Gravitational Velocity of Mass ##M## at Distance ##d## from Gravitating Body

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Discussion Overview

The discussion revolves around the gravitational velocity of a mass ##M## at a distance ##d## from a gravitating body, exploring the implications of special relativity (SR) and general relativity (GR) on this topic. Participants analyze equations derived from Newton's laws and their application to gravitational scenarios, particularly near the Schwarzschild radius.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant presents a derivation of velocity as a function of distance from a gravitating body, leading to concerns about the behavior of the function at the Schwarzschild radius.
  • Another participant questions the validity of hovering at the Schwarzschild radius, suggesting that it is not possible.
  • Some participants express confusion over the mathematical formulation, particularly regarding the signs in the gravitational force equation.
  • A later reply indicates that the computations may yield physically meaningless results when applied to gravity, as gravity is not modeled as a force in relativity.
  • There is mention of a plot showing the velocity of a mass starting from rest at infinity, with discussions on whether it can exceed the speed of light under special relativity.
  • Some participants argue that the discussion may be more appropriate for GR rather than SR, as SR cannot adequately model gravitational effects.
  • One participant suggests that the classical prediction of velocity could lead to scenarios where it exceeds the speed of light, raising further questions about the implications of their calculations.

Areas of Agreement / Disagreement

Participants express differing views on the applicability of special relativity to gravitational scenarios, with some asserting that it cannot be used to model gravity, while others attempt to derive results using SR. The discussion remains unresolved regarding the validity of the mathematical approaches and the physical interpretations of the results.

Contextual Notes

There are limitations in the assumptions made regarding the gravitational force and the conditions under which the equations are applied, particularly near the Schwarzschild radius. The discussion also highlights the potential for confusion in notation and the implications of using SR versus GR.

ChrisVer
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Starting from a locked thread I tried to work the gravity of a body of mass ##M## on another body starting from infinity to some distance ##d## from the gravitating body.
We have from the SR 2nd Newton law that:
[itex]\gamma^3 a = \frac{GM}{r^2}[/itex]

writting [itex]a= \frac{dv}{dt}= v \frac{dv}{dr} = \frac{1}{2} \frac{dv^2}{dr}[/itex]

Naming [itex]v^2/c^2= x[/itex] the above relation becomes:

[itex]\frac{dx}{(1-x)^{3/2}}= \frac{2GM}{c^2 r^2}dr[/itex]

Integrating:

[itex]\int_{0}^{x_d}\frac{dx}{(1-x)^{3/2}}= \int_{\infty}^{d} \frac{2GM}{c^2 r^2}dr[/itex]
[itex]\frac{2}{\sqrt{1-x_d}}-2= - \frac{2GM}{c^2 d}[/itex]

[itex]x_d=1- \Big( 1- \frac{GM}{c^2 d}\Big)^{-2}[/itex]

And so:

[itex]v(d)= c \bigg[ 1- \Big( 1- \frac{GM}{c^2 d}\Big)^{-2} \bigg]^{1/2}[/itex]

I tried plotting this solution as [itex]v(d)[/itex], the good part is that [itex]v<c[/itex] for all distances however I don't understand why for [itex]d=GM/c^2[/itex] I'm obtaining an infinity (and worse- in the imaginary regime)? By the way, that's the Schwarzschild radius...

Even worse, if I set [itex]\frac{GM}{c^2}=1[/itex] the plot of [itex]\beta = v/c = \bigg[ 1- \Big( 1- \frac{1}{d}\Big)^{-2} \bigg]^{1/2}[/itex] is given in my attachment...and doesn't seem to have a real solution away from 1?
 

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ChrisVer said:
I tried plotting this solution as v(d), the good part is that v<c for all distances however I don't understand why for d=GM/c2 I'm obtaining an infinity
Are you trying to compute the falling speed relative to a local hovering observer? You cannot have one hovering at the Schwarzschild radius.
 
A.T. said:
. You cannot have one hovering at the Schwarzschild radius.

So the information of Schwarzschild radius singularity is contained within SR? I solved the problem in a mechanical way...
But the main problem is that for larger radii from the source (distances ##d>R_s##), I am not getting a real solution for ##v##...
 
ChrisVer said:
Starting from a locked thread I tried to work the gravity of a body of mass ##M## on another body starting from infinity to some distance ##d## from the gravitating body.
We have from the SR 2nd Newton law that:
[itex]\gamma^3 a = \frac{GM}{r^2}[/itex]

writting [itex]a= \frac{dv}{dt}= v \frac{dv}{dr} = \frac{1}{2} \frac{dv^2}{dr}[/itex]

Naming [itex]v^2/c^2= x[/itex] the above relation becomes:
..
..

