Throwing a string into a blackhole

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    Blackhole String
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Discussion Overview

The discussion centers on the hypothetical scenario of throwing a string into a black hole and the implications of such an action, particularly regarding the fate of the string and any object attached to it. Participants explore concepts from general relativity, the behavior of strings under extreme conditions, and the potential for energy extraction from black holes.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions what happens to a string thrown into a black hole, particularly if something is attached to it.
  • Another participant suggests that the string may break or the attached object may be reeled in, citing physical limits such as the weak energy condition and the speed of sound in the string.
  • A later reply discusses a relativistic elasticity model that could explain the behavior of the string, noting that it could survive intact even after passing through the event horizon under certain conditions.
  • One participant speculates about the implications of the string being wrapped around a generator, questioning whether energy could be extracted from the black hole if the string does not break.
  • Another participant clarifies that while energy can be extracted from objects falling into a black hole, the process described would ultimately add energy to the black hole rather than extract it.
  • Further discussion includes the idea that the energy of infalling matter contributes to the black hole's mass and can lead to energetic jets, emphasizing the conservation of energy in this context.
  • One participant introduces the concept of length contraction for observers at different positions relative to the black hole, noting the differing perceptions of the string's length and behavior.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the fate of the string and the potential for energy extraction from the black hole. There is no consensus on the implications of the string's behavior or the energy dynamics involved.

Contextual Notes

Limitations include assumptions about the strength and properties of the string, the effects of general relativity on energy conservation, and the conditions under which the string might break or remain intact.

Who May Find This Useful

This discussion may be of interest to those exploring concepts in general relativity, theoretical physics, and the behavior of materials under extreme gravitational conditions.

ice109
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if i threw a string from a great distance into a black hole what would happen? if something was attached to the other end of the string would that thing eventually get realed in?
 
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The short answer is that either the string will break, or the object attached to the string will get reeled in.

There are physical limits as to how strong a string can be, one of them is imposed by the "weak energy condition", another limit is imposed by requiring that the speed of sound in the string can't be greater than the speed of light.

There is a rather detailed (and technical) analysis of this online at http://gregegan.customer.netspace.net.au/SCIENCE/Rindler/RindlerHorizon.html

which uses a relativistic elasticity model (called the hyperelastic model) to model the characteristics of the string.

The hyperelastic model is (relatively) easy to work with mathematically but will only give sensible results if the input parameters are restricted to a reasonable physical range.

The webpage includes some gif-movies of the simulation results, and also has some references to the literature on relativistic elasticity.
 
so i just skipped to the end cause i really don't know anything about GR and we have this

"Although a string lowered in this fashion appears doomed to break eventually, this example shows that there's no reason it can't survive intact not only after crit, but also after the bottom of the string has passed through the horizon according to the string's own definition of simultaneity. In other words, a spacelike slice orthogonal to the world lines of the string's elements can run all the way from the bottom of the string, on the far side of the Rindler horizon, to the point of unreeling, with the tension everywhere remaining well below the limit set by the weak energy condition."

so now suppose this string was wrapped around a generator. what then? if the string doesn't break and turns the generator we get power from the black hole? is there something I'm missing?
 
You should read a bit further:

Given some function of proper time which expresses the rate at which the string is being unreeled, there will be a time [itex]\tau_{crit}[/itex] after which no signal from the point of unreeling can reach the object at the end of the string before it passes through the horizon.

After [itex]\tau_{crit}[/itex], the only way to keep the string from eventually breaking (assuming it hasn't broken already) will be to continue to feed it out at an increasing rate. Clamping the string, attempting to pull the object back up, or even just feeding out the string at a constant rate, will all ultimately cause the string to break, though the exact time when that happens will depend on the physical properties of the string.
 
ice109 said:
so now suppose this string was wrapped around a generator. what then? if the string doesn't break and turns the generator we get power from the black hole? is there something I'm missing?
1. You wouldn't be able to enjoy the benefits of this energy indefinitely, since the generator would get pulled closer to the black hole when you do this.

2. The process you describe doesn't move energy from inside the event horizon to outside, because the rope itself has lots of energy (E=mc2 remember). So the process will put more energy into the black hole, not steal energy from it.
 
You can extract some of an objects rest mass energy by dropping it into a black hole, if that's the point of the original question. Black holes are often associated with very energetic "jets", for instance, and it is the gravitational energy of the infalling matter that helps power them.

http://www.space.com/scienceastronomy/blackhole_jets_040817.html

The black hole grows in mass by the 'energy at infinity' of the infalling matter, not by the rest mass of the infalling matter. This means that part of the energy (including the rest energy) of the infalling matter will go into increasing the mass of the black hole, and part will usually be radiated away during the fall in one form or other. So the total energy of the system stays constant, part of the mass of the infalling object is converted into various forms of energy and radiated away, the rest goes into increasing the mass of the black hole.

While energy conservation can be problematical in GR, a black hole isn't one of those cases where this issue arises. The black hole space-time is static AND asymptotically flat.
 
Last edited:
From what I understand:

Let the string, marked off in equal lengths, to be attached to an observer. For the stationary observer well outside of the event horizon, the lengths will appear to Fitzgerald contract infinitely as the string leads toward this limiting surface. For the observer lowered through the event horizon on the string, the lengths conserve themselves locally, but in the direction of the apparent singularity one sees the event horizon as approaching a pointlike gravitational (and observational) collapse.
 

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