The Vector Mode in the Second-order Cosmological Perturbation Theory - Couverture souple

Saga, Shohei

9789811356902: The Vector Mode in the Second-order Cosmological Perturbation Theory

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ISBN 10 : 9811356904 ISBN 13 : 9789811356902

Editeur : Springer, 2019

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� propos de l'auteur

Dr. Shohei Saga is a JSPS research Fellow at Yukawa Institute for Theoretical Physics, Kyoto University. His work mainly involves observational cosmology. He received his Bachelor of Science from Nagoya University in 2012, and his Master and Doctor of Science from the Department of Physics, Nagoya University in 2014 and 2017, respectively. In March 2014, he was awarded the 2013 Dean Prize by the Department of Physics, Nagoya University.

Les informations fournies dans la section � A propos du livre � peuvent faire r�f�rence � une autre �dition de ce titre.

�diteur: Springer
Date d'�dition: 2019
Langue: anglais
ISBN 10: 9811356904
ISBN 13: 9789811356902
Reliure: Broch�
Nombre de pages: 152
Coordonn�es du fabricant: Springer Nature Customer Service Center GmbH
ProductSafety@springernature.com

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Saga:The Vector Mode in the Second-orde (eng)

Saga, Shohei

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The Vector Mode in the Second-order Cosmological Perturbation Theory (Springer Theses)

Saga, Shohei

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The Vector Mode in the Second-order Cosmological Perturbation Theory

Shohei Saga

Edit� par Springer Nature Singapore Jan 2019, 2019

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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This thesis sheds valuable new light on the second-order cosmological perturbation theory, extensively discussing it in the context of cosmic microwave background (CMB) fluctuations. It explores the observational consequences of the second-order vector mode, and addresses magnetic field generation and the weak lensing signatures, which are key phenomena of the vector mode. The author demonstrates that the second-order vector mode, which never appears at the linear-order level, naturally arises from the non-linear coupling of the first-order scalar modes. This leads to the remarkable statement that the vector-order mode clearly contributes to the generation of cosmological magnetic fields. Moreover, the weak lensing observations are shown to be accessible to the vector mode. On the basis of ongoing and forthcoming observations, the thesis concludes that the second-order vector mode is detectable. 152 pp. Englisch. N� de r�f. du vendeur 9789811356902

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The Vector Mode in the Second-order Cosmological Perturbation Theory (Springer Theses)

Shohei Saga

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The Vector Mode in the Second-order Cosmological Perturbation Theory

Saga, Shohei

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ISBN 10 : 9811356904 ISBN 13 : 9789811356902

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The Vector Mode in the Second-Order Cosmological Perturbation Theory

Shohei Saga

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ISBN 10 : 9811356904 ISBN 13 : 9789811356902

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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Nominated as an outstanding PhD thesis by the Nagoya University, Japan Skillfully describes the development of the complete formalism for the second-order cosmological perturbation theory, involving vector and tensor modesProposes a scenario . N� de r�f. du vendeur 266455177

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The Vector Mode in the Second-order Cosmological Perturbation Theory

Shohei Saga

Edit� par Springer, 2019

ISBN 10 : 9811356904 ISBN 13 : 9789811356902

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Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - This thesis sheds valuable new light on the second-order cosmological perturbation theory, extensively discussing it in the context of cosmic microwave background (CMB) fluctuations. It explores the observational consequences of the second-order vector mode, and addresses magnetic field generation and the weak lensing signatures, which are key phenomena of the vector mode. The author demonstrates that the second-order vector mode, which never appears at the linear-order level, naturally arises from the non-linear coupling of the first-order scalar modes. This leads to the remarkable statement that the vector-order mode clearly contributes to the generation of cosmological magnetic fields. Moreover, the weak lensing observations are shown to be accessible to the vector mode. On the basis of ongoing and forthcoming observations, the thesis concludes that the second-order vector mode is detectable. N� de r�f. du vendeur 9789811356902

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