Calculus of Variations in General Relativity

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SUMMARY

The discussion centers on the calculation of Christoffel connections as presented in Sean M. Carroll's "Spacetime and Geometry." The user seeks clarification on the application of integration by parts in the context of varying the proper time functional, specifically regarding equation 3.52. The resolution confirms that the integration by parts technique is indeed applicable without boundary terms, which are assumed to vanish in this scenario. The user expresses gratitude for the clarification, indicating that a different presentation of the formula was helpful.

PREREQUISITES
  • Understanding of General Relativity concepts, particularly Christoffel connections
  • Familiarity with variational principles in physics
  • Knowledge of integration techniques, specifically integration by parts
  • Proficiency in tensor calculus and the notation used in differential geometry
NEXT STEPS
  • Study the derivation of Christoffel symbols in General Relativity
  • Explore the variational principle in the context of General Relativity
  • Review integration by parts in the context of functional analysis
  • Examine boundary conditions and their implications in variational calculus
USEFUL FOR

Students and researchers in theoretical physics, particularly those focusing on General Relativity and differential geometry, will benefit from this discussion.

wduff
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Hello, this should be an easy one to answer, hope it's in the right place.

I'm going through Sean M. Carroll's text on General Relativity, "Spacetime and Geometry." I'm working through calculating Christoffel connections (section 3.3, if you happen to have the book), which Carroll demonstrates generically by varying the proper time functional.

This yields an integral which he simplifies with "integration by parts," and he provides an example of the procedure for one of the integral's terms (equation 3.52): (sorry about the weird formatting, the integral's down there I promise)

\frac{}{}

\frac{1}{2}\int [g_{\mu \nu }\frac{dx^{\mu }}{d\tau }\frac{d(\delta x^{\nu })}{d\tau }]d\tau =-\frac{1}{2}\int [g_{\mu \nu }\frac{d^{2}x^{\mu }}{d\tau ^{2}}+\frac{dg_{\mu \nu }}{d\tau }\frac{dx^{\mu }}{d\tau }]\delta x^{\nu }d\tau

My problem is, this doesn't look like the "integration by parts" I'm familiar with it. How does sucking out that variational x^nu from the derivative yield the right side of the above equation?

Anyway, if you'd care to help it'd be much appreciated, thanks in advance.
 
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It is exactly integration by parts without the boundary terms, which I assume vanish.
 
Haha so it is... thanks for the link, although I suppose I should have dug it up myself. I just needed to see the formula stated a little differently I guess.

Thanks!
 

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