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200926s2020 ne ad ob 000 0 eng d |
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|a 9781643680958
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|a 539.754
|2 23
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|a UAMI
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|a Gravitational waves and cosmology /
|c edited by E. Coccia, J. Silk and N. Vittorio, directors of the course.
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|a Amsterdam :
|b IOS Press,
|c 2020.
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|a 1 online resource :
|b illustrations, charts
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|a text
|b txt
|2 rdacontent
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|a computer
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|a online resource
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|a Proceedings of the International School of Physics "Enrico Fermi" ;
|v Course 200
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|a Includes bibliographical references.
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|a Intro -- Title Page -- Contents -- Preface -- Course group shot -- F. Fidecaro -- Principles of gravitational wave detection -- 1. The detection of gravitational waves -- 1.1. Gravitational waves -- 1.2. Effect on a single mass -- 1.3. Effect on a pair of masses -- 1.4. The laboratory frame -- 2. Essential properties -- 2.1. Distance ladder -- 2.2. Expected amplitude -- 2.3. Compact objects -- 2.4. Single compact objects -- 2.5. Supernovae -- 2.6. The indirect evidence for gravitational radiation: PSR 1913+16 -- 3. Signals and noise -- 3.1. Noise power spectrum
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|a 3.2. Power spectra in practice -- 3.3. Power spectrum in digitized signals -- 3.4. Signal and noise -- 3.5. Optimal filtering -- 4. Primary noise sources in gravitational wave interferometers -- 5. Position noise -- 5.1. Seismic noise -- 5.2. Seismic attenuation -- 5.3. The Virgo Superattenuator -- 5.4. Thermal noise -- 5.5. Fluctuation-Dissipation theorem -- 5.6. Thermal noise mitigation -- 5.7. Newtonian noise -- 6. Measurement noise -- 6.1. Michelson-Morley interferometry -- 6.2. Fabry-Perot cavities -- 6.3. Power recycling -- 6.4. Standard quantum limit -- 7. Noise curve -- 8. Ending remarks
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|a Fulvio Ricci -- A primer on a real gravitational wave detector -- 1. Introduction -- 2. The modulation -- 3. The detection of the modulation component -- 4. The readout of the output signal -- 5. The Fabry-Perot cavities as Michelson arms -- 5.1. More about the Fabry-Perot cavities -- 6. How to keep the FP cavities in resonance -- 7. The gravitational wave interferometer -- 8. The interferometer control -- 9. The sensitivity curve -- 10. Thermal noise and cryogenics for future gravitational wave detectors -- 11. Reduction of the readout noise -- 12. Conclusion
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|a Viviana Fafone -- Optical aberrations in gravitational wave detectors and a look at the future -- 1. Introduction -- 2. Optical aberrations and their effects -- 3. Correction of optical aberrations -- 4. Mid and longer term perspective for ground-based detectors -- Michela Mapelli -- Astrophysics of stellar black holes -- 1. Lesson learned from the first direct gravitational wave detections -- 2. The formation of compact remnants from stellar evolution and supernova explosions -- 2.1. Stellar winds and stellar evolution -- 2.2. Supernovae (SNe) -- 2.3. The mass of compact remnants
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|a 3. Binaries of stellar black holes -- 3.1. Mass transfer -- 3.2. Common envelope (CE) -- 3.3. Alternative evolution to CE -- 4. The dynamics of black hole binaries -- 4.1. Dynamically active environments -- 4.2. Three-body encounters -- 4.3. Exchanges -- 4.4. Hardening -- 4.5. Dynamical ejections -- 4.6. Formation of intermediate-mass black holes by runaway collisions -- 4.7. Formation of intermediate-mass black holes by repeated mergers -- 4.8. Kozai-Lidov resonance -- 4.9. Summary of dynamics and open issues -- 5. Black hole binaries in cosmological context -- 5.1. Analytic prescriptions
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590 |
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|a ProQuest Ebook Central
|b Ebook Central Academic Complete
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|a eBooks on EBSCOhost
|b EBSCO eBook Subscription Academic Collection - Worldwide
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|a Gravitational waves.
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650 |
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|a Cosmology.
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|a Ondes gravitationnelles.
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|a Cosmologie.
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|a cosmology.
|2 aat
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|a Cosmology
|2 fast
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|a Gravitational waves
|2 fast
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|a Coccia, E.
|q (Eugenio)
|1 https://id.oclc.org/worldcat/entity/E39PBJfcHgx44YCb9mWv3rYByd
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|a Silk, Joseph,
|d 1942-
|1 https://id.oclc.org/worldcat/entity/E39PBJvhpkv93WqK8XWgGx6Yfq
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|a Vittorio, N.
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758 |
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|i has work:
|a Gravitational waves and cosmology (Text)
|1 https://id.oclc.org/worldcat/entity/E39PCFBXdRRtMkBpWrkfcTyyBP
|4 https://id.oclc.org/worldcat/ontology/hasWork
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|a International School of Physics "Enrico Fermi."
|t Proceedings of the International School of Physics "Enrico Fermi" ;
|v course 200.
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