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dc.contributor.authorNamikawa, T.en
dc.contributor.alternative並河, 俊弥ja
dc.date.accessioned2014-08-21T05:58:25Z-
dc.date.available2014-08-21T05:58:25Z-
dc.date.issued2014-06-05-
dc.identifier.issn2050-3911-
dc.identifier.urihttp://hdl.handle.net/2433/189426-
dc.description.abstractThe weak lensing effect on the cosmic microwave background (CMB) induces distortions in the spatial pattern of CMB anisotropies, and statistical properties of CMB anisotropies become a weakly non-Gaussian field. We first summarize the weak lensing effect on the CMB (CMB lensing) in the presence of scalar, vector, and tensor perturbations. Then we focus on the lensing effect on CMB statistics and methods to estimate deflection angles and their power spectrum. We end by summarizing recent observational progress and future prospects.en
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherOxford University Pressen
dc.rights© The Author(s) 2014. Published by Oxford University Press on behalf of the Physical Society of Japan.en
dc.rightsThis is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/3.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.en
dc.titleCosmology from weak lensing of CMBen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitleProgress of Theoretical and Experimental Physicsen
dc.identifier.volume2014-
dc.identifier.issue6-
dc.relation.doi10.1093/ptep/ptu044-
dc.textversionpublisher-
dc.identifier.artnum06B108-
dcterms.accessRightsopen access-
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