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boniphacy
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- TL;DR Summary
- accel on a quasar
I want to derive an acceleration in the case for a stationary mass in the gravity field.
I found the total energy in the GR is provided by a simple equation:
https://en.wikipedia.org/wiki/Schwarzschild_geodesics
## E = mc^2\sqrt{1 - rs/r} * \gamma ##
So, this is easy to provide acceleration for that energy definition, using standard math alone: the gradient.
## g(r) = -GM/r^2 \frac{1}{1 - rs/r} ##
And this should be correct (for a stationary body: v = 0).
I have seen many complicated solutions for this problem, and inconsistent with this result.
What is a problem with this?
I found the total energy in the GR is provided by a simple equation:
https://en.wikipedia.org/wiki/Schwarzschild_geodesics
## E = mc^2\sqrt{1 - rs/r} * \gamma ##
So, this is easy to provide acceleration for that energy definition, using standard math alone: the gradient.
## g(r) = -GM/r^2 \frac{1}{1 - rs/r} ##
And this should be correct (for a stationary body: v = 0).
I have seen many complicated solutions for this problem, and inconsistent with this result.
What is a problem with this?
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