Gravitational deviation of matter travelling near c by a massive body

In summary: No, because the source term of gravity is not relativistic mass, but the stress-energy-momentum tensor. Since this is a fully covariant tensorial quantity, it is invariant under Lorentz transformations, so merely putting an object into relative motion at a very high velocity does not somehow give it a huge gravitational influence.
  • #1
adrian_m
38
1
Light traveling transverse to a massive body (e.g. Sun) is deviated by an angle twice the amount predicted by Newtonian gravitational theory. This is predicted by GR and proven experimentally.

What would be the deviation of a matter particle traveling near c transverse to a massive body? Would it also be deviated by an angle nearly twice the amount predicted by Newtonian theory? Or would it much more because its relativistic mass/energy would make its gravitational mass very large? Or would it be deviated by the Newtonian amount?
 
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  • #2
adrian_m said:
Light traveling transverse to a massive body (e.g. Sun) is deviated by an angle twice the amount predicted by Newtonian gravitational theory. This is predicted by GR and proven experimentally.
Yes, because of the spatial geometry:
http://mathpages.com/rr/s8-09/8-09.htm


adrian_m said:
What would be the deviation of a matter particle traveling near c transverse to a massive body? Would it also be deviated by an angle nearly twice the amount predicted by Newtonian theory?
For nearly c, you get nearly twice the Newtonian deflection. In the limit v << c the deflection tends towards the Newtonian value. That's why we can use Newtonian gravitational theory for most stuff.
 
  • #3
A.T. said:
Yes, because of the spatial geometry:
http://mathpages.com/rr/s8-09/8-09.htm

Agreed.

A.T. said:
For nearly c, you get nearly twice the Newtonian deflection. In the limit v << c the deflection tends towards the Newtonian value. That's why we can use Newtonian gravitational theory for most stuff.

This is the part that was bothering me. The relativistic mass of the particle traveling near c should be very large. Does that not increase its gravitational mass exponentially? If it does, then why does it not increase GMm/R^2 proportionately? I am extrapolating from the understanding that the mass increase does take place and increases the gravitational acceleration between the two bodies, as seen in the extra gravitational acceleration between the Sun and Mercury that causes Mercury's orbit to precess. I realize this is a somewhat Newtonian interpretation, but does GMm/R^2 X (relativistic corrections) totally fail here?
 
  • #4
adrian_m said:
I am extrapolating from the understanding that the mass increase does take place and increases the gravitational acceleration between the two bodies, as seen in the extra gravitational acceleration between the Sun and Mercury that causes Mercury's orbit to precess.
I don't think this is a correct understanding. The orbit procession can be explained in the same way as the doubling of the light deflection, by spatial geometry. See the bottom picture here:

http://www.physics.ucla.edu/demoweb..._and_general_relativity/curved_spacetime.html
 
  • #5
adrian_m said:
The relativistic mass of the particle traveling near c should be very large. Does that not increase its gravitational mass exponentially?

No, because the source term of gravity is not relativistic mass, but the stress-energy-momentum tensor. Since this is a fully covariant tensorial quantity, it is invariant under Lorentz transformations, so merely putting an object into relative motion at a very high velocity does not somehow give it a huge gravitational influence.
 
  • #6
adrian_m said:
This is the part that was bothering me. The relativistic mass of the particle traveling near c should be very large. Does that not increase its gravitational mass exponentially? If it does, then why does it not increase GMm/R^2 proportionately? I am extrapolating from the understanding that the mass increase does take place and increases the gravitational acceleration between the two bodies, as seen in the extra gravitational acceleration between the Sun and Mercury that causes Mercury's orbit to precess. I realize this is a somewhat Newtonian interpretation, but does GMm/R^2 X (relativistic corrections) totally fail here?



gravitational force = GMm/R^2

gravitational acceleration = gravitational force / m = GM/R^2


In an accelerating rocket drop a marble and fire a laser gun horizontally at the same time. After a while check where the marble and the laser pulse are. They will be at the same altitude, and they will have the same downwards velocity.

On the surface of the Earth drop a marble and fire a laser gun horizontally at the same time. After a very short time check where the marble and the laser pulse are. They will be at the same altitude, and they will have the same downwards velocity.

A hammer, a feather, a photon, a relativistic feather, a relativistic hammer, all accelerate downwards the same way.
 
  • #7
jartsa said:
A hammer, a feather, a photon, a relativistic feather, a relativistic hammer, all accelerate downwards the same way.
He is asking about the total deflection angle, which depends on the speed. So it's not the same for a photon, as for a massive object at less than c. Neither in Newtons theory nor in GR.
 
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  • #10
Thanks for all the answers. Checked out all the references also and they are good.

The confirmation I got is that the deviation would be nearly twice the Newtonian value. This is what I suspected would be the case though some other notions were bothering me by throwing up (mistakenly) other possibilities.

Essentially, we can say that for a transverse velocity [itex]v[/itex], the effective acceleration will be the Newtonian acceleration multiplied by a factor of [itex](1+v^2/c^2)[/itex]. Some of the references in this thread also seem to indicate this, and it is consistent with the known deviation of light as well.
 

1. What is gravitational deviation of matter travelling near c by a massive body?

The gravitational deviation of matter travelling near the speed of light (c) by a massive body refers to the phenomenon in which the path of an object is altered due to the gravitational force exerted by a massive body. This is a result of Einstein's theory of general relativity, which states that the presence of a massive body causes a curvature in the fabric of spacetime.

2. How does the mass of the body affect gravitational deviation?

The mass of the body directly affects the strength of its gravitational force. The greater the mass of the body, the stronger its gravitational pull, and the more significant the deviation of matter travelling near c will be.

3. Can light be affected by gravitational deviation?

Yes, light is also affected by gravitational deviation. This was first observed during a solar eclipse in 1919, when the position of stars behind the sun appeared to shift due to the sun's massive gravitational pull.

4. Is gravitational deviation the same as gravitational lensing?

No, gravitational deviation and gravitational lensing are two different phenomena. Gravitational deviation refers to the alteration of an object's path, while gravitational lensing refers to the bending of light by a massive body, resulting in a distorted image of the object behind it.

5. Is gravitational deviation only observed near massive bodies?

No, gravitational deviation can also be observed near objects with smaller masses. However, the effect is more significant near massive bodies due to their stronger gravitational pull.

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