Gravitational Attraction of a Massive Particle

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SUMMARY

The discussion centers on the gravitational attraction of massive particles, specifically protons traveling at near light speed. It highlights that college-level algebra and calculus are insufficient to grasp the equations of General Relativity (GR), which relies on differential geometry and tensor calculus. The Aichelburg-Sexl solution is mentioned as a way to understand the tidal gravitational field of a moving particle, resembling a plane wave. For further learning, Prof. Susskind's free lecture series on GR is recommended.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with differential geometry
  • Knowledge of tensor calculus
  • Basic concepts of gravitational fields and tidal forces
NEXT STEPS
  • Watch Prof. Susskind's lecture series on General Relativity
  • Study differential geometry in the context of physics
  • Learn about tensor calculus applications in GR
  • Research the Aichelburg-Sexl solution and its implications
USEFUL FOR

Students and professionals in physics, particularly those interested in advanced concepts of General Relativity and gravitational interactions at relativistic speeds.

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I was wondering what equations govern calculating the gravitation attraction of a massive particle (say a proton) traveling at near light speed? Thanks!
 
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What is your current level of understanding of physics and mathematics?
 
Lets go with college level Algebra, but I've taken college level Calculus, just don't remember most of it.
 
Okay. Just to be precise, we don't know how the gravitational field looks around single particles because we don't have a working quantum theory of gravity yet. We can say quite a bit about more massive objects though.

Unfortunately, college undergraduate level algebra and calculus is insufficient in order to understand the equations of GR, the matematical framework for which is differential geometry and tensor calculus. As such, giving you the equations immediately would be meaningless. I suggest you take a look at Prof. Susskind's video lecture series on GR, which is available fo free on youtube;

Here is the link to the Special Relativity lecture series:
General relativity lecture series:
 
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Because all objects are affected by gravity, we can't actually measure a "gravitational field" in the same sense that we can measure , say, an electric field. In some specialized circumstances we can work around this lack of a reference particle that would be "unaffected by gravity", but the case of a moving mass isn't one of those special circumstances.

What we could measure, in principle, is the tidal gravitational field of a moving particle - the accelerations induced in nearby test particles relative to each other. Unfortunately, the detailed presentation on it gets rather technical. It's known as the Aichelburg - Sexyl solution, and in general terms, it looks like a plane wave, similar to the electromagnetic case, which behaves in a similar manner.
 

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