Present: Frank Loeffler, Roland Haas, Stefan Ruehe, Erik Schnetter, Ian Hinder, Joshua Faber, Matt Kinsey, Yosef Zlochower, James Healy
Stampede slowdown in Noether release: * Ian suggests using mvapich2 rather than intel MPI (already in simfactory/trunk) * Roland suggests disabling LoopControl * Erik suggest looking at Cactus' timer output * Jim will test performance with these options * Jim had tested old version with current setup and got good performance * Jim will open a trac ticket to focus discussion Using SPH (or other particle code with Cactus): * some interest in SPH in Cactus, each participant presented what they had done in the past and what they would like to do, Erik gave a very short description of the SPH method * Erik implemented a unigrid SPH type code in Cactus ** particles are tied to the 3d cells to find neighbours ** uses 1d Cactus arrays for particle storage ** not yet parallelized ** would need to add code to exchange particles as particles move * Josh has a working MPI parallelized SPH code ** uses grid to compute gravity forces ** Newtonian version is available for download ** Josh has fixed background GR version ** each process keeps the full particle position list in memory ** neighbour list however is distributed across processes ** parallelized around particles, no attempt to keep particles local to grid * Matt has code that evolves many geodesics ** own classes to handle and store particles ** keeps particles on process that owns grid under particle, otherwise interpolation is too costly ** currently scales to billions of particles ** uses Boost serialization to move particles after each step ** works with AMR grid * Ian has similar code to evolve geodesics ** wants to evolve geodesics, do raytracing ** have geodesic integrator using MoL and mesh refinement ** tested with relatively small number of geodesics (everything on one process) * Stefan has worked on an fixes spacetime SPH code for his diplom thesis ** would like to couple to a GR code ** to be used for stellar disruption ** more discussion via email ** invited to join the ET phone calls (they are all public) * notice that geodesics and SPH evolution likely have different laod characteristics since geodesics do not require gradients between particles. For geodesics the time consuming factor is sending interpolated data over the network. * suggestion to implement a "particle" datatype in Cactus so that the infrastructure knows about it and can offer specialized functions to handle with them * technical needed code to increase grid array size using intel 14 compiler: * Frank and Roland tried on stampede but failed to compile the full configuration, received segfault * Ian succeeded compiling the bare (or less than) full ET * Erik suggest reducing debug information and/or optimization level Elliptic solver in ET: * currently the only one known to work with mesh refinement is Eloisa Bentivegna's elliptic solver. Currently available on bitbucket https://bitbucket.org/eloisa/cosmology/overview * tested for Cosmology (written for bh lattice), and for binary black holes (not particularly in this case) simfactory 3: * Erik, Ian, Barry working on new simfactory implementation * designing interfaces and methods * should be usable by non-cactus tools, offer direct interface from python, eg "import mdb from simfactory" * currently not yet feature complete * still important architectural decisions to make * Erik will consult with Ian and send out url of repository use simfactory (2) to manage external libraries: * want to have simfactory build external libraries so that they can be used by non-Cactus projects as well * ExternalLibraries revert to CactusExternal scheme * need to handle multiple different configurations build at the same time on the * possible presentation next Monday on current status Misc: * Yosef to open ticket about being unable to checkpoint on stampede Yours, Roland
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