The aim of this book is to become a major reference text for gravitational-wave physics, covering in detail both the experimental and the theoretical aspects. It is the only existing book on gravitational waves. It brings the reader to the forefront of present-day research, and assumes no previous knowledge of gravitational-wave physics.
The aim of this book is to become a major reference text for gravitational-wave physics, covering in detail both the experimental and the theoretical aspects. It is the only existing book on gravitational waves. It brings the reader to the forefront of present-day research, and assumes no previous knowledge of gravitational-wave physics.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Prof. Michele Maggiore Department of Theoretical Physics, University of Geneva Born in 1963, Michele Maggiore has graduated from University of Pisa in 1986, and has got his PhD from Scuola Normale Superiore in Pisa, in 1989. After postdoctoral positions in Bern and at University of Minnesota he became researcher at INFN in Pisa in 1991. Since 2001 he is Professeur Ordinaire (Professor) at the Dept. of Theoretical Physics, University of Geneva. His research interests cover a broad range of subjects, including quantum field theory, quantum gravity, cosmology, string theory, and the study of gravitational waves of astrophysical or cosmological origin. He is also involved in experimental effors for gravitational wave detection.
Inhaltsangabe
Part I Gravitational-wave theory 1: The geometric approach to GWs 2: The field-theoretical approach to GWs 3: Generation of GWs in linearized theory 4: Applications 5: GW generation by post-Newtonian sources 6: Experimental observation of GW emission in compact binaries Part II Experiments 7: Data analysis techniques 8: Resonant-mass detectors 9: Interferometers
Part I Gravitational-wave theory 1: The geometric approach to GWs 2: The field-theoretical approach to GWs 3: Generation of GWs in linearized theory 4: Applications 5: GW generation by post-Newtonian sources 6: Experimental observation of GW emission in compact binaries Part II Experiments 7: Data analysis techniques 8: Resonant-mass detectors 9: Interferometers
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