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An Overview of Schwarzschild’s Approach to Black Holes By Trey Paul and Chuck Bryant
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Black Holes Definition:Definition: A celestial object created in the collapse of a very massive star that has a gravitational field so strong that light cannot escape it A celestial object created in the collapse of a very massive star that has a gravitational field so strong that light cannot escape it
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Normal Curvature of Spacetime Due to Mass
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Karl Schwarzschild Born to a Jewish family in Frankfurt, Germany By age 16 had published a paper on the orbits of stars He received his doctorate at the University of Munich Known for his radius
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Metrics ∆s ² = (1− 2GM/c²R)c²∆t² − [1/(1-2GM/c²R)]∆R² − R²(∆θ² + sin²θ∆φ²) 2GM / c² ≡ Rs
![Metrics ∆s ² = (1− 2GM/c²R)c²∆t² − [1/(1-2GM/c²R)]∆R² − R²(∆θ² + sin²θ∆φ²) 2GM / c² ≡ Rs](http://images.slideplayer.com./26/8724282/slides/slide_10.jpg "Metrics ∆s ² = (1− 2GM/c²R)c²∆t² − [1/(1-2GM/c²R)]∆R² − R²(∆θ² + sin²θ∆φ²) 2GM / c² ≡ Rs")
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Works Cited "Embedding Diagram." Philosophy and History of Science, Kyoto University. 30 Nov 2007. Hawley, John F., and Katherine A. Holcomb. Foundations of Modern Cosmology. Oxford: Oxford University Press, 1998. O'Connor, J.J.. "Karl Schwarzschild." Schwarzschild Biography. 30 Nov 2007.
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Works Cited "Relativity." Lecture 15. 30 Nov 2007. Thorne, Kip S.. Black Holes & Time Warps: Einstein's Outrageous Legacy. New York: W.W. Norton & Company, 1994.
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