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Introductory Lectures on Black Hole Thermodynamics
www.physics.umd.edur=0 M 3M 4M 5M v = const. Figure 1.1: Diagram of the positive mass EF spacetime, suppressing the angular coordinates, with constant r surfaces vertical and constant v surfaces at 45–. collapsing shell Figure 1.2: Picture of a black hole that forms from a collapsing shell of matter. Since the Schwarzschild \time" coordinate t goes to inflnity at the event horizon, these coordinates are