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dc.contributor.authorEnqvist, Ken_US
dc.contributor.authorMulryne, DJen_US
dc.contributor.authorNurmi, Sen_US
dc.date.accessioned2016-01-04T15:29:09Z
dc.date.issued2015-05en_US
dc.identifier.issn1475-7516en_US
dc.identifier.otherARTN 010en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/10171
dc.description18 pages, 5 figures
dc.description.sponsorshipD.J.M. is supported by a Royal Society University Research Fellowship, and was supported by the Science and Technology Facilities Council grant ST/J001546/1 during the majority of this work. He thanks Helsinki for hospitality during the initial stages of this work. SN is supported by the Academy of Finland grant 257532. KE is supported by the Academy of Finland grants 1263714 and 1218322.en_US
dc.language.isoenen_US
dc.relation.ispartofJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICSen_US
dc.subjectinflationen_US
dc.subjectcosmological perturbation theoryen_US
dc.titleResolving primordial physics through correlated signaturesen_US
dc.typeArticle
dc.rights.holder© 2015 IOP Publishing Ltd and Sissa Medialab srl
dc.identifier.doi10.1088/1475-7516/2015/05/010en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000355794800010&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue5en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US


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