Please use this identifier to cite or link to this item: 192.168.6.56/handle/123456789/74347
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dc.contributor.authorSaga, Shohei-
dc.date.accessioned2019-06-26T12:40:50Z-
dc.date.available2019-06-26T12:40:50Z-
dc.date.issued2018-
dc.identifier.isbn978-981-10-8007-4-
dc.identifier.urihttp://10.6.20.12:80/handle/123456789/74347-
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectCosmological perturbation theory · Cosmic microwave background radiation · Non-gaussianityen_US
dc.titleThe Vector Mode in the Second-order Cosmological Perturbation Theoryen_US
dc.typeBooken_US
Appears in Collections:Physics

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