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dc.contributor.authorHuston, Ien_US
dc.contributor.authorMalik, KAen_US
dc.date.accessioned2017-03-03T14:20:42Z
dc.date.issued2009-09en_US
dc.date.submitted2017-01-18T17:12:14.677Z
dc.identifier.issn1475-7516en_US
dc.identifier.other019
dc.identifier.other019
dc.identifier.other019
dc.identifier.other019en_US
dc.identifier.other019en_US
dc.identifier.other019en_US
dc.identifier.other019en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/19649
dc.format.extent? - ?en_US
dc.relation.ispartofJ COSMOL ASTROPART Pen_US
dc.rightsThis is a pre-copyedited, author-produced version of an article accepted for publication in Journal of Cosmology and Astroparticle Physics following peer review. The version of record is available http://iopscience.iop.org/article/10.1088/1475-7516/2009/09/019/meta
dc.subjectinflationen_US
dc.subjectcosmologicalen_US
dc.subjectperturbation theoryen_US
dc.subjectnon-gaussianityen_US
dc.subjectCOSMOLOGICAL PERTURBATIONSen_US
dc.subjectINFLATIONARY UNIVERSEen_US
dc.subjectNON-GAUSSIANITYen_US
dc.subjectFLUCTUATIONSen_US
dc.subjectGENERATIONen_US
dc.subjectEVOLUTIONen_US
dc.subjectDYNAMICSen_US
dc.subjectMODELSen_US
dc.titleNumerical calculation of second order perturbationsen_US
dc.typeArticle
dc.rights.holderhttps://doi.org/10.1088/1475-7516/2009/09/019
dc.identifier.doi10.1088/1475-7516/2009/09/019en_US
pubs.issue9en_US
pubs.notesNot knownen_US


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