Typo here maybe

##\frac{1}{2} \frac{dv^2}{dr}##
 
Eh?
[itex]\frac{1}{2} \frac{dv^2}{dr}= \frac{1}{2} \big( \frac{dv}{dr} v + v \frac{dv}{dr}\big) = v \frac{dv}{dr}= \frac{dr}{dt} \frac{dv}{dr} = \frac{dv}{dt}=a[/itex]
 
That looks like a GR conversation..:sorry:
 
ChrisVer said:
That looks like a GR conversation..
Yes, for comparison of g under GR with the value you assume based on SR and Newton.
 
I think this is a mistake with the gravitational force I used...I think I should have used a minus sign: [itex]\gamma^3 a = - GM/r^2[/itex]...
The main problem is that, as it is, there is no solution for [itex]d > R_s[/itex] ([itex]v^2<0[/itex]) and this makes physically no sense, since the force I used could as well be some other [itex]1/r^2[/itex] type force (like electromagnetism), with the change [itex]R_s \rightarrow D=\frac{k q_1 q_2}{c^2 m}[/itex].
 
  • #10
The result for [itex]v[/itex] is then:

[itex]v= c \sqrt{1- (1+\frac{GM}{c^2 d} )^{-2}}[/itex]
With a plot (for [itex]R_s= \frac{GM}{c^2}=1[/itex]) like the attached, which makes "sense".
 

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  • #11
ChrisVer said:
Eh?
[itex]\frac{1}{2} \frac{dv^2}{dr}= \frac{1}{2} \big( \frac{dv}{dr} v + v \frac{dv}{dr}\big) = v \frac{dv}{dr}= \frac{dr}{dt} \frac{dv}{dr} = \frac{dv}{dt}=a[/itex]
Oh, you mean ##\frac{d}{dr}v^2##. Your notation confused me.

What is the plot of in your latest post ?
 
  • #12
Mentz114 said:
What is the plot of in your latest post ?

It is let's say [itex]\frac{v}{c} = \beta(r)[/itex]... it shows the change of the velocity of a mass that began from infinity with 0 velocity under the "Newtonian" gravitational law of a point-like mass source [itex]M[/itex] (in terms of "schwarzchild radii" of the source body- of course it should not be confused with schwarzchild radii since I don't work in GR). So for example, when the body is at a distance [itex]x=2 \times \frac{GM}{c^2}[/itex] away from the source, it will have a velocity [itex]v \approx 0.75c[/itex]...
In a closed thread someone said that the velocity of the object would eventually reach a value larger than [itex]c[/itex] due to acceleration. I just wanted to counter this idea via special relativity alone...

I guess this could change for GR, but OK... It was more like a special relativistic application of [itex]F= \frac{dp}{dt}[/itex]. Showing that by applying special relativity alone, it doesn't matter for how long your body has traveled (starting from infinity up to reaching the source at 0), its velocity won't exceed the speed of light.
 
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  • #13
It saves the "classical"/non-relativistic prediction that:
[itex]v= \sqrt{\frac{2GM}{r}}[/itex]
Which allows for [itex]r[/itex] such that [itex]v>c[/itex], eg [itex]r= \frac{2GM}{9c^2}[/itex] which gives [itex]v=3c[/itex]
 
  • #14
ChrisVer said:
It is let's say [itex]\frac{v}{c} = \beta(r)[/itex]... it shows the change of the velocity of a mass that began from infinity with 0 velocity under the "Newtonian" gravitational law of a point-like mass source [itex]M[/itex] [...] So for example, when the body is at a distance [itex]x=2 \times \frac{GM}{c^2}[/itex] away from the source, it will have a velocity [itex]v \approx 0.75c[/itex]...
In a closed thread someone said that the velocity of the object would eventually reach a value larger than [itex]c[/itex] due to acceleration. I just wanted to counter this idea via special relativity alone...
The curve certainly makes sense. You can see those ##\gamma##'s kicking in.
 
  • #15
ChrisVer said:
We have from the SR 2nd Newton law

SR can't be used to model gravity.

ChrisVer said:
So the information of Schwarzschild radius singularity is contained within SR?

No. You need to use GR to model gravity.

ChrisVer said:
That looks like a GR conversation..:sorry:

So should this thread be. You can't model gravity using SR.
 
  • #16
ChrisVer said:
It was more like a special relativistic application of ##F= \frac{dp}{dt}##.

But for gravity, ##F = 0##. Gravity is not a force in relativity. A force in relativity is something that causes proper acceleration. Gravity doesn't. However the computations you are making work out formally, they are physically meaningless as far as gravity is concerned.
 
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  • #17
ChrisVer said:
Starting from a locked thread
Please do not reopen locked threads.
 

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