Centrifugal Acceleration GR: Formula for .8c, 1m Radius

In summary, the proper acceleration of a Langevin observer, or an accelerometer swung around the head with a constant relative speed of v and a radius of r, can be calculated using the formula a = \frac{- v^2}{r \left( 1 - v^2 \right)}, as derived from the Wikipedia page on Born coordinates. This formula takes into account highly relativistic effects, with an extra factor of \gamma^2.
  • #1
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I swing an accelerometer around my head with a constant relative speed of v and a radius of r. I want the exact formula with highly relativistic effects, so v = .8 c and r = 1 meter, say. What proper acceleration will the accelerometer read?
 
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  • #2
Take a look at the Wikipedia page on Born coordinates:

http://en.wikipedia.org/wiki/Born_coordinates

They give a formula for the proper acceleration of a "Langevin observer", which corresponds to the accelerometer being swung around your head. They give it in terms of the angular velocity [itex]\omega[/itex], but using the formula [itex]v = \omega r[/itex], it is easy to come up with a formula in terms of the velocity [itex]v[/itex]:

[tex]a = \frac{- v^2}{r \left( 1 - v^2 \right)}[/tex]

This makes sense; it's just the standard Newtonian formula for centripetal acceleration, with an extra relativistic factor of [itex]\gamma^2[/itex].
 
  • #3
Thank you PeterDonis.
 

1. What is the formula for calculating Centrifugal Acceleration GR at .8c with a radius of 1 meter?

The formula for calculating Centrifugal Acceleration in General Relativity at a speed of .8c with a radius of 1 meter is a = (v^2)/r, where a is the acceleration, v is the velocity, and r is the radius.

2. How is Centrifugal Acceleration GR different from regular Centrifugal Acceleration?

Centrifugal Acceleration in General Relativity (GR) takes into account the effects of gravity and the curvature of spacetime, while regular Centrifugal Acceleration only considers the effects of rotation. This means that Centrifugal Acceleration GR can be calculated in a curved spacetime, while regular Centrifugal Acceleration is calculated in a flat space.

3. What is the significance of using .8c as the speed in the formula for Centrifugal Acceleration GR?

The speed of .8c is significant because it represents a high velocity that is close to the speed of light. This allows us to observe the effects of Centrifugal Acceleration GR on objects moving at extremely high speeds.

4. Can the formula for Centrifugal Acceleration GR be used for any radius or speed?

Yes, the formula for Centrifugal Acceleration GR can be used for any radius or speed, as long as the speed is less than the speed of light. However, for larger radii and slower speeds, the effects of Centrifugal Acceleration GR may be negligible.

5. How does Centrifugal Acceleration GR impact our understanding of gravity and spacetime?

Centrifugal Acceleration GR is an important concept in the theory of General Relativity, as it helps us understand the effects of gravity on objects in motion. It also highlights the connection between gravity and the curvature of spacetime, providing a deeper understanding of the nature of our universe.

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