High speeds - becoming a black hole

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Discussion Overview

The discussion centers around the claim that a spaceship, when accelerated to speeds approaching that of light, could transform into a black hole. Participants explore the implications of relativistic mass, energy requirements for acceleration, and the nature of black holes in different frames of reference.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants argue that a spaceship cannot become a black hole simply by reaching high speeds, as relativistic mass is frame-dependent and does not change in the ship's own frame.
  • Others propose that the energy required to accelerate the ship to near-light speeds could lead to a scenario where it behaves like a black hole due to the equivalence of mass and energy.
  • A participant mentions that the perception of an object as a black hole could vary between observers, suggesting that relativistic effects might lead to different interpretations of gravitational influence.
  • Some contributions emphasize that a black hole is a frame-independent feature of spacetime, asserting that if it is not a black hole in the ship's rest frame, it cannot be one in any other frame.
  • There is a discussion about the implications of Hawking's statements regarding black holes and particle accelerators, with participants questioning the context and interpretation of his claims.
  • Concerns are raised about the role of relativistic mass and its gravitational influence, with some participants cautioning against its use due to potential confusion.
  • Participants discuss the nature of photons and their gravitational effects, debating whether they contribute to spacetime curvature.

Areas of Agreement / Disagreement

Participants express a range of views, with no consensus reached on whether a spaceship can become a black hole at high speeds. The discussion remains unresolved, with competing interpretations of relativistic effects and black hole characteristics.

Contextual Notes

Participants highlight the complexity of the discussion, noting that assumptions about energy, mass, and frame of reference are critical to the arguments presented. There are unresolved mathematical steps and dependencies on definitions that affect the conclusions drawn.

  • #31
aaroman said:
PS I am your friend :) But when somebody tells me that things look the same in two frames of refference, when obviously do not, I don't believe.

Wonderful! However, you have taken the mantra "everything is relative" too far. Black holes are not relative (at least not in the sense that I think you want them to be). No matter how fast you move, the components of the curvature are always finite if there is no black hole, and the components are always divergent at some point if there is a black hole. Also, like prevect said, no matter how fast you move, light beams that escape in one frame will still escape in every other frame hence no black hole in one frame means no black hole in every frame.

Regarding your question about the doppler shifted photons, the gravitational field is the same! What do I mean by this? If you make a transformation of coordinates corresponding to a Lorentz transformation then all that happens is that the components of R_{\alpha \beta \gamma \delta} (or any other tensor) get scrambled up. The curvature invariant that I defined earlier is the same in any frame. Geodesics still deviate in the same way as before, so no true new gravitational effects have been produced (although, of course, the coordinates you assign to geodesic and its tangent vector change).
 
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  • #32
no black hole in one frame means no black hole in every frame
Well, I just edited previous post, I found a paper that says that a singularity can be no singularity in another coordinate frame, so they seem relative if that is true.
Regarding your question about the doppler shifted photons, the gravitational field is the same!
Energy and momentum is different. Why is the gravitational result the same?
The curvature invariant that I defined earlier is the same in any frame
The curvature is invariant, but the force one feels might be different, or else no matter of the reference frame, all would feel the same gravity, which is not true. I tested this experimentally :)
 
  • #33
aaroman said:
Well, I just edited previous post, I found a paper that says that a singularity can be no singularity in another coordinate frame, so they seem relative if that is true.

You have confused a so called coordinate singularity with a true space time singularity. The traditional Schwarzschild metric is
<br /> ds^2 = - \left(1 - \frac{2 M}{r}\right) dt^2 + \frac{1}{\left(1 - \frac{2 M}{r}\right)}dr^2 + r^2 d\Omega^2 <br />
and there is clearly a coordinate singularity at r = 2 M, the event horizon. However, the components of the curvature are perfectly well defined here so there is no actual singularity. The apparent singularity is an artifact of the coordinate system. The Kruskal-Szekeres coordinate system is one way of removing this artifical coordinate singularity. However, the singularity at r = 0 is a true spacetime singularity and cannot be removed by a clever choice of coordinates. The curvature diverges at r = 0.
 
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  • #34
Now I might have a problem with points in physical reality, but for the rest I get it.
 
  • #35
aaroman said:
Not at the same time, though. Fore some is dead, for some is still living. For some is still unborn, so no, person B is not dead in all frames.
Going back to gravity from this analogy, in one frame the "force" felt could be very weak, in another one could be very strong. One frame just has to accelerate enough :)

I'm not questioning physical reality, but the appearance. If I'm not mistaken, for an outside observer, a falling object will never pass through the event horizon of a black hole. That is not true for the object that falls in. It passes through the event horizon in a finite time. So in some sort of way, for one observer B never "dies", for the one that falls though it's completely another matter.

You are correct that a falling object will pass through the event horizon at t=infinity in the coordinate system of the outside observer, and that it will pass through the event horizon in a finite proper time as measured by its own clock. This happens because the coordinate transforms are singular - specifically, it is the Schwarzschild coordinates that are singular in this cae.

If you look at the more detailed post I gave earlier, response #12

https://www.physicsforums.com/showpost.php?p=825259&postcount=12

I mentioned that it was important that the coordinate transforms were not singular.

The result of this is that because the coordinate transforms aren't singular, a beam of light that escapes to infinity in the rest frame of the object still escapes to infinity in "the" coordinate system in which the object is moving.

In flat space-time, you are probably familiar with time dilation for a moving object. The time dilation factor can be very large, but will always be finite. This finite time dilation means that there are no singularities in the coordinate transform for a moving observer - the Lorentz transform - any event t occurring on the moving train at a finite time occurs at a finite time t' on the non-moving station, and vica-versa.

PS I just looked over some papers: either they are wrong, or the affirmation that a black hole is a black hole in all reference frames which was presented on this thread is wrong. Talking abaout the Schwartzchild solution, is says something like that:
one can discover different coordinate frames in terms of which no singularity is seen. ... Introduce new coordinates ("Kruskal coordinates")
Well, I think I gave enough. It's from "Introduction to General Relativity" by G. Hooft. So what's the truth here? Is it a black hole or not in all coordinates?

This quote is about the "bad behavior" of the Schwarzschild coordinates at the event horizon that was mentioned earlier. A black hole in Kruskal coordinates remains a black hole - the Kruskal coordinates simply remove the "bad behavior" that the Schwarzschild coordinates exhibit at the event horizon.
 

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