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Black Holes: physics and astronomy

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Presentation on theme: "Black Holes: physics and astronomy"— Presentation transcript:

1 Black Holes: physics and astronomy

2 Black Holes in classical physics: Given a mass M, how compact (squished) does it have to be?
Schwarzschild Radius Rs = 2GM c2

3 General Relativity and Black Holes
General Relativity: a theory of gravity Basic mathematical object: 4 dimensional spacetime

4 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

5 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

6 Question: Do black holes exist in nature?
What would you look for? What kind of observation would reveal a black hole?

7 Cygnus X-1: the prototype black hole
Artists’s conception of Cygnus X-1

8 Where Cygnus X-1 is located

9 An example of a black hole system
Black hole and a red dwarf

10 A key to black holes: hot accretion disks

11 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

12 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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