The abacus cosmological N-body code
ABSTRACT We present abacus, a fast and accurate cosmological N-body code based on a new method for calculating the gravitational potential from a static multipole mesh. The method analytically separates the near- and far-field forces, reducing the former to direct 1/r2 summation and the latter to a...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2021-11, Vol.508 (1), p.575-596 |
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creator | Garrison, Lehman H Eisenstein, Daniel J Ferrer, Douglas Maksimova, Nina A Pinto, Philip A |
description | ABSTRACT
We present abacus, a fast and accurate cosmological N-body code based on a new method for calculating the gravitational potential from a static multipole mesh. The method analytically separates the near- and far-field forces, reducing the former to direct 1/r2 summation and the latter to a discrete convolution over multipoles. The method achieves 70 million particle updates per second per node of the Summit supercomputer, while maintaining a median fractional force error of 10−5. We express the simulation time-step as an event-driven ‘pipeline’, incorporating asynchronous events such as completion of co-processor work, input/output, and network communication. abacus has been used to produce the largest suite of N-body simulations to date, the abacussummit suite of 60 trillion particles, incorporating on-the-fly halo finding. abacus enables the production of mock catalogues of the volume and resolution required by the coming generation of cosmological surveys. |
doi_str_mv | 10.1093/mnras/stab2482 |
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We present abacus, a fast and accurate cosmological N-body code based on a new method for calculating the gravitational potential from a static multipole mesh. The method analytically separates the near- and far-field forces, reducing the former to direct 1/r2 summation and the latter to a discrete convolution over multipoles. The method achieves 70 million particle updates per second per node of the Summit supercomputer, while maintaining a median fractional force error of 10−5. We express the simulation time-step as an event-driven ‘pipeline’, incorporating asynchronous events such as completion of co-processor work, input/output, and network communication. abacus has been used to produce the largest suite of N-body simulations to date, the abacussummit suite of 60 trillion particles, incorporating on-the-fly halo finding. abacus enables the production of mock catalogues of the volume and resolution required by the coming generation of cosmological surveys.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/stab2482</identifier><language>eng</language><publisher>United States: Oxford University Press</publisher><subject>ASTRONOMY AND ASTROPHYSICS ; cosmology ; methods: numerical ; theory</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2021-11, Vol.508 (1), p.575-596</ispartof><rights>2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society 2021</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c366t-ca97cdb0029a7d94fd9c27e6d48f63266fb6c3634725f6c65acf1a962cb30ce13</citedby><cites>FETCH-LOGICAL-c366t-ca97cdb0029a7d94fd9c27e6d48f63266fb6c3634725f6c65acf1a962cb30ce13</cites><orcidid>0000-0002-9853-5673 ; 0000000298535673</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,1604,27924,27925</link.rule.ids><linktorsrc>$$Uhttps://dx.doi.org/10.1093/mnras/stab2482$$EView_record_in_Oxford_University_Press$$FView_record_in_$$GOxford_University_Press</linktorsrc><backlink>$$Uhttps://www.osti.gov/servlets/purl/1979511$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Garrison, Lehman H</creatorcontrib><creatorcontrib>Eisenstein, Daniel J</creatorcontrib><creatorcontrib>Ferrer, Douglas</creatorcontrib><creatorcontrib>Maksimova, Nina A</creatorcontrib><creatorcontrib>Pinto, Philip A</creatorcontrib><creatorcontrib>UT-Battelle LLC/ORNL, Oak Ridge, TN (United States)</creatorcontrib><creatorcontrib>Flatiron Institute, New York, NY (United States)</creatorcontrib><creatorcontrib>Harvard Univ., Cambridge, MA (United States)</creatorcontrib><title>The abacus cosmological N-body code</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT
