Momentum conservation for a free-falling body in GR

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SUMMARY

The discussion focuses on the conservation of momentum for a free-falling body in General Relativity (GR), specifically analyzing the equation $$m\frac{\mathrm{d}p_\beta}{\mathrm{d}t} = \frac{1}{2}\left[g_{\mu\beta,\nu}+g_{\nu\mu,\beta} - g_{\nu\beta,\mu} \right]p^\nu p^\mu$$. Participants clarify the symmetry properties of the indices involved, noting that the terms in the brackets do not vanish but exhibit cancellation when contracted with the momentum vectors. The key insight is that the term $$g_{\mu\beta,\nu} - g_{\nu\beta,\mu}$$ is antisymmetric, while the momentum contraction $$p^\nu p^\mu$$ is symmetric, leading to an overall cancellation.

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  • Understanding of General Relativity (GR) principles
  • Familiarity with tensor calculus and index notation
  • Knowledge of the properties of Christoffel symbols
  • Experience with momentum conservation laws in physics
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This discussion is beneficial for physicists, students of General Relativity, and anyone interested in the mathematical foundations of momentum conservation in curved spacetime scenarios.

complexconjugate
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Homework Statement
The conservation law for the energy-momentum vector of a free-falling massive particle is: $$m\frac{\mathrm{d}p^\alpha}{\mathrm{d}t} = -\Gamma^\alpha_{\beta\mu}p^\beta p^\mu$$. Show the conservation law for the covector reads: $$m\frac{\mathrm{d}p_\beta}{\mathrm{d}t} = \frac{1}{2}g_{\mu\nu,\beta}p^\beta p^\mu$$
Relevant Equations
I: $$m\frac{\mathrm{d}p^\alpha}{\mathrm{d}t} = -\Gamma^\alpha_{\beta\mu}p^\beta p^\mu$$
II: $$m\frac{\mathrm{d}p_\beta}{\mathrm{d}t} = \frac{1}{2}g_{\mu\nu,\beta}p^\beta p^\mu$$
Hello everyone!
It seems I can't solve this exercise and I don't know where I fail.
By inserting the metric on the lefthand side of I. and employing the chain rule, the equation eventually reads (confirmed by my notes from the tutorial):
$$m\frac{\mathrm{d}p_\delta}{\mathrm{d}t} = \Gamma^\gamma_{\beta\delta}g_{\mu\gamma}p^\beta p^\mu$$
Now contracting the metric with the Christoffel symbol and renaming indices gives $$m\frac{\mathrm{d}p_\beta}{\mathrm{d}t} = \frac{1}{2}\left[g_{\mu\beta,\nu}+g_{\nu\mu,\beta} - g_{\nu\beta,\mu} \right]p^\nu p^\mu$$
Now I don't understand why two terms in the brackets vanish. Is there some symmetry in the indices I'm missing?
Thanks for any hints.
 
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complexconjugate said:
Homework Statement:: Show the conservation law for the covector reads: $$m\frac{\mathrm{d}p_\beta}{\mathrm{d}t} = \frac{1}{2}g_{\mu\nu,\beta}p^\beta p^\mu$$
Something's wrong here. On the left side, ##\beta## is a lone index. But on the right side, ##\beta## is a summation index.

$$m\frac{\mathrm{d}p_\beta}{\mathrm{d}t} = \frac{1}{2}\left[g_{\mu\beta,\nu}+g_{\nu\mu,\beta} - g_{\nu\beta,\mu} \right]p^\nu p^\mu$$
Now I don't understand why two terms in the brackets vanish. Is there some symmetry in the indices I'm missing?
Thanks for any hints.
In general, none of the terms within the bracket vanish or cancel. However, after contracting the terms in the bracket with ##p^\nu p^\mu##, you will see that there will be some cancellation.
 
TSny said:
Something's wrong here.
I noticed, I copied the Latex code and forgot to swap out the beta... the upper beta should be a nu.
TSny said:
you will see that there will be some cancellation
I think I see what you mean, can you tell me how to justify it properly? Something like symmetry between nu and mu because it's both times contracted with the momentum?

Thank you a lot!
 
complexconjugate said:
I think I see what you mean, can you tell me how to justify it properly? Something like symmetry between nu and mu because it's both times contracted with the momentum?
Yes

$$m\frac{\mathrm{d}p_\beta}{\mathrm{d}t} = \frac{1}{2}\left[g_{\mu\beta,\nu}+g_{\nu\mu,\beta} - g_{\nu\beta,\mu} \right]p^\nu p^\mu$$

To see what happens, consider the first and last terms in the bracket of the right-hand side and contract them with ##p^\nu p^\mu##. Write out these terms explicitly; i.e., carry out the sum over ##\mu## and ##\nu##. You'll probably never need to do that again :oldsmile:

The idea is that ##g_{\mu\beta,\nu} - g_{\nu\beta,\mu}## is antisymmetric with respect to ##\mu## and ##\nu## and it's being contracted with ##p^\nu p^\mu## which is symmetric with respect to ##\mu## and ##\nu##
 
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