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Unformatted text preview: PHYS5523 Theory of Relativity Test 2: The Gravitational Field of a Single Body November 2, 2011 General Instructions: This is a three hour, open book test with three problems. Complete all three problems. Problem 1: A Radially Infalling Observer. a) Demonstrate that a radially infalling observer always measures the speed of radially moving photons (whether they are traveling inwards or outward) to be c relative to his own velocity. Accomplish this by finding the velocity of both the photons and the observer himself in the reference frame of a radially infalling observer as given by the GullstrandPainleve coordinates. The Schwarschild metric in GullstrandPainleve coordinates is ds 2 = (1 2 M r ) dt ′ 2 + 2 radicalbigg 2 M r dt ′ dr + dr 2 + r 2 dθ 2 + r 2 sin 2 θdφ 2 (1) where t ′ is the GullstrandPainleve coordinate time, which is the same as the proper time for an observer freelyfalling from infinity, and r , θ and φ are the Schwarzschild coordinates of the same name. b) Now consider the viewpoint of a radially infalling observer (observer 1) compared to that of an observer stationary at infinity in the Schwarzschild...
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This note was uploaded on 12/01/2011 for the course PHYS 5523 taught by Professor Kennefick during the Fall '11 term at Arkansas.
 Fall '11
 Kennefick
 Theory Of Relativity

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