dc.creator | Briggs, JP | |
dc.creator | Pennycook, SJ | |
dc.creator | Fergusson, James Robert | |
dc.creator | Jäykkä, J | |
dc.creator | Shellard, Edward Paul | |
dc.date.accessioned | 2018-11-24T23:18:32Z | |
dc.date.available | 2016-01-28T15:41:36Z | |
dc.date.available | 2018-11-24T23:18:32Z | |
dc.date.issued | 2016-01-19 | |
dc.identifier | https://www.repository.cam.ac.uk/handle/1810/253535 | |
dc.identifier.uri | http://repository.aust.edu.ng/xmlui/handle/123456789/3299 | |
dc.description.abstract | We present a case study describing efforts to optimise and modernise “Modal”, the simulation and analysis pipeline used by the Planck satellite experiment for constraining general non-Gaussian models of the early universe via the bispectrum (or three-point correlator) of the cosmic microwave background radiation. We focus on one particular element of the code: the projection of bispectra from the end of inflation to the spherical shell at decoupling, which defines the CMB we observe today. This code involves a three-dimensional inner product between two functions, one of which requires an integral, on a non-rectangular domain containing a sparse grid. We show that by employing separable methods this calculation can be reduced to a one-dimensional summation plus two integrations, reducing the overall dimensionality from four to three. The introduction of separable functions also solves the issue of the non-rectangular sparse grid. This separable method can become unstable in certain scenarios and so the slower non-separable integral must be calculated instead. We present a discussion of the optimisation of both approaches.
We demonstrate significant speed-ups of ≈100× , arising from a combination of algorithmic improvements and architecture-aware optimisations targeted at improving thread and vectorisation behaviour. The resulting MPI/OpenMP hybrid code is capable of executing on clusters containing processors and/or coprocessors, with strong-scaling efficiency of 98.6% on up to 16 nodes. We find that a single coprocessor outperforms two processor sockets by a factor of 1.3× and that running the same code across a combination of both microarchitectures improves performance-per-node by a factor of 3.38× . By making bispectrum calculations competitive with those for the power spectrum (or two-point correlator) we are now able to consider joint analysis for cosmological science exploitation of new data. | |
dc.language | en | |
dc.publisher | Elsevier | |
dc.publisher | Journal of Computational Physics | |
dc.rights | http://creativecommons.org/licenses/by/4.0/ | |
dc.rights | http://creativecommons.org/licenses/by/4.0/ | |
dc.rights | http://creativecommons.org/licenses/by/4.0/ | |
dc.rights | Attribution 4.0 International | |
dc.rights | Attribution 4.0 International | |
dc.rights | Attribution 4.0 International | |
dc.title | Separable projection integrals for higher-order correlators of the cosmic microwave sky: Acceleration by factors exceeding 100 | |
dc.type | Article | |