02260nam0 22004573i 450 VAN021276720230612111007.984N978981108007420210916d2018 |0itac50 baengSG|||| |||||ˆThe ‰Vector Mode in the Second-order Cosmological Perturbation TheoryDoctoral Thesis accepted by the Nagoya University, Nagoya, JapanShohei SagaSingaporeSpringer2018xiii, 136 p.ill.24 cm001VAN01041932001 Springer thesesrecognizing outstanding Ph.D. research210 BerlinSpringer2010-VAN0212768ˆThe ‰Vector Mode in the Second-order Cosmological Perturbation Theory186832700A79 (77-XX)Physics [MSC 2020]VANC023182MF85-XXAstronomy and Astrophysics [MSC 2020]VANC023246MF85A40Cosmology [MSC 2020]VANC023267MF83FxxCosmology [MSC 2020]VANC023580MF83DxxRelativistic gravitational theories other than Einstein's, including asymmetric field theories [MSC 2020]VANC034075MF21cm RadiationKW:KCosmic Microwave Background FluctuationsKW:KCosmic Microwave Background LensingKW:KCosmological Vector ModeKW:KLarge-scale Structure of the CosmosKW:KMagnetogenesisKW:KPrimordial Magnetic FieldsKW:KWeak lensingKW:KSGSingaporeVANL000061SagaShoheiVANV182903835970Springer <editore>VANV108073650ITSOL20240614RICAhttp://doi.org/10.1007/978-981-10-8007-4E-book – Accesso al full-text attraverso riconoscimento IP di Ateneo, proxy e/o ShibbolethBIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICAIT-CE0120VAN08NVAN0212767BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA08CONS e-book 3803 08eMF3803 20210916 Vector Mode in the Second-order Cosmological Perturbation Theory1868327UNICAMPANIA