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

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SUMMARY

The discussion focuses on solving the problem of mass and energy of a collapsing gas shell using the formalism outlined in Exercise 21.25 of "Gravitation" by Misner, Thorne, and Wheeler (MTW). Key metrics involved include the Schwarzschild metric for the exterior, a flat space-time metric for the interior, and a specific metric for the shell defined by ##ds^2 = -d\tau^2 + R^2(\tau)(d\theta^2 + sin^2\theta d\phi^2##. The solution process involves understanding the evolution of the shell over time, represented in ADM coordinates as ##\tau, \theta, and \phi##.

PREREQUISITES
  • Understanding of the Schwarzschild metric in general relativity
  • Familiarity with ADM coordinates and their implications
  • Knowledge of the concept of world tubes in spacetime
  • Access to "Gravitation" by Misner, Thorne, and Wheeler for reference
NEXT STEPS
  • Study the metrics used in general relativity, focusing on the Schwarzschild solution
  • Explore the concept of world tubes and their significance in spacetime geometry
  • Review Exercise 21.25 and related problems in "Gravitation" for deeper insights
  • Read "Problem Book in Relativity and Gravitation" by Lightman, Press, Price, and Teukolsky for practical examples
USEFUL FOR

Students and researchers in theoretical physics, particularly those focusing on general relativity and gravitational dynamics, will benefit from this discussion.

TerryW
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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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