Prove that at the event horizon of a black hole the time becomes zero or freezes.
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A: Required: The value of the Ricci tensor on the event horizon of a Schwarzschild black hole.
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- A black hole is defined as a region in spacetime where the gravitational force is so large that nothing can escape the gravitational pull. Not even light has enough speed to escape the gravity of a black hole.
- The event horizon of a black hole is defined as the distance beyond which the escape velocity crosses the speed of light. It is given by the Schwarzschild radius,
Here G is the universal gravitational constant, M is the mass of the black hole, and c is the speed of light.
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- In 1999, scientists discovered a new class of black holes with masses 100 to 10,000 times the mass of our sun that occupy less space than our moon. Suppose that one of these black holes has a mass of 1x10^3 suns and a radius equal to one-half the radius of our moon. What is the density of the black hole in g/cm^3? The radius of our sun is 7.0x10^5 km, and it has an average density of 1.4x10^3 kg/m^3. The diameter of the moon is 2.16x10^3 miles.How would it appear to an outside observer if someone were to enter a black hole?Let's say a spaceship is approaching Sagittarius A*. How close to this black hole must the spaceship get to experience time twice as slowly?
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