Supermassive black holes:
This is a coherent and accessible account of the concepts that are vital for understanding supermassive black holes. The treatment is largely analytic and gives in-depth discussions of the underlying physics. It will be useful for advanced courses in astrophysics, and as a handbook for active resear...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Cambridge
Cambridge University Press
2023
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| Schlagworte: | |
| Online-Zugang: | Inhaltsverzeichnis |
| Zusammenfassung: | This is a coherent and accessible account of the concepts that are vital for understanding supermassive black holes. The treatment is largely analytic and gives in-depth discussions of the underlying physics. It will be useful for advanced courses in astrophysics, and as a handbook for active researchers |
| Beschreibung: | xvii, 308 Seiten Illustrationen, Diagramme |
| ISBN: | 9781108488051 |
Internformat
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Datensatz im Suchindex
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| adam_text | Contents Preface Acknowledgements page xi xvi 1 Black Holes and Galaxies 1.1 Basic Properties 1.2 The Eddington Limit 1.3 SMBH Accretion 1.4 SMBH Locations 1.5 The SMBH Environment 1.6 Supermassive Black Holes and Galaxies 1 1 3 6 7 11 17 2 Black Holes and General Relativity 2.1 Introduction 2.2 Event Horizons and Causal structure 2.3 Black Hole Spacetimes 2.4 Extracting Black Hole Spin Energy 2.5 Limitations of Quasi-Newtonian Treatments 19 19 22 26 30 33 3 Astrophysical Gases 3.1 Introduction 3.2 Gas Dynamics 3.3 Shocks 3.4 Plasmas 3.5 Magnetohydrodynamics 3.6 Non-ideal MHD 3.7 Force-Free Electrodynamics 40 40 41 45 51 53 64 65 4 Disc Accretion on to Black Holes 4.1 Orbits around Black Holes 66 66 vii
Contents viii 4.2 4.3 4.4 4.5 4.6 4.7 4.8 4.9 4.10 4.11 4.12 4.13 5 Thin Accretion Discs Steady Thin Discs Disc Spectra and Emission Lines Non-thermal Emission When Is a Disc Thin? Disc Stability The Local Structure of Thin Discs Disc Self-Gravity Discs with Super-Eddington Mass Supply When Is the Steady Disc Assumption Valid? Disc Viscosity Numerical Simulations of AccretionFlows 71 77 81 83 84 86 88 92 94 99 100 107 Supermassive Black Hole Growth 5.1 Introduction 5.2 Feeding the Hole 5.3 Chaotic and Misaligned Accretion 5.4 Chaotic Accretion and SMBH Growth 5.5 Massive Seed Black Holes 5.6 Disc Warping, Breaking, and Tearing 5.7 SMBH Binaries and the Last Parsec Problem 5.8 Tidal Disruption Events 5.9 Quasi-Periodic Eruptions 112 112 114 121 131 136 137 155 173 179 6 The Black Hole Scaling Relations 6.1 Introduction 6.2 Black Hole Winds 6.3 Eddington Winds 6.4 The Wind Shock 6.5 The Af-o Relation 6.6 Clearing Out a Galaxy: The Energy-Driven Phase 6.7 Effects of a Galaxy Disc: Triggered Starbursts 6.8 The Three M-а Relations 6.9 The Black Hole-Bulge Mass Relation 6.10 The Assembly Picture of the Scaling Relations 6.11 Momentum or Energy? 6.12 Feedback from Hyper-Eddington Mass Supply 6.13 Cosmological Simulations and M-a 6.14 Small versus Large-Scale Feedback 187 187 189 192 198 209 212 225 229 231 233 239 244 245 245
Contents 7 SMBH Feedback in General 7.1 Introduction 7.2 Radiation Driving 7.3 Jets 7.4 Can Jets Precess? 7.5 Do Jets Move? 8 Black Hole Demographics 8.1 Introduction 8.2 Chaotic Accretion and theLocal AGN Luminosity Function 8.3 How Big Can a Black Hole Grow? 8.4 Evading M-o Problems References Index ix 248 248 248 254 266 271 273 273 274 277 282 289 299 306
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| adam_txt |
Contents Preface Acknowledgements page xi xvi 1 Black Holes and Galaxies 1.1 Basic Properties 1.2 The Eddington Limit 1.3 SMBH Accretion 1.4 SMBH Locations 1.5 The SMBH Environment 1.6 Supermassive Black Holes and Galaxies 1 1 3 6 7 11 17 2 Black Holes and General Relativity 2.1 Introduction 2.2 Event Horizons and Causal structure 2.3 Black Hole Spacetimes 2.4 Extracting Black Hole Spin Energy 2.5 Limitations of Quasi-Newtonian Treatments 19 19 22 26 30 33 3 Astrophysical Gases 3.1 Introduction 3.2 Gas Dynamics 3.3 Shocks 3.4 Plasmas 3.5 Magnetohydrodynamics 3.6 Non-ideal MHD 3.7 Force-Free Electrodynamics 40 40 41 45 51 53 64 65 4 Disc Accretion on to Black Holes 4.1 Orbits around Black Holes 66 66 vii
