Getting geodesic from variational principle

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The discussion focuses on deriving the geodesic equation from a given metric using the variational principle. The initial attempt to variate the action leads to an incorrect equation, prompting questions about the correctness of the Lagrangian used. It is suggested that the Euler-Lagrange equations derived from different forms of the Lagrangian may yield different results, complicating the derivation. A correct approach involves using the Lagrangian that directly incorporates the metric and considers energy levels. Ultimately, the conversation emphasizes the importance of the correct formulation of the Lagrangian to achieve the desired geodesic equation.
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Homework Statement
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Relevant Equations
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The metric is $$ds^2 = \frac{dr^2 + r^2 d\theta ^2}{r^2-a^2} - \frac{r^2 dr^2}{(r^2-a^2)^2}$$

I need to prove the geodesic is: $$a^2 (\frac{dr}{d \theta})^2 + a^2 r^2 = K r^4$$

My method was to variate the action ##\int\frac{(\frac{dr}{d\theta})^2 + r^2 }{r^2-a^2} - \frac{r^2 (\frac{dr}{d\theta})^2}{(r^2-a^2)^2} d \theta##

But the equation i am getting is $$a^2 (\frac{dr}{d \theta})^2 + r^2 = K (r^2-a^2)^2$$
Which can not be reduced to the answer.

I am a little confused, i could simpy calculate the Christoffel symbol, but i think this variation method easier, yet i am not sure how to use it.

So basically, my guess on why i have got the wrong answer is that the "lagrangean" i am variating is wrong. So what lagrangean indeed give us the right answer? Only ##g_{ab} \frac{dx^a}{ds} \frac{dx^b}{ds}= 1 ## and ##\sqrt{g_{ab} \frac{dx^a}{d\lambda} \frac{dx^b}{d\lambda}}##? Or the lagrangean i used above is right, and i have done some algebric error?
 
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Your approach failed because in general the Euler-Lagrange equations produced from L_1(r, dr/d\theta) are not the same as those obtained from L_2(r, dr/d\theta) = \sqrt{L_1}: <br /> \begin{split}<br /> \frac{d}{d\theta} \left( \frac{\partial L_2}{\partial r&#039;}\right) - \frac{\partial L_2}{\partial r}<br /> &amp;= \frac{d}{d\theta} \left( \frac{1}{2L_2} \frac{\partial L_1}{\partial r&#039;} \right) - \frac{1}{2L_2}\frac{\partial L_1}{\partial r} \\<br /> &amp;= \frac{1}{2L_2} \left[\frac{d}{d\theta} \left( \frac{\partial L_1}{\partial r&#039;}\right) - \frac{\partial L_1}{\partial r}\right] + \frac{\partial L_1}{\partial r&#039;} \frac{d}{d\theta}\left( \frac{1}{2L_2} \right) \\<br /> &amp;\neq \frac{1}{2L_2} \left[\frac{d}{d\theta} \left( \frac{\partial L_1}{\partial r&#039;}\right) - \frac{\partial L_1}{\partial r}\right]<br /> \end{split}<br /> If you take s as the independent variable then you can work with f(r) r&#039;^2 + g(r) \theta&#039;^2 directly because by definition its total derivative with respect to s is zero and you end up with the same Euler-Lagrange equation as you obtain from \sqrt{f(r) r&#039;^2 + g(r) \theta&#039;^2}.
 
You have a Lagrangian system
$$L=\dot r^2\Big(\frac{1}{r^2-a^2}-\frac{r^2}{(r^2-a^2)^2}\Big)+\frac{r^2}{r^2-a^2}\dot\theta^2.$$
You must consider this system at the energy level ##L=1##
perhaps the following cyclic integral will be of use
$$\frac{\partial L}{\partial \dot \theta}=const$$
 
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