Rindler coordinates in Minkowski spacetime

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SUMMARY

Rindler coordinates in two-dimensional Minkowski spacetime are defined by the metric $$(ds)^{2} = - R^{2}(d\eta)^{2} + (dR)^{2}$$ for accelerating observers, contrasting with inertial coordinates represented by $$(ds)^{2} = - (dt)^{2} + (dx)^{2}$$. The transformation between these coordinate systems is given by $$x = R\cosh\eta$$ and $$t = R\sinh\eta$$. Rindler observers, who maintain a fixed R, experience constant acceleration, while inertial observers at fixed x do not follow a geodesic. The discussion also addresses the limitations of Rindler coordinates, which only cover the right wedge of Minkowski space, and the implications for communication between Minkowski and Rindler observers.

PREREQUISITES
  • Understanding of Minkowski spacetime
  • Familiarity with coordinate transformations in physics
  • Knowledge of geodesics and acceleration in relativity
  • Basic concepts of horizons in spacetime
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  • Study the implications of proper acceleration in Rindler coordinates
  • Explore the concept of horizons in general relativity
  • Investigate the relationship between Rindler observers and black hole physics
  • Learn about the communication limits between different observer frames in relativity
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Physicists, students of relativity, and anyone interested in the geometrical interpretation of spacetime and acceleration in Minkowski space.

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In an inertial coordinate system in two-dimensional Minkowski spacetime, the metric takes the form
$$(ds)^{2} = - (dt)^{2} + (dx)^{2},$$
and in an accelerating coordinate system in two-dimensional Minkowski spacetime, the metric takes the form
$$(ds)^{2} = - R^{2}(d\eta)^{2} + (dR)^{2}.$$
The coordinates ##t## and ##x## are called inertial coordinates and the coordinates ##\eta## and ##R## are called Rindler coordinates.

These coordinates describe the line element of Minkowski spacetime from the perspective of an inertial observer and of an accelerating observer respectively.
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Rindler coordinates in Minkowski spacetime are related to inertial coordinates in Minkowski spacetime by the change of coordinates
$$x = R\cosh\eta, \qquad t = R\sinh\eta.$$
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An inertial observer is an observer sitting at fixed ##x##. This is not a geodesic - it is a stationary trajectory.

A Rindler observer is an observer sitting at fixed ##R##. This is not a geodesic - it is a uniformly accelerating trajectory.
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1. How can you prove that an observer sitting at fixed ##R## has a fixed acceleration?

2. How can you prove that the Rindler coordinates only cover the right wedge of Minkowski space? Why don't Rindler coordinates cover the other three patches of Minkowski space?

3. Can a Minkowski observer ever communicate with a Rindler observer?

4. Why do Rindler observers see a horizon at ##R = 0##? How is this horizon similar to a black hole horizon?
 
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Did you try to map curves of constant-##R## or constant-##\eta## into an ordinary spacetime diagram?
Given the trajectory of a particle, can you determine the velocity and acceleration?
 
spaghetti3451 said:
An inertial observer is an observer sitting at fixed ##x##. This is not a geodesic - it is a stationary trajectory.
Are you sure of this?
 
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spaghetti3451 said:
. How can you prove that an observer sitting at fixed R has a fixed acceleration?
Just calculate the proper acceleration and show that it is constant wrt time.

spaghetti3451 said:
3. Can a Minkowski observer ever communicate with a Rindler observer?
If you and a friend are in an elevator and one of you jumps do you expect an interruption in communication?
 
Last edited:
An inertial observer is an observer sitting at fixed ##x##. This is not a geodesic - it is a stationary trajectory.

Huh? An observer in an inertial frame with a constant velocity (including a constant velocity of zero) is following a geodesic.
 
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