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dc.contributor.authorSanghai, VAAen_US
dc.contributor.authorClifton, Ten_US
dc.date.accessioned2018-02-15T15:17:43Z
dc.date.available2016-04-07en_US
dc.date.issued2016-04-07en_US
dc.date.submitted2018-02-02T16:39:22.920Z
dc.identifier.issn2470-0010en_US
dc.identifier.otherARTN 089903en_US
dc.identifier.otherARTN 089903en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/32423
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.93.089903
dc.titlePost-Newtonian cosmological modelling (vol 91, 103532, 2015)en_US
dc.typeArticle
dc.rights.holder© 2016 American Physical Society
dc.identifier.doi10.1103/PhysRevD.93.089903en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000373584100009&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue8en_US
pubs.notesNo embargoen_US
pubs.publication-statusPublisheden_US
pubs.volume93en_US


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