| dc.contributor.author | Sanghai, VAA | en_US |
| dc.contributor.author | Clifton, T | en_US |
| dc.date.accessioned | 2018-02-15T15:17:43Z | |
| dc.date.available | 2016-04-07 | en_US |
| dc.date.issued | 2016-04-07 | en_US |
| dc.date.submitted | 2018-02-02T16:39:22.920Z | |
| dc.identifier.issn | 2470-0010 | en_US |
| dc.identifier.other | ARTN 089903 | en_US |
| dc.identifier.other | ARTN 089903 | en_US |
| dc.identifier.other | ARTN 089903 | en_US |
| dc.identifier.uri | http://qmro.qmul.ac.uk/xmlui/handle/123456789/32423 | |
| 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.93.089903 | |
| dc.title | Post-Newtonian cosmological modelling (vol 91, 103532, 2015) | en_US |
| dc.type | Article | |
| dc.rights.holder | © 2016 American Physical Society | |
| dc.identifier.doi | 10.1103/PhysRevD.93.089903 | en_US |
| pubs.author-url | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000373584100009&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
| pubs.issue | 8 | en_US |
| pubs.notes | No embargo | en_US |
| pubs.publication-status | Published | en_US |
| pubs.volume | 93 | en_US |
