Escaping a Black Hole's Event Horizon

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    Event horizon Horizon
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Discussion Overview

The discussion revolves around the concept of escaping a black hole's event horizon, exploring classical and relativistic perspectives on the behavior of objects, particularly spaceships, near this boundary. Participants examine the implications of kinetic energy, gravitational forces, and the limitations imposed by general relativity.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant presents a classical derivation of the Schwarzschild radius, questioning the escape of objects that can exert forces, such as a spaceship throwing off fuel.
  • Another participant points out that the kinetic energy formula used is nonrelativistic and suggests that relativistic formulas should be applied for particles moving close to the speed of light.
  • A participant expresses confusion about what prevents a spaceship from escaping the event horizon when throwing off fuel at a constant rate, pondering the necessity of exceeding the speed of light for escape.
  • One participant asserts that time stops at the event horizon, implying a fundamental change in the nature of movement and escape at this boundary.
  • Another participant reiterates the question about escaping the event horizon, emphasizing that black holes are not Newtonian and that reasoning based on classical physics is flawed. They explain that accelerating infinitely fast would be required to remain at the same radius as one approaches the event horizon.

Areas of Agreement / Disagreement

Participants express differing views on the applicability of classical mechanics versus general relativity in the context of black holes. There is no consensus on the mechanics of escaping the event horizon, with multiple competing perspectives remaining unresolved.

Contextual Notes

Participants highlight limitations in reasoning based on classical physics when discussing black holes, indicating a need for a deeper understanding of general relativity. The discussion also reflects uncertainty regarding the mathematical justification for escape conditions.

cyborg6060
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When classically deriving the Schwarzschild radius of a black hole, the kinetic energy of an outgoing particle (moving at the impossible-to-achieve maximum of the speed of light) is equated with the gravitational potential of the black hole at that point.

\frac{1}{2}mc^2 = \frac{GMm}{r}
r=\frac{2GM}{c^2}

This seems reasonable for justification that light cannot escape, but what about objects that can do work or exert forces?

The gravitational force of the black hole at the event horizon is:

F = \frac{GMm}{r^2}

One could imagine a spaceship throwing off fuel in the opposite direction so that

\frac{Δp}{Δt} = \frac{GMm}{r^2}.

I'm well aware that this is not the case, so I'm curious as to what the reasoning is. Thanks for the help!
 
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the formula above does give the correct value of r but

I would just like to point out that ½mc² is the nonrelativistic formula for kinetic energy (of a particle moving at c)

In reality, for velocities close to c, one would have to use the relativistic forumula to find the actual kinetic energy.

66f7e00a057b2bf8fb7e7fbfb188a4ae.png
 
My issue is that I don't see what prevents a spaceship throwing off fuel at a constant rate A kg/s, so that:

\frac{dp}{dt} = \frac{GMm}{r^2}

A v = \frac{GM(m - At)}{r^2}.

What prevents this system (classically, so long as v is not too large) from escaping the event horizon?

My initial thought would be that v would have to be greater than the speed of light, but I can't quite justify that mathematically.

Any thoughts would be incredibly helpful.
 
time stops at the event horizon

http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html
 
Last edited by a moderator:
cyborg6060 said:
My issue is that I don't see what prevents a spaceship throwing off fuel at a constant rate A kg/s, so that:

\frac{dp}{dt} = \frac{GMm}{r^2}

A v = \frac{GM(m - At)}{r^2}.

What prevents this system (classically, so long as v is not too large) from escaping the event horizon?

My initial thought would be that v would have to be greater than the speed of light, but I can't quite justify that mathematically.

Any thoughts would be incredibly helpful.

In a Newtonian sense, you're right. But black holes are not Newtonian objects, and although you get the right answer for the Schwarzschild radius, it's completely by incorrect reasoning. It's not actually an issue with special relativity -- but with the much larger theory of General Relativity.

If you imagine yourself going towards the event horizon of a real Einsteinian black hole, you would need to accelerate infinitely fast as you fell down towards the event horizon just to stay at the same radius! Curiously, once you've fallen past the event horizon, any amount of blasting your rockets you do will only hasten your eventual demise! If you want to live as long as possible, the best bet is to sit there and do nothing.
 

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