Solving Radially-Directed Geodesics in AdS Space

In summary, we are given the global AdS metric in terms of coordinates and a geodesic equation. Using the Christoffel symbols, we simplify the equations for the radially-directed geodesics and look for massless solutions. Using reduction of order, we find a solution for the metric and solve for \tau(\rho).
  • #1
physicus
55
3

Homework Statement



We consider global AdS given by the coordinates [itex](\rho,\tau, \Omega_i), i=1,\ldots,d[/itex] and the metric
[itex] ds^2=L^2(-cosh^2\,\rho\,d\tau^2+d\rho^2+sinh^2\,\rho\,d \Omega_i{}^2)[/itex]
Find the trajectory [itex]\tau(\rho)[/itex], radially-directed geodesics, strating from [itex]\rho=\rho_0[/itex] with proper time [itex]\tau(\rho_0)[/itex].


Homework Equations



Geodesic equation: [itex]\frac{d^2x^{\mu}}{d \lambda^2}+\Gamma^\mu_{\nu \alpha}\frac{dx^\nu}{d \lambda}\frac{dx^\alpha}{d \lambda}=0[/itex]


The Attempt at a Solution



I calculated the Christoffel symbols to obtain the following non-zero components:
[itex]\Gamma^\rho_{\tau\tau}=sinh\,\rho[/itex]
[itex]\Gamma^\phi_{ii}=-cosh\,\rho[/itex]
[itex]\Gamma^\tau_{\rho\tau}=\Gamma^\tau_{\tau\rho}=tanh\,\rho[/itex]
[itex]\Gamma^i_{\rho i}= \Gamma^i_{i\rho}=coth\,\rho[/itex]

Using the geodesic equation this yields:
[itex]\frac{d^2\rho}{d\lambda^2}+sinh\,\rho\,\left(\frac{d\tau}{d\lambda}\right)^2-\sum_i cosh\,\rho\,\left(\frac{d\Omega_i}{d\lambda}\right)^2=0[/itex]
[itex]\frac{d^2\tau}{d\lambda^2}+2tanh\,\rho\,\frac{d \rho}{d\lambda}\frac{d\tau}{d\lambda}=0[/itex]
[itex]\frac{d^2\Omega_i}{d\lambda^2}+2coth\,\rho\,\sum_j \frac{d \rho}{d\lambda}\frac{d\Omega_j}{d\lambda}=0[/itex]

We are looking for radially directed geodesics, i.e. try if there are solutions with [itex]\frac{d \Omega_i}{d\lambda}=0[/itex]. Since this ansatz leads to [itex]\frac{d^2 \Omega_i}{d\lambda^2}=0[/itex] it is consistent with the above equations. Therefore, we can simplify:
[itex]\frac{d^2 \rho}{d\lambda^2}+sinh\,\rho\,\left(\frac{d\tau}{d\lambda}\right)^2=0[/itex] (*)
[itex]\frac{d^2\tau}{d\lambda^2}+2tanh\,\rho\,\frac{d \rho}{d\lambda}\frac{d\tau}{d\lambda}=0[/itex]

Since we look for massless geodesics we require
[itex]g_{\mu\nu}\frac{dx^\mu}{ \lambda}\frac{dx^\nu}{d \lambda}=0[/itex]
[itex]\Rightarrow -cosh\,\rho\,\left(\frac{d\tau}{d\lambda}\right)^2+\left(\frac{d\rho}{d\lambda}\right)^2+\sum_i sinh\,\rho\,\left(\frac{d\Omega_i}{d\lambda}\right)^2=0[/itex]
[itex]\Rightarrow -cosh\,\rho\,\left(\frac{d\tau}{d\lambda}\right)^2+\left(\frac{d\rho}{d\lambda}\right)^2 = 0[/itex]

We can use this to simplify (*) to get
[itex] \frac{d^2\rho}{d\lambda^2}+tanh\,\rho\,\left(\frac{d\rho}{d\lambda}\right)^2=0[/itex]

However, I still don't see a solution. Does anyone have an idea?

Cheers, physicus
 
  • Like
Likes jadyliber
Physics news on Phys.org
  • #2
physicus said:
I calculated the Christoffel symbols to obtain the following non-zero components:
[itex]\Gamma^\rho_{\tau\tau}=sinh\,\rho[/itex]
[itex]\Gamma^\phi_{ii}=-cosh\,\rho[/itex]

These two Christoffels were wrong. It should be
[itex]\Gamma^\rho_{\tau\tau}=sinh\,\rho\,cosh\,\rho[/itex]
[itex]\Gamma^\phi_{ii}=-sinh\,\rho\,cosh\,\rho[/itex]

However, I end up with the same equation.
 
