The two volumes of Gravitational Waves provide a comprehensive and detailed account of the physics of gravitational waves. Volume 2 discusses what can be learned from gravitational waves in astrophysics and in cosmology, by systematizing a large body of theoretical developments that have taken place over the last decades.
The two volumes of Gravitational Waves provide a comprehensive and detailed account of the physics of gravitational waves. Volume 2 discusses what can be learned from gravitational waves in astrophysics and in cosmology, by systematizing a large body of theoretical developments that have taken place over the last decades.
Michele Maggiore is Professor of Physics at the Department of Theoretical Physics, University of Geneva, Switzerland. He served as President of the Physics Section at the University of Geneva until 2017.
Inhaltsangabe
III: Astrophysical Sources of GWs 10: Stellar collapse 11: Neutron stars 12: Black-hole perturbation theory 13: Properties of dynamical space-times 14: GWs from coalescing compact binaries. Theory IV: Cosmology and Gravitational Waves 17: Basics of FRW cosmology 18: Helicity decomposition of the metric perturbations 19: Evolution of cosmological perturbations 20: The imprint of GWs on the CMB 21: Inflation and primordial perturbations 22: Stochastic backgrounds of cosmological origin 23: Stochastic backgrounds and pulsar timing arrays
III: Astrophysical Sources of GWs 10: Stellar collapse 11: Neutron stars 12: Black-hole perturbation theory 13: Properties of dynamical space-times 14: GWs from coalescing compact binaries. Theory IV: Cosmology and Gravitational Waves 17: Basics of FRW cosmology 18: Helicity decomposition of the metric perturbations 19: Evolution of cosmological perturbations 20: The imprint of GWs on the CMB 21: Inflation and primordial perturbations 22: Stochastic backgrounds of cosmological origin 23: Stochastic backgrounds and pulsar timing arrays
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