Does a black hole have a surface area?

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Discussion Overview

The discussion revolves around the concept of whether a black hole has a surface area, specifically focusing on the nature of the event horizon and its relationship to the Schwarzschild radius. Participants explore the geometric properties of black holes, the definitions of relevant terms, and the implications of these definitions in the context of black hole physics.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants propose that the surface area of a black hole is related to the event horizon, questioning whether it can be defined by the Schwarzschild radius.
  • Others argue that the Schwarzschild radius should be understood as a coordinate label rather than a physical radius, emphasizing that the area is the fundamental geometric quantity.
  • A later reply clarifies that the area of the horizon is not defined by the formula ##4 \pi R_s^2##, but rather that ##R_s## is derived from the area, indicating a logical precedence of area over radius.
  • Some participants express confusion about the relationship between the Schwarzschild radius and the surface area, suggesting that the surface area corresponds to a sphere with the Schwarzschild radius.
  • Others challenge this view by stating that the black hole's horizon does not have a geometric center and cannot be treated as a conventional spherical object in Euclidean space.
  • There is a discussion about the implications of Newtonian gravity in the context of black holes, with some participants asserting that Newtonian principles do not apply to black holes.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the definitions and implications regarding the surface area of black holes and the Schwarzschild radius. Multiple competing views remain, particularly concerning the interpretation of the Schwarzschild radius and its relationship to the event horizon.

Contextual Notes

Participants highlight the importance of understanding the geometric properties of black holes and the limitations of using classical definitions. The discussion reveals dependencies on definitions and unresolved interpretations of the mathematical framework involved.

Stephanus
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[Moderator's note: Spin-off from another thread.]

Keith said:
So it's not that bigger black holes emit less hawking radiation than smaller ones? It's just that the surface area becomes more spread out as the black hole becomes larger and is distributed less intensely to an object that remains a constant size? In other words, theoretically, if an object geometrically grew at the same rate as the black hole, would it experience the same amount of hawking radiation the whole time?
I'm sorry, does black hole have surface area? Did you mean the sphere defined by Schwarzschild Radius?
 
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Stephanus said:
does black hole have surface area?

Yes. More precisely, the hole's horizon does. See below.

Stephanus said:
Did you mean the sphere defined by Schwarzschild Radius?

Yes, but you're looking at it backwards. The "Schwarzschild radius" is really ##\sqrt{A / 4 \pi}##, where ##A## is the area of the horizon (which is a 2-sphere). The area is the geometric quantity; the "radius" is just a coordinate label and doesn't correspond to a physical radius.
 
PeterDonis said:
Yes. More precisely, the hole's horizon does.
The event horizon.
PeterDonis said:
Stephanus said:
Did you mean the sphere defined by Schwarzschild Radius?
Yes, but you're looking at it backwards. The "Schwarzschild radius" is really ##\sqrt{A / 4 \pi}##, where ##A## is the area of the horizon (which is a 2-sphere). The area is the geometric quantity; the "radius" is just a coordinate label and doesn't correspond to a physical radius.
Perhaps I should state my question more clearly
The area defined by ##4\pi {R_{schwarzshild}}^2##?
 
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Stephanus said:
The event horizon.

Yes.

Stephanus said:
The area defined by ##4\pi {R_{schwarzshild}}^2##?

The answer is still the same: you are looking at it backwards. The area is not defined by ##4 \pi R_s^2##. ##R_s## is defined as ##\sqrt{A / 4 \pi}##. The area ##A##, as the geometric quantity, is logically prior to ##R_s##, which is just a coordinate label.
 
PeterDonis said:
The answer is still the same: you are looking at it backwards. The area is not defined by ##4 \pi R_s^2##. ##R_s## is defined as ##\sqrt{A / 4 \pi}##. The area ##A##, as the geometric quantity, is logically prior to ##R_s##, which is just a coordinate label.
Okay...
So the surface area of a black hole is the surface area of a sphere which has the Schwarzschild radius IS ##4 \Pi R_s##
While Rs itself is defined by https://en.wikipedia.org/wiki/Schwarzschild_radius#Formula
##R_s = \frac{2GM}{c^2}##, still Newton, right? Only instead of Ve2, we replace it with the speed of light.
 
Stephanus said:
So the surface area of a black hole is the surface area of a sphere which has the Schwarzschild radius

No. It is the surface area of a sphere which is labeled by the radial coordinate ##R_s##. That number is not the actual geometric radius of that sphere; in fact, that sphere, the horizon, has no geometric radius in the ordinary sense. , because it has no geometric center. A black hole is not just a spherical object sitting in ordinary Euclidean space.

Stephanus said:
Rs itself is defined by https://en.wikipedia.org/wiki/Schwarzschild_radius#Formula
##R_s = \frac{2GM}{c^2}##,

That formula tells you how to calculate ##R_s##, yes. But it doesn't tell you how ##R_s## is defined, geometrically. It doesn't tell you that ##R_s## is the geometric radius of anything. It just tells you how to calculate a number.

To see what ##R_s## actually means, you have to look at the metric; you have to look at what determines which 2-sphere is the hole's horizon; and you have to look at what geometric properties that 2-sphere actually has. When you look at all those things, you find that, as I said before, ##R_s## is not the geometric radius of the horizon; it's just a coordinate label. The geometric property that actually characterizes the horizon is its area.

One way to see this is to find coordinates in which the horizon is labeled by a different coordinate; for example, isotropic coordinates. In these coordinates, the horizon is labeled by the radial coordinate ##R = GM / 2 c^2##, i.e., 1/4 of the value ##R_s## that labels it in Schwarzschild coordinates. But the area of the horizon is the same, because that's an invariant geometric property.

Stephanus said:
still Newton, right? Only instead of Ve2, we replace it with the speed of light.

No. A black hole is certainly not an object to which Newtonian gravity applies.
 

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