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Sean Carroll Chapter 5.1

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  1. Feb 8, 2015 #1
    1. The problem statement, all variables and given/known data
    Consider a perfect fluid in a static, circularly symmetric (2+1)-dimensional spacetime.

    Derive the analogue of the Tolman-Oppenheimer-Volkov (TOV) equation for (2+1)-dimensions

    2. Relevant equations
    Schwarzchild metric

    3. The attempt at a solution
    Okay. I'm trying to think this through. I've replaced the phi component of the schwarzchild metric with some random variable because we only need circular symmetry. but where do I go from here?
     
  2. jcsd
  3. Feb 13, 2015 #2
    Thanks for the post! This is an automated courtesy bump. Sorry you aren't generating responses at the moment. Do you have any further information, come to any new conclusions or is it possible to reword the post?
     
  4. Feb 14, 2015 #3
    Nevermind. I have solved it!
     
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