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03_E2_ws2_key
03_E2_ws2_key

... 3. Calculate the gravitational potential difference between: a) point A and the base of the hill GP = gh = (10N/kg)-100m = -1000J/kg b) point B and the base of the hill GP = gh = (10N/kg)-200m = -2000J/kg c) point C and point A GP = gh = (10N/kg) 0m = 0 d) point C and point E GP = gh = (10N/kg)2 ...
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... relatively elongated by about 1.0 x 10–9. If the gravitational field is not uniform over the rod, the spacings are affected non-uniformly; so, the rod is deformed. 6.4 Vibrating particle and point-dense mass The factor m/r in (18), (22), and (26) is meaningful as range density (m/r) or point density ...
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... Block 1 (mass M1) rests on a horizontal surface. A horizontal string is attached to the block, passing over a pulley to a hanging block having mass M2 which hangs vertically a distance h from the floor. The pulley is a uniform cylinder of mass M and radius R. The string has negligible mass and the p ...
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... Editor's INTRODUCTION "Newton attempted to explain the force of gravity on two hypotheses: the existence of a medium, or ether, and action at a distance. The first hypothesis he rejected as being physically absurd, the second as contrary to reason. Newton had, therefore, no theory of gravity. Howev ...
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... What is a Neutron Star? • The collapsed core of a medium-sized star, 3 to 8 times the mass of our sun. • The core of this star had to have a mass greater than the Chandrasekhar Limit, 1.4 times the sun’s mass. ...
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... 15. When a falling object stops accelerating, it has reached______________________ velocity. 16. If there were no air resistance, what would be the velocities of hailstones during a hailstorm? _______________________________________________________________ 17. The motion of a body when only the forc ...
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... by the results obtained from the study of Hawking effect, Chapter 4 also explains the laws of black hole thermodynamics, particularly the generalized second law of thermodynamics. In Chapter 5 we study quantum fields in FRW universes. Calculations are again simplified by considering a scalar field i ...
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Introduction to general relativity

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