  • #3
Try reduction of order. Set

[tex]u = \frac{d\rho}{d\lambda},[/tex]

so that

[tex]\frac{d^2 \rho}{d\lambda^2} = \frac{du}{d\lambda} = \frac{du}{d\rho} \frac{d\rho}{d\lambda} = \frac{du}{d\rho}u.[/tex]
 
  • #4
physicus said:

Homework Statement



Since we look for massless geodesics we require
[itex]g_{\mu\nu}\frac{dx^\mu}{ \lambda}\frac{dx^\nu}{d \lambda}=0[/itex]

Why are you looking for massless geodesics? Is this required?
 
  • #5
Sorry, I forgot the "massless" in the problem statement. It is indeed required.

I try reduction of order [itex]u=\frac{d\rho}{d\lambda}, v=\frac{d\tau}{d\lambda}[/itex].

This yields
[itex]\frac{du}{d\lambda}+tanh\,\rho\,u^2=0[/itex]
Since [itex]\frac{du}{d\lambda}=\frac{du}{d\rho}u[/itex] we get
[itex]\frac{du}{d\rho}=-tanh\,\rho\,u[/itex]
[itex]\Rightarrow u=\frac{1}{cosh\,\rho}[/itex]
[itex]\Rightarrow \frac{d\rho}{d\lambda}=\frac{1}{cosh\,\rho}[/itex]

Also, from the second equation [itex]\frac{d^2\tau}{d\lambda^2}+2tanh\,\rho\,\frac{d \rho}{d\lambda}\frac{d\tau}{d \lambda}=0[/itex]
[itex]\Rightarrow \frac{dv}{d\lambda}+2tanh\,\rho\,\frac{d\rho}{d \lambda}v=0[/itex]
Since [itex]\frac{dv}{d\lambda}=\frac{dv}{d\rho}\frac{d\rho}{d\lambda}[/itex]
[itex]\Rightarrow \frac{dv}{d\rho}+2tanh\,\rho\,v=0[/itex]
[itex]\Rightarrow \frac{dv}{v}=-2tanh\,\rho\,d\rho[/itex]
[itex]\Rightarrow log\,v=-2log\,cosh\,\rho[/itex]
[itex]\Rightarrow v=\frac{1}{cosh^2\,\rho}[/itex]
[itex]\Rightarrow \frac{d\tau}{d\lambda}=\frac{1}{cosh^2\,\rho}[/itex]

This is in agreement with the third equation I found:
[itex]-cosh^2\,\rho\,\left(\frac{d\tau}{d\lambda}\right)^2+\left(\frac{d\rho}{d\lambda}\right)^2=0[/itex]

We want to find [itex]\tau(\rho)[/itex]. Can we conclude the following?
[itex]\frac{d\tau}{d\rho}=\frac{d\tau}{d\lambda}\frac{d \lambda}{d\rho}= \frac{d\tau}{d\lambda}\left(\frac{d\rho}{d\lambda}\right)^{-1}=\frac{1}{cosh\,\rho}[/itex]

This would yield: [itex]\tau(\rho)=2tan^{-1}(tanh(\rho/2))+\tau(\rho_0)[/itex]
This seems a bit complicated. Is it right?
 

FAQ: Solving Radially-Directed Geodesics in AdS Space

What is AdS space and why is it important in science?

AdS space, short for anti-de Sitter space, is a type of curved space in which the geometry is described by the anti-de Sitter metric. It is important in science because it is used to model certain phenomena in theoretical physics, including black holes and higher-dimensional space-time.

What are radially-directed geodesics and how are they solved in AdS space?

Radially-directed geodesics are paths that follow the shortest distance between two points in a curved space. In AdS space, these paths can be solved using the geodesic equation, which describes the motion of a particle in a curved space.

What are some real-world applications of solving radially-directed geodesics in AdS space?

Solving radially-directed geodesics in AdS space has practical applications in fields such as astrophysics and cosmology. It can help us understand the behavior of particles in the vicinity of black holes, as well as the dynamics of the early universe.

What are some challenges in solving radially-directed geodesics in AdS space?

One of the main challenges in solving radially-directed geodesics in AdS space is the difficulty in obtaining precise solutions due to the complexity of the geodesic equation. Additionally, the presence of singularities in the space can also pose challenges in solving these paths.

How does solving radially-directed geodesics in AdS space contribute to our understanding of the universe?

Studying radially-directed geodesics in AdS space allows us to gain insights into the fundamental laws of physics, such as the behavior of particles in curved space and the effects of gravity. This knowledge can then be applied to better understand the nature of the universe and its evolution.

Back
Top