Derive Escape Velocity GR: Source for Schwarzschild Metric

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SUMMARY

The formula for escape velocity in the context of General Relativity (GR) for a spherical mass, such as Earth, is expressed as v_e = (2GM/r)^{1/2}, which aligns with classical physics. To derive this, one must analyze a radial geodesic starting from rest at infinity using the Schwarzschild metric. Key resources for this derivation include Carroll's lecture notes and the Wikipedia page on Schwarzschild geodesics. It is crucial to note that while the escape velocity formula appears similar to the Newtonian result, it differs by a factor of (1 - r_{s}/r), where r_{s} is the Schwarzschild radius.

PREREQUISITES
  • Understanding of General Relativity concepts, particularly the Schwarzschild metric
  • Familiarity with geodesic equations in GR
  • Basic knowledge of escape velocity and its derivation
  • Ability to manipulate equations involving energy and angular momentum in a relativistic context
NEXT STEPS
  • Study the derivation of escape velocity using the Schwarzschild metric from Carroll's lecture notes
  • Explore the Wikipedia page on Schwarzschild geodesics for additional insights
  • Investigate the implications of the factor (1 - r_{s}/r) on escape velocity
  • Review homework problems related to escape velocity in various GR textbooks
USEFUL FOR

Students and researchers in physics, particularly those focusing on General Relativity, astrophysics, and gravitational physics, will benefit from this discussion.

snoopies622
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TL;DR
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:
<br /> v_e = (2GM/r)^{1/2}<br />
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 (1 - r_{s}/r).

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

<br /> \frac {dr}{dT} = E^2/m^2 c^2 - (1 - r_{s}/r)(c^2 + h^2 / r^2)<br />

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

with (1 - r_{s}/r) = (dt/dT) (E/mc^2)
 
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 (1 - r_{s}/r).
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

<br /> \frac {dr}{dT} = E^2/m^2 c^2 - (1 - r_{s}/r)(c^2 + h^2 / r^2)<br />

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

with (1 - r_{s}/r) = (dt/dT) (E/mc^2)
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!
 

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