Question about tensor derivative

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The discussion centers on the derivation of equations of motion for a force-free particle in General Relativity (GR) using the Lagrangian formalism as presented in Stephani's book. The Lagrangian is defined as L = (m/2) g_{αβ} ẋ^α ẋ^β. The participant seeks clarification on the origin of the second term in the equation g_{αν} ẋ̈^α + g_{αν,β} ẋ^α ẋ^β - (1/2)g_{αβ,ν} ẋ^α ẋ^β = 0. The response highlights the application of the product and chain rules in differentiation, emphasizing that the metric tensor g_{αν} is time-dependent, which is crucial for understanding the dynamics involved.

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lync4495
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Hello,

I'm beginning to learn GR and ran across the following in the beginning of Stephani's book.

In deriving the equations of motion for a force-free particle, we have the Lagrangian:
[tex]L = \frac{m}{2} g_{\alpha \beta} \dot{x}^\alpha \dot{x}^\beta[/tex]

To construct the equations of motion we need
[tex]\frac{\partial L}{\partial \dot{x}^\nu} = m g_{\alpha \nu} \dot{x}^\alpha[/tex]

and

[tex]\frac{\partial L}{\partial x^\nu} = L_{,\nu} = \frac{m}{2} g_{\alpha \beta, \nu} \dot{x}^\alpha \dot{x}^\beta[/tex]

Then from the Lagrange equations we get

[tex]g_{\alpha \nu }\ddot{x}^\alpha + g_{\alpha \nu, \beta} \dot{x}^\alpha \dot{x}^\beta - \frac{1}{2}g_{\alpha \beta, \nu}\dot{x}^\alpha \dot{x}^\beta =0[/tex]

I don't understand where the second term in the last equation comes from.
 
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lync4495 said:
Hello,

I'm beginning to learn GR and ran across the following in the beginning of Stephani's book.

In deriving the equations of motion for a force-free particle, we have the Lagrangian:
[tex]L = \frac{m}{2} g_{\alpha \beta} \dot{x}^\alpha \dot{x}^\beta[/tex]

To construct the equations of motion we need
[tex]\frac{\partial L}{\partial \dot{x}^\nu} = m g_{\alpha \nu} \dot{x}^\alpha[/tex]

and

[tex]\frac{\partial L}{\partial x^\nu} = L_{,\nu} = \frac{m}{2} g_{\alpha \beta, \nu} \dot{x}^\alpha \dot{x}^\beta[/tex]

Then from the Lagrange equations we get

[tex]g_{\alpha \nu }\ddot{x}^\alpha + g_{\alpha \nu, \beta} \dot{x}^\alpha \dot{x}^\beta - \frac{1}{2}g_{\alpha \beta, \nu}\dot{x}^\alpha \dot{x}^\beta =0[/tex]

I don't understand where the second term in the last equation comes from.

It comes from the product and chain rules:

[tex]\frac{d}{d \tau} \left( \frac{\partial L}{\partial \dot{x}^\nu} \right) = m \frac{d}{d \tau} \left( g_{\alpha \nu} \dot{x}^\alpha \right) = m \frac{d}{d \tau} \left( g_{\alpha \nu} \right) \dot{x}^\alpha + m g_{\alpha \nu} \frac{d}{d \tau} \left( \dot{x}^\alpha \right).[/tex]

In the second-last term,

[tex]\frac{d}{d \tau} = \frac{d x^\beta}{d \tau}\frac{\partial}{\partial x^\beta}[/tex]

is used.
 
Oh ok. Thank you.

I wasn't realizing the metric tensor was a function of time. Now that I think about it, it makes sense that it is.
 

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