Introduces quantum field theory together with its most important applications to cosmology and astroparticle physics in a coherent framework. Applications such as topological defects, phase transitions, dark matter, external gravitational fields, and black holes help students to bridge the gap between undergraduate courses and research literature.
Introduces quantum field theory together with its most important applications to cosmology and astroparticle physics in a coherent framework. Applications such as topological defects, phase transitions, dark matter, external gravitational fields, and black holes help students to bridge the gap between undergraduate courses and research literature.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Michael Kachelriess is Professor of Physics at the Norwegian University of Science and Technology in Trondheim. After receiving his PhD from Ruhr University at Bochum in 1996, he held fellowships at Gran Sasso National Laboratory, the University of Valencia, the Theory Division of CERN, and the Max Planck Institute for Physics in Munich. His research focuses on theoretical astroparticle physics, and he has published widely in this field.
Inhaltsangabe
1: Classical Mechanics 2: Quantum Mechanics 3: Free Scalar Field 4: Scalar Field with Lambda phi 4 Interaction 5: Global Symmetries and Noether's Theorom 6: Space-time Symmetries 7: Spin-1 and Spin-2 Fields 8: Fermions and the Dirac Equation 9: Scattering Processes 10: Gauge Theories 11: Renormalisation I: Perturbation Theory 12: Renormalisation II: Improving Perturbation Theory 13: Symmetries and Symmetry Breaking 14: GSW Model of Electroweak Interactions 15: Thermal Field Theory 16: Phase Transitions and Topological Defects 17: Anomalies, Instantons and Axions 18: Hadrons, Partons and QCD 19: Gravity as a Gauge Theory 20: Cosmological Models for a Homogeneous, Isotropic Universe 21: Thermal Relics 22: Baryogenesis 23: Quantum Fields in Curved Space-Time 24: Inflation 25: Black Holes 26: Cosmological Constant
1: Classical Mechanics 2: Quantum Mechanics 3: Free Scalar Field 4: Scalar Field with Lambda phi 4 Interaction 5: Global Symmetries and Noether's Theorom 6: Space-time Symmetries 7: Spin-1 and Spin-2 Fields 8: Fermions and the Dirac Equation 9: Scattering Processes 10: Gauge Theories 11: Renormalisation I: Perturbation Theory 12: Renormalisation II: Improving Perturbation Theory 13: Symmetries and Symmetry Breaking 14: GSW Model of Electroweak Interactions 15: Thermal Field Theory 16: Phase Transitions and Topological Defects 17: Anomalies, Instantons and Axions 18: Hadrons, Partons and QCD 19: Gravity as a Gauge Theory 20: Cosmological Models for a Homogeneous, Isotropic Universe 21: Thermal Relics 22: Baryogenesis 23: Quantum Fields in Curved Space-Time 24: Inflation 25: Black Holes 26: Cosmological Constant
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