Contents viii 4.2 4.3 4.4 4.5 4.6 4.7 4.8 4.9 4.10 4.11 4.12 4.13 5 Thin Accretion Discs Steady Thin Discs Disc Spectra and Emission Lines Non-thermal Emission When Is a Disc Thin? Disc Stability The Local Structure of Thin Discs Disc Self-Gravity Discs with Super-Eddington Mass Supply When Is the Steady Disc Assumption Valid? Disc Viscosity Numerical Simulations of AccretionFlows 71 77 81 83 84 86 88 92 94 99 100 107 Supermassive Black Hole Growth 5.1 Introduction 5.2 Feeding the Hole 5.3 Chaotic and Misaligned Accretion 5.4 Chaotic Accretion and SMBH Growth 5.5 Massive Seed Black Holes 5.6 Disc Warping, Breaking, and Tearing 5.7 SMBH Binaries and the Last Parsec Problem 5.8 Tidal Disruption Events 5.9 Quasi-Periodic Eruptions 112 112 114 121 131 136 137 155 173 179 6 The Black Hole Scaling Relations 6.1 Introduction 6.2 Black Hole Winds 6.3 Eddington Winds 6.4 The Wind Shock 6.5 The Af-o Relation 6.6 Clearing Out a Galaxy: The Energy-Driven Phase 6.7 Effects of a Galaxy Disc: Triggered Starbursts 6.8 The Three M-а Relations 6.9 The Black Hole-Bulge Mass Relation 6.10 The Assembly Picture of the Scaling Relations 6.11 Momentum or Energy? 6.12 Feedback from Hyper-Eddington Mass Supply 6.13 Cosmological Simulations and M-a 6.14 Small versus Large-Scale Feedback 187 187 189 192 198 209 212 225 229 231 233 239 244 245 245
Contents 7 SMBH Feedback in General 7.1 Introduction 7.2 Radiation Driving 7.3 Jets 7.4 Can Jets Precess? 7.5 Do Jets Move? 8 Black Hole Demographics 8.1 Introduction 8.2 Chaotic Accretion and theLocal AGN Luminosity Function 8.3 How Big Can a Black Hole Grow? 8.4 Evading M-o Problems References Index ix 248 248 248 254 266 271 273 273 274 277 282 289 299 306 |
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| illustrated | Illustrated |
| index_date | 2024-07-03T22:37:57Z |
| indexdate | 2024-07-10T10:00:47Z |
| institution | BVB |
| isbn | 9781108488051 |
| language | English |
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| physical | xvii, 308 Seiten Illustrationen, Diagramme |
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| spelling | King, Andrew R. 1947- Verfasser (DE-588)1089223692 aut Supermassive black holes Andrew King, University of Leicester Cambridge Cambridge University Press 2023 xvii, 308 Seiten Illustrationen, Diagramme txt rdacontent n rdamedia nc rdacarrier This is a coherent and accessible account of the concepts that are vital for understanding supermassive black holes. The treatment is largely analytic and gives in-depth discussions of the underlying physics. It will be useful for advanced courses in astrophysics, and as a handbook for active researchers Black holes (Astronomy) Schwarzes Loch (DE-588)4053793-6 gnd rswk-swf Schwarzes Loch (DE-588)4053793-6 s DE-604 Erscheint auch als Online-Ausgabe 978-1-108-76884-9 Digitalisierung UB Bayreuth - ADAM Catalogue Enrichment application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=034556541&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
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| title | Supermassive black holes |
| title_auth | Supermassive black holes |
| title_exact_search | Supermassive black holes |
| title_exact_search_txtP | Supermassive black holes |
| title_full | Supermassive black holes Andrew King, University of Leicester |
| title_fullStr | Supermassive black holes Andrew King, University of Leicester |
| title_full_unstemmed | Supermassive black holes Andrew King, University of Leicester |
| title_short | Supermassive black holes |
| title_sort | supermassive black holes |
| topic | Black holes (Astronomy) Schwarzes Loch (DE-588)4053793-6 gnd |
| topic_facet | Black holes (Astronomy) Schwarzes Loch |
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