LEADER 02260nam0 22004573i 450 001 VAN0212767 005 20230612111007.984 017 70$2N$a9789811080074 100 $a20210916d2018 |0itac50 ba 101 $aeng 102 $aSG 105 $a|||| ||||| 200 1 $aˆThe ‰Vector Mode in the Second-order Cosmological Perturbation Theory$eDoctoral Thesis accepted by the Nagoya University, Nagoya, Japan$fShohei Saga 210 $aSingapore$cSpringer$d2018 215 $axiii, 136 p.$cill.$d24 cm 410 1$1001VAN0104193$12001 $aSpringer theses$erecognizing outstanding Ph.D. research$1210 $aBerlin$cSpringer$d2010- 500 1$3VAN0212768$aˆThe ‰Vector Mode in the Second-order Cosmological Perturbation Theory$91868327 606 $a00A79 (77-XX)$xPhysics [MSC 2020]$3VANC023182$2MF 606 $a85-XX$xAstronomy and Astrophysics [MSC 2020]$3VANC023246$2MF 606 $a85A40$xCosmology [MSC 2020]$3VANC023267$2MF 606 $a83Fxx$xCosmology [MSC 2020]$3VANC023580$2MF 606 $a83Dxx$xRelativistic gravitational theories other than Einstein's, including asymmetric field theories [MSC 2020]$3VANC034075$2MF 610 $a21cm Radiation$9KW:K 610 $aCosmic Microwave Background Fluctuations$9KW:K 610 $aCosmic Microwave Background Lensing$9KW:K 610 $aCosmological Vector Mode$9KW:K 610 $aLarge-scale Structure of the Cosmos$9KW:K 610 $aMagnetogenesis$9KW:K 610 $aPrimordial Magnetic Fields$9KW:K 610 $aWeak lensing$9KW:K 620 $aSG$dSingapore$3VANL000061 700 1$aSaga$bShohei$3VANV182903$0835970 712 $aSpringer $3VANV108073$4650 801 $aIT$bSOL$c20240614$gRICA 856 4 $uhttp://doi.org/10.1007/978-981-10-8007-4$zE-book ? Accesso al full-text attraverso riconoscimento IP di Ateneo, proxy e/o Shibboleth 899 $aBIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$1IT-CE0120$2VAN08 912 $fN 912 $aVAN0212767 950 $aBIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08CONS e-book 3803 $e08eMF3803 20210916 996 $aVector Mode in the Second-order Cosmological Perturbation Theory$91868327 997 $aUNICAMPANIA