Lemaitre Coordinates: Plotting Freefall & Light Paths

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The discussion focuses on the plotting of free-falling observers in Lemaitre coordinates, highlighting the relationship between spatial and time coordinates in the context of gravitational effects. The diagram illustrates the central singularity, ingoing light paths, and outgoing light rays, while also comparing Lemaitre coordinates to Schwarzschild coordinates. A key observation is that the radar distance between observers increases in Lemaitre time, despite constant spatial separation. Additionally, it is noted that the speed of light in Lemaitre coordinates approaches infinity rather than the speed of light (c) as one moves away from the gravitational source.

PREREQUISITES
  • Understanding of Lemaitre coordinates and their application in general relativity
  • Familiarity with Schwarzschild coordinates and their significance in gravitational contexts
  • Basic knowledge of light propagation in curved spacetime
  • Proficiency in interpreting mathematical equations related to general relativity
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  • Study the Lemaitre metric and its implications for free-fall dynamics
  • Explore the mathematical derivation of light paths in curved spacetime
  • Investigate the relationship between radar distance and proper time in general relativity
  • Learn about the physical significance of null trajectories in gravitational fields
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Physicists, astrophysicists, and students of general relativity who are interested in the dynamics of free-falling observers and the behavior of light in curved spacetime.

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The attached diagram is a plot of two free falling observers (vertical black lines) in Lemaitre coordinates. http://en.wikipedia.org/wiki/Lemaitre_metric

The solid black diagonal line is the central singularity. Curved blue lines are ingoing light paths and curved red lines are outgoing light rays. The diagonal dashed grey lines are lines of constant radius in Schwarzschild coordinates.

The Wiki article gives some information on the Lemaitre metric but some additional information and calculations are need to obtain the equations in a form that can be plotted on a graph.

A curious feature highlighted by the diagram is that despite the distance between the two free falling observers being constant in terms of Lemaitre spatial coordinates, the radar distance is increasing in terms of the Lemaitre time coordinate which I assume is just the proper time of a falling observer. It is also clear from the diagram that far away from the gravitational source where spacetime becomes flat, the speed of light in Lemaitre coordinates does not tend towards c, but tends towards infinite.
 

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yuiop said:
It is also clear from the diagram that far away from the gravitational source where spacetime becomes flat, the speed of light in Lemaitre coordinates does not tend towards c, but tends towards infinite.

It also follows from the metric, which gives for a null, radial trajectory

<br /> \frac{d\rho}{d\tau}=\sqrt{\frac{r}{r_g}}<br /> [/itex]<br /> <br /> I don&#039;t think it has physical significance.
 
Mentz114 said:
It also follows from the metric, which gives for a null, radial trajectory

<br /> \frac{d\rho}{d\tau}=\sqrt{\frac{r}{r_g}}<br />

I don't think it has physical significance.

Came across this old thread while poking around the internet (it's high on Google's results for "Lemaitre coordinates"), figured I'd fix the formatting for the next person to come along.
 

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