Mass/Energy of a collapsing gas shell (MTW 21.27)

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The discussion focuses on solving the problem of the mass and energy of a collapsing gas shell using the formalism from Exercise 21.25. Key points include the use of three metrics: the Schwarzschild metric outside the shell, flat space-time inside, and a specific metric for the shell itself. As the shell evolves, it creates a 'world tube' with space-like normals, leading to the identification of coordinates in ADM terms. Additionally, a reference to the Problem Book in Relativity and Gravitation is suggested for further guidance. Overall, the conversation emphasizes the importance of understanding the metrics and their implications for solving the problem.
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Homework Statement
Derive equation 21.176e for a collapsing gas shell
Relevant Equations
See attached extract from MTW
Hi Everyone.

Can anyone give me some hints which will point out how to solve this problem, particularly using 'the formalism of Ex 21.25'.

I've kicked this around for a couple of weeks now and I haven't been able to come up with anything.

Regards

TerryW

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Hi to any reader passing this way.

If you too are stuck on this problem, I can now offer a few thoughts on how to get to the solution after being given some very helpful guidance by TSny.

1. There are three metrics to be used - The metric outside the shell (Schwartzschild), the metric inside the shell (flat space-time) and the metric on the shell itself (which isn't given but is
##ds^2 = -d\tau^2 + R^2(\tau)(d\theta^2 + sin^2\theta d\phi^2##)

2. As the shell evolves with time (##\tau##), it creates a 'world tube', the normal to which is space-like. The consequence of this is that in ADM co-ordinate speak, the three co-ordinates of the shell are ## \tau, \theta and \phi## which correspond to i,j, and k.

(It took a good bit of time and some valuable help from TSny to get comfortable with the idea that n doesn't have to be time-like).

3. The quick way is to locate a copy of Problem Book in Relativity and Gravitation by Lightman, Press, Price and Teukolsky and turn to page 586.

So thanks to TSnyTerryW
 
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