How to calculate the four-momentum of a photon in FRW Metric

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SUMMARY

The discussion focuses on calculating the four-momentum of a photon in the Friedmann-Robertson-Walker (FRW) metric using both the geodesic equation and Lagrangian mechanics. The Lagrangian is defined as L = g_{ij} (dx^i/d\lambda)(dx^j/d\lambda) = -\dot{t}^2 + a^2(t)(\dot{r}^2 + r^2 \dot{\theta}^2 + r^2 \sin^2\theta \dot{\phi}^2). The four-momentum components are derived from the Lagrangian using p_i = ∂L/∂\dot{x}_i, with simplifications based on the isotropic nature of the metric. The discussion also emphasizes that the geodesic equation yields the same results for the time component of momentum.

PREREQUISITES
  • Understanding of the Friedmann-Robertson-Walker (FRW) metric
  • Familiarity with Lagrangian mechanics
  • Knowledge of geodesic equations in general relativity
  • Basic calculus, particularly partial derivatives
NEXT STEPS
  • Study the derivation of the geodesic equation in the context of general relativity
  • Learn about the application of Lagrangian mechanics in relativistic physics
  • Explore isotropic metrics and their implications in cosmology
  • Investigate the role of Christoffel symbols in calculating geodesics
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Students and researchers in theoretical physics, particularly those focusing on general relativity and cosmology, will benefit from this discussion. It is especially relevant for those studying the dynamics of photons in curved spacetime.

JohnH123
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Homework Statement
Find the 4-momentum of a photon moving in the x-direction. That is, find dt/dλ
and dx/dλ as functions of a. Note that dt/dλ at a = 1 is the present-day frequency f0.
Relevant Equations
The spatially flat Robertson-Walker Metric: ds^2 = -dt^2 + a^2(t)[dr^2+r^2(dtheta^2 + sin^2(theta)dphi^2)]
I have calculated the Christoffel symbols for the above given metric, but I don't understand how to calculate a photon's four-momentum using this information. I believe it has something to do with the null geodesic equation but I can't understand how to put that information into the problem. Thank you.
 
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This problem can be done using geodesic equation of motion. But there is a simpler way to do using Lagrangian mechanics. The Lagrangian of the given metric is:
##L= g_{ij}\frac{dx^i}{d\lambda}\frac{dx^j}{d\lambda}= -\dot t^2+ a^2(t)(\dot r^2+ r^2 \dot \theta^2+ r^2 \sin^2\theta \dot \phi^2) ##

Now, the momentum is :
##p_i=\frac{\partial L}{\partial \dot x_i}##
Now, simplify it for example using the fact that metric is isotropic to evaluate ##r_{th}## component of momentum. For ##t## component, you will get same result as geodesic equation. Solve it (again using the fact that metric is isotropic to remove ##\theta## and ##\phi## components from metric).
 
Abhishek11235 said:
This problem can be done using geodesic equation of motion. But there is a simpler way to do using Lagrangian mechanics. The Lagrangian of the given metric is:
##L= g_{ij}\frac{dx^i}{d\lambda}\frac{dx^j}{d\lambda}= -\dot t^2+ a^2(t)(\dot r^2+ r^2 \dot \theta^2+ r^2 \sin^2\theta \dot \phi^2) ##

Now, the momentum is :
##p_i=\frac{\partial L}{\partial \dot x_i}##
Now, simplify it for example using the fact that metric is isotropic to evaluate ##r_{th}## component of momentum. For ##t## component, you will get same result as geodesic equation. Solve it (again using the fact that metric is isotropic to remove ##\theta## and ##\phi## components from metric).
Just so I’m clear, ##\frac{\partial L}{\partial \dot x_i}## means the partial of the lagrangian with respect to each coordinate right? So the four momentum has components in coordinates {t, r, ##\theta##, ##\phi##}, so those components are found by finding ##\frac{\partial L}{\partial \dot t}##, ##\frac{\partial L}{\partial \dot r}## and so on, correct?
 
Abhishek11235 said:
This problem can be done using geodesic equation of motion. But there is a simpler way to do using Lagrangian mechanics. The Lagrangian of the given metric is:
##L= g_{ij}\frac{dx^i}{d\lambda}\frac{dx^j}{d\lambda}= -\dot t^2+ a^2(t)(\dot r^2+ r^2 \dot \theta^2+ r^2 \sin^2\theta \dot \phi^2) ##

Now, the momentum is :
##p_i=\frac{\partial L}{\partial \dot x_i}##
Now, simplify it for example using the fact that metric is isotropic to evaluate ##r_{th}## component of momentum. For ##t## component, you will get same result as geodesic equation. Solve it (again using the fact that metric is isotropic to remove ##\theta## and ##\phi## components from metric).
Also, could you please expand on how I could calculate the four-momentum using the geodesic equation? I believe that’s the method my professor would like me to use, as stated in the problem. Thank you.
 

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