latentcorpse
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I'm a bit confused by the following:
We can derive the equation of motion for a particle traveling on a timelike worldline by applying the Euler-Lagrange equations to the Lagrangian
\mathcal{L}=- g_{\mu \nu}(x(\tau)) \frac{d x^\mu}{d \tau} \frac{d x^\nu}{d \tau}
However, to derive the field equations of General Relativity, we extremise the Einstein-Hilbert action
S_{\text{EH}}[g] = \frac{1}{16 \pi} \int_{\mathcal{M}} d^4x \sqrt{-g} R where the integration is performed over the manifold \mathcal{M} and R is the Ricci Scalar
However this suggests that the necessary Lagrangian is
\mathcal{L}=\frac{1}{16 \pi} R i.e. the integrand of the Einstein-Hilbert action.
My question is, why are the two Lagrangians the same. Surely they should be?
Secondly, I understand the motivation for the Einstein-Hilbert action, but where does the first Lagrangian actually come from? As far as I can tell they just seem to introduce it so that we end up with \ddot{x^\mu} + \Gamma^\mu{}_\nu \rho} \dot{x}^\nu \dot{x}^\rho=0 after applying the Euler-Lagrange equations.
We can derive the equation of motion for a particle traveling on a timelike worldline by applying the Euler-Lagrange equations to the Lagrangian
\mathcal{L}=- g_{\mu \nu}(x(\tau)) \frac{d x^\mu}{d \tau} \frac{d x^\nu}{d \tau}
However, to derive the field equations of General Relativity, we extremise the Einstein-Hilbert action
S_{\text{EH}}[g] = \frac{1}{16 \pi} \int_{\mathcal{M}} d^4x \sqrt{-g} R where the integration is performed over the manifold \mathcal{M} and R is the Ricci Scalar
However this suggests that the necessary Lagrangian is
\mathcal{L}=\frac{1}{16 \pi} R i.e. the integrand of the Einstein-Hilbert action.
My question is, why are the two Lagrangians the same. Surely they should be?
Secondly, I understand the motivation for the Einstein-Hilbert action, but where does the first Lagrangian actually come from? As far as I can tell they just seem to introduce it so that we end up with \ddot{x^\mu} + \Gamma^\mu{}_\nu \rho} \dot{x}^\nu \dot{x}^\rho=0 after applying the Euler-Lagrange equations.