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Double power series method for approximating cosmological perturbations

dc.contributor.authorWren, AJen_US
dc.contributor.authorMalik, KAen_US
dc.date.accessioned2017-06-01T09:31:54Z
dc.date.available2017-05-15en_US
dc.date.issued2017-04-28en_US
dc.date.submitted2017-05-24T14:27:38.133Z
dc.identifier.issn2470-0010en_US
dc.identifier.otherARTN 083526
dc.identifier.otherARTN 083526en_US
dc.identifier.otherARTN 083526en_US
dc.identifier.otherARTN 083526en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/23470
dc.description.sponsorshipScience and Technology Facilities Council (STFC) Grant No. ST/J001546/1.en_US
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.95.083526
dc.titleDouble power series method for approximating cosmological perturbationsen_US
dc.typeArticle
dc.rights.holder© 2017 American Physical Society
dc.identifier.doi10.1103/PhysRevD.95.083526en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000400255100006&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue8en_US
pubs.notesNo embargoen_US
pubs.publication-statusPublisheden_US
pubs.volume95en_US


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