Particle Physics and Cosmology: The Interface

G. Smadja

ISBN 10: 1402031599 / ISBN 13: 9781402031595

Editore: Springer Netherlands, Springer Netherlands Mär 2005, 2005

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This item is printed on demand - Print on Demand Titel. Neuware -This Carg` ese school of Particle physics is meant to bridge the narr- ing gap between astrophysical observations and particle physics. The lectures supply the students with a theoretical background which covers severalaspectsofthecosmologicalscenario: matter-antimatterasym- try, the nature of dark matter, the acceleration of the expansion and the cosmological constant and the geometry of the universe as well as m- ernviewsonparticlephysicsincludingsupersymmetry, extradimensions scenarii and neutrino oscillations. ix Preface TheinvestigationofnuclearabundancesbyAlpher,Bethe,andGamow (1948) was the rst intrusion of subatomic physics into cosmology. In contrast with their assumption, most nuclear species are now known to be produced in stars, but their bold step led to predictions which have largely been proven to be right: -a crude estimate of the densities during primordial nucleosynthesis -the presence of a residual 3K radiation today. the issues they addressed are still relevant. The origin of matter is not fully understood,and the CMB has grown into a powerful tool to inv- tigate the early eras of the universe. The progress of cosmological observations has now led to a ¿standard¿ slow-roll in ation model, which accounts quantitatively for many - served features of the universe. As the lectures will show, it still leaves large unchartered areas, and the underlying particle physics aspects are yettobeelucidated.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 532 pp. Englisch.

Codice articolo 9781402031595

Dati bibliografici

• Titolo: Particle Physics and Cosmology: The Interface
• Editore: Springer Netherlands, Springer Netherlands Mär 2005
• Data di pubblicazione: 2005
• Lingua: Inglese
• ISBN 10: 1402031599
• ISBN 13: 9781402031595
• Rilegatura: Taschenbuch
• Condizione: Neu
• Dimensioni: 235 L x 155 A x 29 P (millimetri) 235 millimetri di larghezza per 155 millimetri di altezza per 29 millimetri di profondità
• Peso: 797 grammi

Descrizione articolo

Riassunto

This Carg` ese school of Particle physics is meant to bridge the narr- ing gap between astrophysical observations and particle physics. The lectures supply the students with a theoretical background which covers severalaspectsofthecosmologicalscenario: matter-antimatterasym- try, the nature of dark matter, the acceleration of the expansion and the cosmological constant and the geometry of the universe as well as m- ernviewsonparticlephysicsincludingsupersymmetry, extradimensions scenarii and neutrino oscillations. ix Preface TheinvestigationofnuclearabundancesbyAlpher,Bethe,andGamow (1948) was the ?rst intrusion of subatomic physics into cosmology. In contrast with their assumption, most nuclear species are now known to be produced in stars, but their bold step led to predictions which have largely been proven to be right: -a crude estimate of the densities during primordial nucleosynthesis -the presence of a residual 3K radiation today. the issues they addressed are still relevant. The origin of matter is not fully understood,and the CMB has grown into a powerful tool to inv- tigate the early eras of the universe. The progress of cosmological observations has now led to a standard slow-roll in?ation model, which accounts quantitatively for many - served features of the universe. As the lectures will show, it still leaves large unchartered areas, and the underlying particle physics aspects are yettobeelucidated.

Contenuti

Contributing Authors. Foreword. Preface. Acknowledgments. ElectroWeak Symmetry Breaking as of 2003; R. Barbieri. Current Status of the CKM Matrix and the CP Violation; A. Stocchi. Neutrino Masses; S. Pokorski. Neutrinos; J. Bouchez. Baryo- and Leptogenesis (outline); W. Buchmueller. Scalar fields in particle physics in cosmology; P. Binetruy. Inflation, Quantum Fluctuations and Cosmological Perturbations; D. Langlois. Cosmic Microwave Background Cosmology; G.F. Smoot. Cosmology with Supernovae la; G. Smadja. Dark Matter and Galaxy Formation; J. Silk. Supersymmetric Extension of the Standard Model; D. Kazakov. Gaugino Condensation and SUSY Breakdown; H.P. Nilles. Is Dark Matter Supersymmetric?; W. de Boer. Cargese Lectures on Extra Dimensions; R. Rattazzi