <akhilanger AT gmail.com> wrote:
Hi Casey,

We have an AMR implementation on Charm. Right now it is just restricted to Advection simulations but we are working on it to make it a generic framework. Right now I do not have performance numbers for AMR. However, ChaNGa group can share performance numbers for the N-body simulations.

Regards,
Akhil

On Wed, Sep 21, 2011 at 3:12 PM, Casey W. Stark <caseywstark AT gmail.com> wrote:
I am interested in tinkering with the charm++ particles and AMR frameworks (or just charm) for cosmological simulations. I realize there is changa, and I'm sure I could leverage some of the N-body work, but I am interested in Eularian hydro. I don't know if enzo developers (http://code.google.com/p/enzo/) have contacted the list before, but I'm sure some of them are interested as well.

Is anyone familiar with the performance of the particles/AMR frameworks well above 1,000 cores? I'm sure this depends a lot on the implementation and details of the solver used, but I figured someone might have tried this before.

Best,
Casey W. Stark
Astrophysics PhD student, UC Berkeley

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