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The top documents tagged [classical gas]
1 Dr J. Miao PH507 The Hydrostatic Equilibrium Equations for Stars
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Stellar Interior. Solar Facts Radius: –R = 7 10 5 km = 109 R E Mass : –M = 2 10 30 kg –M = 333,000 M E Density: – = 1.4 g/cm 3 –(water is
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1 Mr T. Tunnukij & Dr. C. Hicks, University of Newcastle upon Tyne Teerawut Tunnukij Christian Hicks
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Prof. Ming-Jer Chen Department of Electronics Engineering National Chiao-Tung University
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Nearly perfect liquids: strongly coupled systems from quark-gluon plasmas to ultracold atoms Gordon Baym University of Illinois 8 April 2009 8 April 2009
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PH507 The Hydrostatic Equilibrium Equations for Stars
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Compressor Less Refregerator Peltier Effect
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Shear viscosity of a gluon plasma in heavy ion collisions
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An Introduction to Statistical Mechanics and Thermodynamics - Swendsen
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