We are going to solve the equations stellar structure - with some simplified assumptions. (a) Obtain an expression for t

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We Are Going To Solve The Equations Stellar Structure With Some Simplified Assumptions A Obtain An Expression For T 1 (37.76 KiB) Viewed 178 times

We are going to solve the equations stellar structure - with some simplified assumptions. (a) Obtain an expression for the pressure profile (ie P(r)) of a star with constant density p, where the outer boundary, R, is P(R)=0. (b) Use the appropriate equation of state to obtain the related temperature profile, T(r). (c) The generation of energy in a star is given by e(p, T, composition). In the star described above, e x T4 as is approximately true for the p-p chain. At what radius will the energy generation drop to 20% of the central value? Ignore the effects of composition on the energy generation.