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Stellar structure of stars problem

  1. Mar 4, 2014 #1
    1. The problem statement, all variables and given/known data
    Consider a star of radius R, with density p that is constant, composed of classical, nonrelativistic, idealg gas of fully ionized hydrogen.
    a. Solve the equations of stellar structure for the pressure profile, P(r) with the boundary condition P(R)=0
    b. Find the temperature profile T(r)
    c. Assume that the nuclear energy production rate depends on temperature as E==T^4. At what radius does E decrease to 0.1 of its central value, and what fraction of the star's volume is included within this radius?


    2. Relevant equations
    A) dP(r)=-G*M(r)*ρ(r)*dr/r^2
    B)dT(r)/dr = -3/4 *( L(r)*k(r)*ρ(r))/(4∏r^24acT(r)^3)
    C) I'm not sure about the formulas for C



    3. The attempt at a solution
    I think I get A part. You have to integrate from r to R of
    dP(r)=-G*M(r)*ρ*dr/r^2 ;ρ= M(r)/(4/3)∏r^3, solve for M(r)
    =-G*ρ^2*(4/3)*∏*integration of r

    b part: I have no idea. Which values will be constant and why?

    c part: I'm also not sure which equations to use

    Please help and explain thoroughly or set me on the right track! Also please explain the concepts too! Thanks
     
  2. jcsd
  3. Mar 4, 2014 #2

    SteamKing

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    For part c, you have to solve part b and figure out the radial distribution of temperature within the star.
     
  4. Mar 4, 2014 #3
    Thanks!
    any idea on part b?
     
  5. Mar 4, 2014 #4

    SteamKing

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    You've got a first order ODE to solve here. It's not clear what functions L(r) and k(r) are and how they vary with r, nor what boundary conditions to apply.
     
  6. Mar 4, 2014 #5
    Yeah, that's what I'm trying to figure out. Would the luminosity be constant in this case? or would I need another equation to substitute it with?
     
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