dc.contributor.author | Goldberg, SR | en_US |
dc.contributor.author | Gallagher, CS | en_US |
dc.contributor.author | Clifton, T | en_US |
dc.date.accessioned | 2017-11-28T14:36:42Z | |
dc.date.available | 2017-10-23 | en_US |
dc.date.issued | 2017-11-10 | en_US |
dc.date.submitted | 2017-11-14T14:01:27.908Z | |
dc.identifier.issn | 2470-0010 | en_US |
dc.identifier.other | ARTN 103508 | en_US |
dc.identifier.other | ARTN 103508 | en_US |
dc.identifier.other | ARTN 103508 | en_US |
dc.identifier.other | ARTN 103508 | en_US |
dc.identifier.uri | http://qmro.qmul.ac.uk/xmlui/handle/123456789/28975 | |
dc.relation.ispartof | PHYSICAL REVIEW D | en_US |
dc.rights | This 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.title | Perturbation theory for cosmologies with nonlinear structure | en_US |
dc.type | Article | |
dc.rights.holder | © 2017 American Physical Society | |
dc.identifier.doi | 10.1103/PhysRevD.96.103508 | en_US |
pubs.author-url | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000414850100002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
pubs.issue | 10 | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 96 | en_US |