Schwarzschild Solution space-time geometry point mass
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BHs: evidence for stellar mass black holes lognM Black Hole Mass Distribution
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BH: evidence for supermassive black holes log nM Black Hole Mass Distribution
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BH: primordial black holes: not yet ruled out log nM Black Hole Mass Distribution
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Primordial BHs
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What are primordial BHs?
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Why do we care about PBH
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Astrophysical constraints:
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Masses in the Stellar Graveyard
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Observational Evidence for Stellar Mass Black Holes
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Evidence For Elusive Imbhs From An Observed Tidal Disruption Events TDEs
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This is the most efficient known way of using mass to get energy:
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accretion on to a black hole must power the most luminous phenomena in the universe
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Eddington implies limit on growth rate of mass: since
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Emitted spectrum of an accrediting object
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b Gravitational energy of each accreted electron-proton pair turned directly into heat at shock temperature
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For supermassive black holes we have
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Modelling accreting sources
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examine both problems in the following
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Accreting Black Holes in a Nearby Galaxy M1011
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Bondi-Hoyle Lyttleton Accretion
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Accretion disc formation
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Thus in general matter orbits accretor. What happens?
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accretion disc structure see APIA Ch 5
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disc formation is unavoidable
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Accretion discs are universal:
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accretion disc structure
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Q&A
Description:
Delve into the fascinating world of supermassive black holes in this comprehensive graduate-level lecture. Explore current theories on the formation of seed black holes, accretion processes driving their growth, and the impact on their surrounding environment. Learn about key concepts including the Schwarzschild solution, mass distributions of different black hole types, and the physics of accretion discs. Examine observational evidence for stellar mass black holes, intermediate-mass black holes, and the potential existence of primordial black holes. Gain insights into modeling techniques for accreting sources, including Bondi-Hoyle Lyttleton accretion and disc formation. Understand the Eddington limit, emitted spectra of accreting objects, and the universal nature of accretion discs across various cosmic scales.
Formation, Fueling, and Feedback from Supermassive Black Holes - Lecture 1