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Black Holes: physics and astronomy
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Black Holes in classical physics: Given a mass M, how compact (squished) does it have to be?
Schwarzschild Radius Rs = 2GM c2
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General Relativity and Black Holes
General Relativity: a theory of gravity Basic mathematical object: 4 dimensional spacetime
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Basic Ingredients of General Relativity
(A) Objects move between 2 points in spacetime on the shortest path between those points (geodesics) (B) The presence of mass warps or bends spacetime The Einstein Field Equations
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General Relativistic Black Holes
For sufficient concentration of mass in sufficiently small region, there is a rip or hole poked in spacetime Schwarzschild Radius DEMO with analogs
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Question: Do black holes exist in nature?
What would you look for? What kind of observation would reveal a black hole?
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Cygnus X-1: the prototype black hole
Artists’s conception of Cygnus X-1
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Where Cygnus X-1 is located
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An example of a black hole system
Black hole and a red dwarf
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A key to black holes: hot accretion disks
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Present knowledge about black holes
20 confirmed black hole systems Least massive: solar masses Most massive: solar masses Remember all pulsars have 1.4 solar masses
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Black holes on larger scales: the center of the Milky Way
A black hole of 2.5 million solar masses, and more to come
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