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dc.contributor.authorChristopherson, AJen_US
dc.contributor.authorCarlos Hidalgo, Jen_US
dc.contributor.authorRampf, Cen_US
dc.contributor.authorMalik, KAen_US
dc.date.accessioned2017-03-02T14:22:05Z
dc.date.issued2016-02-25en_US
dc.date.submitted2017-01-18T17:02:26.220Z
dc.identifier.issn2470-0010en_US
dc.identifier.otherARTN 043539
dc.identifier.otherARTN 043539
dc.identifier.otherARTN 043539
dc.identifier.otherARTN 043539en_US
dc.identifier.otherARTN 043539en_US
dc.identifier.otherARTN 043539en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/19612
dc.relation.ispartofPHYSICAL REVIEW Den_US
dc.rightsThis is a pre-copyedited, author-produced version of an article accepted for publication in Physical Review D following peer review. The version of record is available https://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.043539
dc.titleSecond-order cosmological perturbation theory and initial conditions for N-body simulationsen_US
dc.typeArticle
dc.rights.holder© 2016 American Physical Society
dc.identifier.doi10.1103/PhysRevD.93.043539en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000370807300003&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue4en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume93en_US


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