Derive Escape Velocity GR: Source for Schwarzschild Metric

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snoopies622
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Wondering how to find the escape velocity formula consistent with relativity.
I was surprised to read that the formula for escape velocity — at least for a spherical mass like the Earth — is the same in relativity as it is in classical physics:
[tex] v_e = (2GM/r)^{1/2}[/tex]
I'm wondering if someone can give me a good source for deriving this. (I assume one takes a radial geodesic starting at rest from infinity using the Schwarzschild metric and finding its velocity at radius r?) Thanks.
 
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snoopies622 said:
I'm wondering if someone can give me a good source for deriving this.

Many GR textbooks give this as a homework problem.

snoopies622 said:
(I assume one takes a radial geodesic starting at rest from infinity using the Schwarzschild metric and finding its velocity at radius r?)

Yes.
 
Thanks Peter, actually I was hoping for a link to something on the internet since my college physics library is still semi-closed due to the Covid-19.
 
Carroll's lecture notes, around equations 7.43 to 7.48 for the geodesic equation. Read back a bit for definitions of ##E##, ##L##, ##\epsilon##.
 
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Epilogue:

I had forgotten about this, but using a couple equations found here

https://en.wikipedia.org/wiki/Schwarzschild_geodesics

and substituting, I get that the escape velocity isn't exactly the same as the Newtonian result (see OP) but differs by a factor [itex](1 - r_{s}/r)[/itex].

All I did was find E by setting dr/dT = 0, h (angular momentum) =0 and r=infinity in the given

[tex] \frac {dr}{dT} = E^2/m^2 c^2 - (1 - r_{s}/r)(c^2 + h^2 / r^2)[/tex]

and then let [itex]v^2 = (dr/dT)^2 / (dt/dT)^2[/itex]

with [itex](1 - r_{s}/r) = (dt/dT) (E/mc^2)[/itex]
 
snoopies622 said:
using a couple equations found here

https://en.wikipedia.org/wiki/Schwarzschild_geodesics

and substituting, I get that the escape velocity isn't exactly the same as the Newtonian result (see OP) but differs by a factor [itex](1 - r_{s}/r)[/itex].
This is not correct. The formula in your OP is correct.

snoopies622 said:
All I did was find E by setting dr/dT = 0, h (angular momentum) =0 and r=infinity in the given

[tex] \frac {dr}{dT} = E^2/m^2 c^2 - (1 - r_{s}/r)(c^2 + h^2 / r^2)[/tex]

and then let [itex]v^2 = (dr/dT)^2 / (dt/dT)^2[/itex]

with [itex](1 - r_{s}/r) = (dt/dT) (E/mc^2)[/itex]
That doesn't give you escape velocity. Escape velocity is just ##dr / dT##. What you are calculating here, ##dr / dt##, is just a coordinate velocity and has no direct physical meaning.
 
Thanks Peter, I'm relieved to hear this since i just noticed that my dr/dt formula gives an escape velocity of zero at the surface of a Schwarzschild black hole!