Timelike Geodesics: Solving Reissner Nordstrom Line Element

  • Thread starter Thread starter alex_b93
  • Start date Start date
  • Tags Tags
    Geodesics
Join the discussion
Registration is free. Ask a follow-up in this thread, or start your own.
2 replies · 1K views
alex_b93
Messages
12
Reaction score
0

Homework Statement


Using the Reissner Nordstrom line element, which I've given in the relevant equations section, I'm looking to show that the time like Geodesics obey the equation again show below.

Homework Equations


Line Element[/B]
##ds^2= - U(r)c^2dt^2 +\frac{dr^2}{U(r)} +r^2(d\theta^2 + sin^2(\theta)d\phi^2)##
##U(r)=1-\frac{r_s}{r}+\frac{G^2Q^2}{r^2}##

Equation to Obey
##\frac{1}{2} (\frac{dr}{d\tau})^2 +V(r) = \varepsilon##

The Attempt at a Solution


I've presumed as we are looking for a ##dr'## the Euler Lagrange equation we would be interested would be[/B]
##\frac{d}{d\tau}(\frac{\partial L^2}{\partial r'}) - \frac{\partial L^2}{\partial r}##

If I work this through my answer doesn't really resemble the equation I'm looking for, I get the ##(\frac{dr}{d\tau})^2##, but I can't get the ##\frac{1}{2}## factor, plus I have other terms in the denominator.
I also have a lot of other terms but they could possibly be grouped into ##V(r)##.

I was hoping somebody could confirm whether the method I'm attempting is correct, as then I'll know if I'm incorrectly calculating it or it is something else.

Many thanks.
 
Physics news on Phys.org
Here are a couple of other hints:

First, [itex]\tau[/itex] and [itex]s[/itex] are the same thing, so [itex]\frac{ds}{d\tau} = 1[/itex]. So if you take the expression for [itex]s[/itex], this gives you one "constant of the motion".

Second, if you have a Lagrangian of the form [itex]L(r, \frac{dr}{d\tau}, t, \frac{dt}{d\tau}, \theta, \frac{d\theta}{d\tau}, \phi \frac{d\phi}{d\tau})[/itex], and [itex]L[/itex] doesn't mention [itex]\tau[/itex], then the following quantity is conserved (has the same value for all [itex]\tau[/itex]):

[itex]H = (\sum_j P_j U^j) - L[/itex]

where [itex]U^j = \frac{d x^j}{d\tau}[/itex] and [itex]P_j = \dfrac{\partial L}{\partial U^j}[/itex].

So [itex]H[/itex] gives you a second constant of the motion. So [itex]H = E[/itex], for some constant [itex]E[/itex]