Physics, 12.07.2019 19:10 michaela134
simple stellar models consider a sphere of mass m and radius r. calculate the gravitational potential energy inside the sphere as a function of radius p(r), assuming (a) a density ρ const which is independent of the distance to the center (b) a density which increases towards the centre according to in both cases (a) and (b), write down the volume-averaged average internal pressure needed for hydrostatic pressure, and determine how the pressure within the spher e depends on the distance from the centre
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