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====Moving from the Center, Outward through the Core==== <ol> <li> Remembering that the "gridline" with n = 1 is at the center of the configuration, specify value of <math>(\delta r)_n</math> at n = 2. </li> <li> Determine <math>(\delta \rho)_{1.5}</math>, which is the first radial zone. </li> <li> Determine <math>(\delta P)_{1.5}</math> from the core's equation of state. </li> <li> Evaluate the pressure gradient at n = 2 by calculating <math>\tilde{M}_r/(4\pi \tilde{r}^4)</math>, appreciating that <math>\tilde{r}_2 = (r_0 + \delta r)_2</math>. </li> <li> Knowing the pressure gradient at the n = 2 gridline, and the perturbed pressure at n = 1.5, determine <math>(\delta P)_{2.5}</math>. </li> <li> Determine <math>(\delta \rho)_{2.5}</math> from the core's equation of state. </li> <li> Knowing <math>(\delta \rho)_{2.5}</math> and <math>(\delta r)_n</math> at n = 2, determine <math>(\delta r)_n</math> at n = 3. </li> <li> Evaluate the pressure gradient at n = 3 by calculating <math>\tilde{M}_r/(4\pi \tilde{r}^4)</math>, appreciating that <math>\tilde{r}_3 = (r_0 + \delta r)_3</math>. </li> <li> Knowing the pressure gradient at the n = 3 gridline, and the perturbed pressure at n = 2.5, determine <math>(\delta P)_{3.5}</math>. </li> </ol> Repeat from #6 … until we've determined <math>(\delta r)_n</math> at n = 21, that is, the perturbation at the core/envelope interface. Also, go ahead and evaluate the perturbed pressure gradient at the interface; ultimately we need this pressure gradient (as viewed from the perspective of the core) to match the pressure gradient as viewed from then perspective of the envelope.
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