Gravitational waves and cosmology /:
Gespeichert in:
Weitere Verfasser: | , , |
---|---|
Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Amsterdam :
IOS Press,
2020.
|
Schriftenreihe: | Proceedings of the International School of Physics "Enrico Fermi" ;
Course 200 |
Schlagworte: | |
Online-Zugang: | Volltext |
Beschreibung: | 1 online resource : illustrations, charts |
Bibliographie: | Includes bibliographical references. |
ISBN: | 9781643680958 1643680951 |
Internformat
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490 | 1 | |a Proceedings of the International School of Physics "Enrico Fermi" ; |v Course 200 | |
504 | |a Includes bibliographical references. | ||
505 | 0 | |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 | |
505 | 8 | |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 | |
505 | 8 | |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 | |
505 | 8 | |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 | |
505 | 8 | |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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adam_text | |
any_adam_object | |
author2 | Coccia, E. (Eugenio) Silk, Joseph, 1942- Vittorio, N. |
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contents | 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 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 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 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 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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discipline | Physik |
format | Electronic eBook |
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id | ZDB-4-EBA-on1197842068 |
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indexdate | 2024-11-27T13:30:04Z |
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isbn | 9781643680958 1643680951 |
language | English |
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series2 | Proceedings of the International School of Physics "Enrico Fermi" ; |
spelling | Gravitational waves and cosmology / edited by E. Coccia, J. Silk and N. Vittorio, directors of the course. Amsterdam : IOS Press, 2020. 1 online resource : illustrations, charts text txt rdacontent computer c rdamedia online resource cr rdacarrier Proceedings of the International School of Physics "Enrico Fermi" ; Course 200 Includes bibliographical references. 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 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 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 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 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 Gravitational waves. http://id.loc.gov/authorities/subjects/sh85056562 Cosmology. http://id.loc.gov/authorities/subjects/sh85033169 Ondes gravitationnelles. Cosmologie. cosmology. aat Cosmology fast Gravitational waves fast Electronic book. Coccia, E. (Eugenio) https://id.oclc.org/worldcat/entity/E39PBJfcHgx44YCb9mWv3rYByd http://id.loc.gov/authorities/names/n96000161 Silk, Joseph, 1942- https://id.oclc.org/worldcat/entity/E39PBJvhpkv93WqK8XWgGx6Yfq http://id.loc.gov/authorities/names/n79090652 Vittorio, N. http://id.loc.gov/authorities/names/n90648470 has work: Gravitational waves and cosmology (Text) https://id.oclc.org/worldcat/entity/E39PCFBXdRRtMkBpWrkfcTyyBP https://id.oclc.org/worldcat/ontology/hasWork International School of Physics "Enrico Fermi." Proceedings of the International School of Physics "Enrico Fermi" ; course 200. http://id.loc.gov/authorities/names/n42019799 FWS01 ZDB-4-EBA FWS_PDA_EBA https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=2632788 Volltext |
spellingShingle | Gravitational waves and cosmology / 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 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 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 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 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 Gravitational waves. http://id.loc.gov/authorities/subjects/sh85056562 Cosmology. http://id.loc.gov/authorities/subjects/sh85033169 Ondes gravitationnelles. Cosmologie. cosmology. aat Cosmology fast Gravitational waves fast |
subject_GND | http://id.loc.gov/authorities/subjects/sh85056562 http://id.loc.gov/authorities/subjects/sh85033169 |
title | Gravitational waves and cosmology / |
title_auth | Gravitational waves and cosmology / |
title_exact_search | Gravitational waves and cosmology / |
title_full | Gravitational waves and cosmology / edited by E. Coccia, J. Silk and N. Vittorio, directors of the course. |
title_fullStr | Gravitational waves and cosmology / edited by E. Coccia, J. Silk and N. Vittorio, directors of the course. |
title_full_unstemmed | Gravitational waves and cosmology / edited by E. Coccia, J. Silk and N. Vittorio, directors of the course. |
title_short | Gravitational waves and cosmology / |
title_sort | gravitational waves and cosmology |
topic | Gravitational waves. http://id.loc.gov/authorities/subjects/sh85056562 Cosmology. http://id.loc.gov/authorities/subjects/sh85033169 Ondes gravitationnelles. Cosmologie. cosmology. aat Cosmology fast Gravitational waves fast |
topic_facet | Gravitational waves. Cosmology. Ondes gravitationnelles. Cosmologie. cosmology. Cosmology Gravitational waves Electronic book. |
url | https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=2632788 |
work_keys_str_mv | AT cocciae gravitationalwavesandcosmology AT silkjoseph gravitationalwavesandcosmology AT vittorion gravitationalwavesandcosmology |