Lemaitre Coordinates: Plotting Freefall & Light Paths

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The discussion focuses on a diagram illustrating two free-falling observers in Lemaitre coordinates, highlighting the central singularity and the paths of light. It notes that while the distance between observers remains constant in Lemaitre spatial coordinates, the radar distance increases in Lemaitre time coordinates. The diagram also reveals that, far from the gravitational source, the speed of light in Lemaitre coordinates approaches infinity rather than the speed of light (c). Additionally, a derived equation for a null, radial trajectory is presented, although its physical significance is questioned. Overall, the conversation emphasizes the complexities of plotting and understanding Lemaitre coordinates in the context of general relativity.
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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.
 
In an inertial frame of reference (IFR), there are two fixed points, A and B, which share an entangled state $$ \frac{1}{\sqrt{2}}(|0>_A|1>_B+|1>_A|0>_B) $$ At point A, a measurement is made. The state then collapses to $$ |a>_A|b>_B, \{a,b\}=\{0,1\} $$ We assume that A has the state ##|a>_A## and B has ##|b>_B## simultaneously, i.e., when their synchronized clocks both read time T However, in other inertial frames, due to the relativity of simultaneity, the moment when B has ##|b>_B##...

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