Are Black Holes Really Black and Just Holes?

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Discussion Overview

The discussion revolves around the nature of black holes, questioning whether they are truly "black" and if they can be accurately described as "holes." Participants explore various theoretical and conceptual aspects, including classical and quantum mechanical perspectives, dimensionality, and implications for astrophysics.

Discussion Character

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

Main Points Raised

  • Some participants assert that black holes are classically black due to their event horizons, which prevent light from escaping, while others note that quantum effects suggest they may emit a small amount of radiation.
  • There is ambiguity around the term "hole," with some suggesting it refers to a hole in spacetime, while others question the appropriateness of the term altogether.
  • Some physicists propose that black holes might act as gateways to other universes, though this remains speculative and is countered by concerns about extreme gravitational forces.
  • Participants discuss the dimensionality of black holes, with some arguing they are not spherical or star-like, while others emphasize the significance of the event horizon's geometry.
  • There are claims that supermassive black holes could serve as cosmological constants, but this is contested by others who argue they do not consume entire galaxies.
  • Questions arise about the density of supermassive black holes, with some suggesting they can be less dense than water when considering average density calculations.
  • Entropy in the context of black holes is discussed, with clarification that it does not directly relate to the rate of evaporation but rather to the counting of microstates in statistical mechanics.

Areas of Agreement / Disagreement

The discussion contains multiple competing views and remains unresolved on several points, particularly regarding the nature of black holes, their dimensionality, and the implications of their properties.

Contextual Notes

Participants express uncertainty about the precise definitions and implications of terms used in the discussion, such as "hole" and "entropy," and there are unresolved mathematical considerations regarding density and dimensionality.

Dremmer
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Are they really black? And are they really holes? I'd say they are actually neither. Would I be right?
 
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a) Classically, yes they are black. What I mean is that the obvious boundary of the object, the event horizon, is a one way barrier in that things can only go in, not out. This includes light. So an object which is absorbing all light but giving off none would indeed appear pitch black.

Quantum mechanically, the story is not so simple and it turns off that black holes do 'shine' a little. However, this effect is far too miniscule to be important for any astrophysical (read: caused by collapsing stars) black holes.

b) The word hole, in this sense, doesn't really have a precise meaning. Perhaps what is meant is that they are 'holes' in the fabric of spacetime, but this is equally imprecise. Usually this is seen visually by having an embedding diagram in which the BH literally looks like a type of funnel, but this is an artifact of the way we choose to draw these diagrams. In another sense, perhaps they are holes in that things fall in but do not come out. I don't really know what is meant by the assertion of them being just 'holes', so I can't really say.
 
While some physicists suspect they may be gateways to other universes, it is definitely a one way street.
 
Chronos said:
While some physicists suspect they may be gateways to other universes, it is definitely a one way street.

Perhaps, but you would be pulled apart by the immense gravitational pull before you got through it, which is why we don't know for sure. Also, I don't think they are "holes" so much as spheres, because, after all, they are collapsed stars.
 
They aren't really spherical or star-like in any sense. They are infinitely small, you could argue that it's just plain weight.
 
Their dimensionality is typically defined by their event horizon, which extends a measurable distance from the putative singularity.
 
T=0 said:
Perhaps, but you would be pulled apart by the immense gravitational pull before you got through it, which is why we don't know for sure. Also, I don't think they are "holes" so much as spheres, because, after all, they are collapsed stars.

Feodalherren said:
They aren't really spherical or star-like in any sense. They are infinitely small, you could argue that it's just plain weight.

The event horizon is a spherical region of space (in a non-rotating black hole) that is simply the point where the curvature of space becomes such that all paths in spacetime lead into the black hole. In more classical terms it's where the force of gravity become strong keep even light in. One inch out from this barrier the force is ALMOST as strong, but not quite, and the force is reduced with distance.
 
Surely that means that super-massive black holes could work as the cosmological constant, along with dark matter, but also could bring the end to whole solar systems, maybe even galaxies.
 
  • #10
Supermassive black holes are known to exist at the center of most large galaxies - some with masses on the order of 10 billion solar. They are not known to eat the entire galaxy, or corrupt neighboring galaxies.
 
  • #11
@T=0
Not really. For example, if the Earth suddenly condensed to the size of a BH (for whatever reason,) any observer on the Moon wouldn't notice a thing other than, of course, the Earth shrinking. Shrinking something doesn't mean it becomes superpowerful gravitationally, it just means stuff can get closer before being held up by its surface.
 
  • #12
Are Black Holes 2 Dimensional? And if so does that mean that when a 3 dimensional object is sucked into one that it is somehow reassembled as a 2 dimensional object and it's 3D characteristics are ripped from it and left to hover the black hole?
 
  • #13
Also, I read somewhere that Supermassive Black Holes less dense than water, is this true?
 
  • #14
Alex1 said:
Are Black Holes 2 Dimensional? And if so does that mean that when a 3 dimensional object is sucked into one that it is somehow reassembled as a 2 dimensional object and it's 3D characteristics are ripped from it and left to hover the black hole?

Perhaps in some sense, but I doubt it's the sense you're thinking of. The entropy of a black hole is proportional to the area of its event horizon, a two dimensional surface, rather than the total volume of the black hole. Nevertheless, they occupy a definite three-dimensional volume in our universe (as long as we're calling anything within and including the EH the 'black hole').

And yes a SMBH can indeed be less dense on average than water. I speak on average because the calculation is done by simply dividing the total mass by the volume of the sphere enclosed in the event horizon. The radius of the the event horizon scales like M, so volume goes like M^3. Thus, density = M/Vol = M/M^3 = M^-2, so you can make the average density arbitrarily small simply by increasing the mass.
 
  • #15
When you use the term Entrophy in the context of a Black Hole, is that just the rate at which it's evaporating?
 
  • #16
Alex1 said:
When you use the term Entrophy in the context of a Black Hole, is that just the rate at which it's evaporating?

Well since entropy is not in any way a measure of rate of evaporation no. The quantities are related in a thermodynamic context (and arose basically at the same time as Hawking and Bekenstein were figuring these things out), but the entropy is really just the standard entropy of statistical mechanics: a counting of microstates.
 
  • #17
Alright cool Thanks
 

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