Quick expression on geodesic equation

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SUMMARY

The discussion centers on the derivation of the geodesic equation as presented in Hobson's book. The equation is expressed as \(\dot{u}^{\mu} = - \Gamma_{v\sigma}^\mu u^v u^\sigma\), leading to the formulation of \(\dot{u}_{\mu}\) in terms of the metric tensor \(g_{\mu \nu}\) and its derivatives. Key steps include the application of the chain rule and the relationship between the Christoffel symbols and the metric tensor. The final result is achieved through careful cancellations and substitutions, confirming the validity of the derived equation.

PREREQUISITES
  • Understanding of differential geometry concepts, particularly geodesics.
  • Familiarity with the metric tensor and its properties in general relativity.
  • Knowledge of Christoffel symbols and their role in the geodesic equation.
  • Proficiency in tensor calculus and manipulation of tensor equations.
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  • Study the derivation of the geodesic equation in detail using "General Relativity" by Hobson.
  • Explore the implications of the geodesic equation in curved spacetime.
  • Learn about the role of Christoffel symbols in the context of Riemannian geometry.
  • Investigate applications of geodesics in modern physics, such as in cosmology and gravitational wave studies.
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This discussion is beneficial for physicists, mathematicians, and students studying general relativity, particularly those focusing on the mathematical foundations of geodesics and their applications in theoretical physics.

unscientific
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Taken from Hobson's book:

geodesic1.png


How did they get this form?

[tex]\dot u^{\mu} = - \Gamma_{v\sigma}^\mu u^v u^\sigma[/tex]
[tex]\dot u^{\mu} g_{\mu \beta} \delta_\mu ^\beta = - g_{\mu \beta} \delta_\mu ^\beta \Gamma_{v\sigma}^\mu u^v u^\sigma[/tex]
[tex]\dot u_{\mu} = - \frac{1}{2} g_{\mu \beta} \delta_\mu ^\beta g^{\mu \gamma} \left(\partial_v g_{\sigma \gamma} + \partial_\sigma g_{v\gamma} - \partial_\gamma g_{v\sigma} \right)[/tex]
[tex]= - \frac{1}{2} \delta_\mu ^\beta \delta_\beta ^\gamma \left(\partial_v g_{\sigma \gamma} + \partial_\sigma g_{v\gamma} - \partial_\gamma g_{v\sigma} \right)[/tex]
[tex]= -\frac{1}{2} \left( \partial_v g_{\sigma \mu} + \partial_\sigma g_{v\mu} - \partial_\mu g_{v\sigma} \right)[/tex]

Why are the first two terms zero?
 
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unscientific said:
Taken from Hobson's book:

geodesic1.png


How did they get this form?

[tex]\dot u^{\mu} = - \Gamma_{v\sigma}^\mu u^v u^\sigma[/tex]
[tex]\dot u^{\mu} g_{\mu \beta} \delta_\mu ^\beta = - g_{\mu \beta} \delta_\mu ^\beta \Gamma_{v\sigma}^\mu u^v u^\sigma[/tex]
[tex]\dot u_{\mu} = - \frac{1}{2} g_{\mu \beta} \delta_\mu ^\beta g^{\mu \gamma} \left(\partial_v g_{\sigma \gamma} + \partial_\sigma g_{v\gamma} - \partial_\gamma g_{v\sigma} \right)[/tex]
[tex]= - \frac{1}{2} \delta_\mu ^\beta \delta_\beta ^\gamma \left(\partial_v g_{\sigma \gamma} + \partial_\sigma g_{v\gamma} - \partial_\gamma g_{v\sigma} \right)[/tex]
[tex]= -\frac{1}{2} \left( \partial_v g_{\sigma \mu} + \partial_\sigma g_{v\mu} - \partial_\mu g_{v\sigma} \right)[/tex]

Why are the first two terms zero?

Since [itex]u_\mu = g_{\mu \nu} u^\nu[/itex], then
[itex]\dot{u}_\mu = \dot{g}_{\mu \nu} u^\nu + g_{\mu \nu} \dot{u}^\nu[/itex]

Using the chain rule, or whatever the rule is, [itex]\dot{g}_{\mu \nu} = u^\sigma \partial_\sigma g_{\mu \nu}[/itex]. So we have:

[itex]\dot{u}_\mu = u^\sigma u^\nu \partial_\sigma g_{\mu \nu} + g_{\mu \nu} \dot{u}^\nu[/itex]

Using [itex]\dot{u}^\nu = - \Gamma^\nu_{\sigma \lambda} u^\sigma u^\lambda[/itex], we have:

[itex]\dot{u}_\mu = u^\sigma u^\nu \partial_\sigma g_{\mu \nu} - g_{\mu \nu} \Gamma^\nu_{\sigma \lambda} u^\sigma u^\lambda[/itex]

Finally, using [itex]g_{\mu \nu} \Gamma^\nu_{\sigma \lambda} = \Gamma_{\mu \sigma \lambda} = \frac{1}{2}(\partial_\sigma g_{\mu \lambda} + \partial_\lambda g_{\mu \sigma} - \partial_\mu g_{\sigma \lambda})[/itex], we can write this as:

[itex]\dot{u}_\mu = u^\sigma u^\nu \partial_\sigma g_{\mu \nu} - \frac{1}{2} u^\sigma u^\lambda (\partial_\sigma g_{\mu \lambda} + \partial_\lambda g_{\mu \sigma} - \partial_\mu g_{\sigma \lambda})[/itex]

After some cancellations, you get their result.
 
stevendaryl said:
Since [itex]u_\mu = g_{\mu \nu} u^\nu[/itex], then
[itex]\dot{u}_\mu = \dot{g}_{\mu \nu} u^\nu + g_{\mu \nu} \dot{u}^\nu[/itex]

Using the chain rule, or whatever the rule is, [itex]\dot{g}_{\mu \nu} = u^\sigma \partial_\sigma g_{\mu \nu}[/itex]. So we have:

[itex]\dot{u}_\mu = u^\sigma u^\nu \partial_\sigma g_{\mu \nu} + g_{\mu \nu} \dot{u}^\nu[/itex]

Using [itex]\dot{u}^\nu = - \Gamma^\nu_{\sigma \lambda} u^\sigma u^\lambda[/itex], we have:

[itex]\dot{u}_\mu = u^\sigma u^\nu \partial_\sigma g_{\mu \nu} - g_{\mu \nu} \Gamma^\nu_{\sigma \lambda} u^\sigma u^\lambda[/itex]

Finally, using [itex]g_{\mu \nu} \Gamma^\nu_{\sigma \lambda} = \Gamma_{\mu \sigma \lambda} = \frac{1}{2}(\partial_\sigma g_{\mu \lambda} + \partial_\lambda g_{\mu \sigma} - \partial_\mu g_{\sigma \lambda})[/itex], we can write this as:

[itex]\dot{u}_\mu = u^\sigma u^\nu \partial_\sigma g_{\mu \nu} - \frac{1}{2} u^\sigma u^\lambda (\partial_\sigma g_{\mu \lambda} + \partial_\lambda g_{\mu \sigma} - \partial_\mu g_{\sigma \lambda})[/itex]

After some cancellations, you get their result.

Brilliant, thank you!
 

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