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Perturbation theory for cosmologies with nonlinear structure

dc.contributor.authorGoldberg, SRen_US
dc.contributor.authorGallagher, CSen_US
dc.contributor.authorClifton, Ten_US
dc.date.accessioned2017-11-28T14:36:42Z
dc.date.available2017-10-23en_US
dc.date.issued2017-11-10en_US
dc.date.submitted2017-11-14T14:01:27.908Z
dc.identifier.issn2470-0010en_US
dc.identifier.otherARTN 103508en_US
dc.identifier.otherARTN 103508en_US
dc.identifier.otherARTN 103508en_US
dc.identifier.otherARTN 103508en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/28975
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.96.103508
dc.titlePerturbation theory for cosmologies with nonlinear structureen_US
dc.typeArticle
dc.rights.holder© 2017 American Physical Society
dc.identifier.doi10.1103/PhysRevD.96.103508en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000414850100002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue10en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume96en_US


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