We present abacus, a fast and accurate cosmological N-body code based on a new method for calculating the gravitational potential from a static multipole mesh. The method analytically separates the near- and far-field forces, reducing the former to direct 1/r2 summation and the latter to a discrete convolution over multipoles. The method achieves 70 million particle updates per second per node of the Summit supercomputer, while maintaining a median fractional force error of 10−5. We express the simulation time-step as an event-driven ‘pipeline’, incorporating asynchronous events such as completion of co-processor work, input/output, and network communication. abacus has been used to produce the largest suite of N-body simulations to date, the abacussummit suite of 60 trillion particles, incorporating on-the-fly halo finding. abacus enables the production of mock catalogues of the volume and resolution required by the coming generation of cosmological surveys.</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>cosmology</subject><subject>methods: numerical</subject><subject>theory</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNqFkDtPwzAUhS0EEqGwMkcwMbj1I7mOR1TxkipYymzZNzYNSuIqTof-e1JaZqYjXX33HOkj5JazOWdaLrp-sGmRRutEUYkzknEJJRUa4JxkjMmSVorzS3KV0jdjrJACMnK_3vjcOou7lGNMXWzjV4O2zd-pi_V-utX-mlwE2yZ_c8oZ-Xx-Wi9f6erj5W35uKIoAUaKViusHWNCW1XrItQahfJQF1WAaQyCg4mUhRJlAITSYuBWg0AnGXouZ-Tu2BvT2JiEzehxg7HvPY6Ga6VLfoDmRwiHmNLgg9kOTWeHveHMHDyYXw_mz8P08HBq3W3_Y38Any9ftQ</recordid><startdate>20211101</startdate><enddate>20211101</enddate><creator>Garrison, Lehman H</creator><creator>Eisenstein, Daniel J</creator><creator>Ferrer, Douglas</creator><creator>Maksimova, Nina A</creator><creator>Pinto, Philip A</creator><general>Oxford University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OIOZB</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-9853-5673</orcidid><orcidid>https://orcid.org/0000000298535673</orcidid></search><sort><creationdate>20211101</creationdate><title>The abacus cosmological N-body code</title><author>Garrison, Lehman H ; Eisenstein, Daniel J ; Ferrer, Douglas ; Maksimova, Nina A ; Pinto, Philip A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c366t-ca97cdb0029a7d94fd9c27e6d48f63266fb6c3634725f6c65acf1a962cb30ce13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>cosmology</topic><topic>methods: numerical</topic><topic>theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Garrison, Lehman H</creatorcontrib><creatorcontrib>Eisenstein, Daniel J</creatorcontrib><creatorcontrib>Ferrer, Douglas</creatorcontrib><creatorcontrib>Maksimova, Nina A</creatorcontrib><creatorcontrib>Pinto, Philip A</creatorcontrib><creatorcontrib>UT-Battelle LLC/ORNL, Oak Ridge, TN (United States)</creatorcontrib><creatorcontrib>Flatiron Institute, New York, NY (United States)</creatorcontrib><creatorcontrib>Harvard Univ., Cambridge, MA (United States)</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Garrison, Lehman H</au><au>Eisenstein, Daniel J</au><au>Ferrer, Douglas</au><au>Maksimova, Nina A</au><au>Pinto, Philip A</au><aucorp>UT-Battelle LLC/ORNL, Oak Ridge, TN (United States)</aucorp><aucorp>Flatiron Institute, New York, NY (United States)</aucorp><aucorp>Harvard Univ., Cambridge, MA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The abacus cosmological N-body code</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2021-11-01</date><risdate>2021</risdate><volume>508</volume><issue>1</issue><spage>575</spage><epage>596</epage><pages>575-596</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>ABSTRACT
We present abacus, a fast and accurate cosmological N-body code based on a new method for calculating the gravitational potential from a static multipole mesh. The method analytically separates the near- and far-field forces, reducing the former to direct 1/r2 summation and the latter to a discrete convolution over multipoles. The method achieves 70 million particle updates per second per node of the Summit supercomputer, while maintaining a median fractional force error of 10−5. We express the simulation time-step as an event-driven ‘pipeline’, incorporating asynchronous events such as completion of co-processor work, input/output, and network communication. abacus has been used to produce the largest suite of N-body simulations to date, the abacussummit suite of 60 trillion particles, incorporating on-the-fly halo finding. abacus enables the production of mock catalogues of the volume and resolution required by the coming generation of cosmological surveys.</abstract><cop>United States</cop><pub>Oxford University Press</pub><doi>10.1093/mnras/stab2482</doi><tpages>22</tpages><orcidid>https://orcid.org/0000-0002-9853-5673</orcidid><orcidid>https://orcid.org/0000000298535673</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | ASTRONOMY AND ASTROPHYSICS cosmology methods: numerical theory |
title | The abacus cosmological N-body code |
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