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Falling into a black hole
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Classroom Contents
Black Holes - Lecture 4
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- 1 Summer School on Gravitational-Wave Astronomy
- 2 Black Holes Lecture - 04
- 3 Stability of Stars
- 4 Stability of Matter
- 5 OV: Oppenheimer - Volkoff Equation of State
- 6 Stability of Stars in GTR
- 7 General Relativistic Instability
- 8 Laws of gravitation
- 9 Newtonian Gravity
- 10 Einstein's generalizations
- 11 Einstein's Zeroth Law of Gravity
- 12 In regions where no matter is present
- 13 In regions where matter is present
- 14 Conservation Laws
- 15 Einstein's field equations
- 16 Newtonian limit
- 17 Schwarzschild metric
- 18 The Schwarzschild Geometry
- 19 The Schwarzschild Radius
- 20 The surface of the black hole is known as the Event Horizon
- 21 Approximate metric at large distances from the centre.
- 22 Effective potential in Newtonian theory
- 23 Effective potential in Einstein's theory
- 24 ORBITS in Einstein's theory
- 25 The last "unstable" circular orbit is at a radius of 1.5 Rg. The velocity of the particle will be 'c'
- 26 Important new result
- 27 Gravitational Capture
- 28 Cross Section for Gravitational capture
- 29 Radial Motion of Particles
- 30 Falling towards a black hole
- 31 Time to reach Rg from r = r1
- 32 Falling into a black hole
- 33 Radial motion of photons
- 34 Inside the horizon
- 35 The Lemaitre coordinates 1933
- 36 Q&A
