Sean Carroll Chapter 5.1

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Homework Statement


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

Homework Equations


Schwarzchild metric

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?
 

Answers and Replies

  • #2
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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?
 
  • #3
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Nevermind. I have solved it!
 

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