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Generating the cosmic microwave background power asymmetry with g(NL)

dc.contributor.authorKenton, Zen_US
dc.contributor.authorMulryne, DJen_US
dc.contributor.authorThomas, Sen_US
dc.date.accessioned2016-06-01T13:58:24Z
dc.date.available2015-06-19en_US
dc.date.issued2015-07-06en_US
dc.identifier.issn2470-0010en_US
dc.identifier.otherARTN 023505en_US
dc.identifier.otherARTN 023505en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/12621
dc.relation.ispartofPHYSICAL REVIEW Den_US
dc.rights“The final publication is available at http://journals.aps.org/prd/abstract/10.1103/PhysRevD.92.023505”
dc.titleGenerating the cosmic microwave background power asymmetry with g(NL)en_US
dc.typeArticle
dc.identifier.doi10.1103/PhysRevD.92.023505en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000357494900004&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue2en_US
pubs.notesNo embargoen_US
pubs.notesversion accepted by PRDen_US
pubs.publication-statusPublisheden_US
pubs.volume92en_US


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