Gravitational Constant in GR: How & Why?

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SUMMARY

The gravitational constant, denoted as G, is utilized in both classical gravitation and General Relativity (GR) due to its role as a universal conversion factor between different units. This consistency allows GR to reduce to Newtonian gravity under specific conditions, such as slow-moving test particles in weak gravitational fields. The constant was originally determined by Henry Cavendish for classical gravitation, and its application in GR is essential for maintaining the continuity of gravitational theory. Thus, there was no need to measure a new constant for GR.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with Newtonian gravity principles
  • Knowledge of the gravitational constant (G)
  • Basic grasp of unit conversion in physics
NEXT STEPS
  • Study the derivation of Einstein's field equations in General Relativity
  • Explore the implications of G in various gravitational scenarios
  • Investigate the historical context of Cavendish's experiments
  • Learn about the limits of Newtonian gravity and its transition to GR
USEFUL FOR

Students of physics, researchers in gravitational theory, and anyone interested in the foundational concepts of General Relativity and its relationship with classical gravitation.

Zak
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(precursor: I have not formally studied GR)

I have noticed that the gravitational constant found in classical gravitation is also used in GR. Why is this the case? Am I correct in thinking that the constant was determined by Cavendish and was for the classical theory of gravitation? So, my question: how do we know that the same gravitational constant is suitable for GR and why did we not have to, say, measure a new constant?
 
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Zak said:
(precursor: I have not formally studied GR)

I have noticed that the gravitational constant found in classical gravitation is also used in GR. Why is this the case? Am I correct in thinking that the constant was determined by Cavendish and was for the classical theory of gravitation? So, my question: how do we know that the same gravitational constant is suitable for GR and why did we not have to, say, measure a new constant?

We get ##G## into the Einstein equations by requiring that they reduce to the classical gravitation law in the limit of slow (test-)particles in low gravitational fields.

Essentially the reason is that we want GR to supersede Newtonian gravity.
 
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Zak said:
I have noticed that the gravitational constant found in classical gravitation is also used in GR. Why is this the case?
As JorisL mentioned, you can look at is as a requirement so that GR can reduce to Newtonian gravity in the appropriate limit.

Another way to look at it is that G is just a universal conversion factor between different units, so any time that you will convert between the same units you will get a the same conversion factor.
 
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Zak said:
I have noticed that the gravitational constant found in classical gravitation is also used in GR. Why is this the case?
You can think of it in terms of reducing to Newtonian gravitation in the appropriate limit. You can also look at it as a conversion factor between different units. So then it is the same in both theories as long as you use the same units.
 

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