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Separable projection integrals for higher-order correlators of the cosmic microwave sky: Acceleration by factors exceeding 100

dc.creatorBriggs, JP
dc.creatorPennycook, SJ
dc.creatorFergusson, James Robert
dc.creatorJäykkä, J
dc.creatorShellard, Edward Paul
dc.date.accessioned2018-11-24T23:18:32Z
dc.date.available2016-01-28T15:41:36Z
dc.date.available2018-11-24T23:18:32Z
dc.date.issued2016-01-19
dc.identifierhttps://www.repository.cam.ac.uk/handle/1810/253535
dc.identifier.urihttp://repository.aust.edu.ng/xmlui/handle/123456789/3299
dc.description.abstractWe 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.languageen
dc.publisherElsevier
dc.publisherJournal of Computational Physics
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsAttribution 4.0 International
dc.rightsAttribution 4.0 International
dc.rightsAttribution 4.0 International
dc.titleSeparable projection integrals for higher-order correlators of the cosmic microwave sky: Acceleration by factors exceeding 100
dc.typeArticle


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