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Yet another question about black holes |
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| Sep16-12, 08:38 PM | #1 |
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Yet another question about black holes
A comparison of a large star and a black hole: Both have identical masses.
Correct me if I'm wrong but gravitationally, they would be the same because we assume that the gravitational force acts from the center of mass. So here's the question: If both the black hole and the star have the same mass and the same gravitational pull, why does the black hole have an event horizon? I know that it has something to do with the density of the stellar object but I was hoping that someone could explain this to me a little better. |
| Sep16-12, 08:48 PM | #2 |
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Hi.
My guess is that if the two celestial bodies are covered by curtains and we feel only the same gravitational effects outside them thus we cannot know which is BH and which is ordinaly star. When we remove curtains we find that star is big and sparse and BH is compact and dense like 1 kg of cotton and 1 kg of iron. Who claims that cotton and iron should be same volume ? GR says too much compact body make horizon around it. |
| Sep16-12, 08:55 PM | #3 |
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I understand that despite the difference in the densities, the gravitational forces would be identical to a point. My question has to do with why one has an escape velocity < c and why the other has an escape velocity > c.
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| Sep16-12, 09:16 PM | #4 |
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Yet another question about black holes
Let us say the event horizon is the "surface" of the black hole and the photosphere is the "surface" of the star. What is the major difference between the two? Diameter. The black hole is TINY, while the star is hundreds of thousands if not millions of kilometers across. We can get MUCH closer to the center of the black hole than we can to the star before we cross the boundary. If we could go into the star we would see that there is material BEHIND us now that isn't pulling us towards the center anymore. So for the same distance from the center, the black hole has more mass pulling you in to the center.
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| Sep16-12, 11:40 PM | #5 |
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For a black hole, for which all of the mass is essentially crushed down to a single point, you can actually get close enough i.e. to within a radius of the object where escape v > c. |
| Sep17-12, 10:38 AM | #6 |
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These explanations were exactly what I was looking for. Thanks!
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| Sep24-12, 03:21 PM | #7 |
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The gravity is given by the mass of the gravitational body and the distance between the point you measure and its point-mass (the point in its centre), as you know. (and G, but this is besides the point) More precisely, directly proportional with the former and inversely proportional with the later.
In the case of the star, because it is too extended (large radius), the distance between its centre and this point on its surface is too large to generate a gravity sufficient to stop light. Now, you may get inside the star towards its centre, but the net gravity does not increase anymore, because you've got mass around pulling in all directions. This was just to explain why there's no black hole inside. :P But the matter of the black hole is that compact that it fits - or is smaller than - the Schwarzschild radius, which is the distance from the center to the point where, in respect to the given mass of the object, the gravity is that large that light cannot escape. And don't confuse the event horizon with the surface of the gravitational body of the black hole. If the radius of the body is equal to its corresponding mass' Schwarzschild radius (which is also the radius of the sphere determined by the event horizon), then they coincide. But this body may be even more compact, which means the radius of its matter can be smaller than its Schwarzschild radius, however no one outside can see that because its even horizon (the "surface" at the distance of its Schwarzschild radius) is around it and lets nothing escape. So the black hole is this entire phenomenon: not only the body inside, but also this "black aura" around it. |
| Sep24-12, 03:40 PM | #8 |
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| Sep24-12, 04:26 PM | #9 |
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A black hole is formed anytime the radius of a gravitating body is less than its Schwarzschild limit [which is a function of mass]. This does not require a singularity, although there is currently no explanation what would prevent a singularity from forming at such high densities.
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| Sep24-12, 04:46 PM | #10 |
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Yeah, cool, thank you Chronos! Minutes before I found an answer on a different thread that ringed the bell:
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| Sep26-12, 03:47 PM | #11 |
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The event horizon is where escape velocity increases past c. There is no such boundary for stars, because when you go inside a star, the mass you have passed screens out the gravitational force. the force actually approaches zero as you approach the center of a massive star. You can get arbitrarily close to a black hole's singularity and there is still no screening of the gravitational force. Therefore, you will ultimately pass a radius as which the escape velocity is greater than the speed of light.
Study GAUSS'S LAW in the context of mass and gravity (instead of charge and electromagnetism), and take a look at the equations for escape velocity and gravitational force (Newton's law will do just fine for these purposes) and you will see the difference between the two scenarios you posed. |
| Sep28-12, 02:45 PM | #12 |
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I have searched for information on black holes many times and never found this question directly addressed. How can a singularity exist when matter that falls into a black hole “stops” at the event horizon? I understand that from the perspective of the matter which has entered the event horizon that time hasn’t stopped but from the perspective of the outside universe it has. So that all the matter that has ever fallen into a black hole is still suspended at the event horizon, meaning that in finite time no matter will ever reach the singularity. So you might say that the matter in a black hole will reach the singularity in the infinite future. However, given that black holes evaporate by Hawking Radiation, all black holes have finite lifespans, and will evaporate before any matter can reach the singularity. As far as I can tell, from the perspective of the matter which has reached the event horizon the black hole would instantly evaporate the moment the event horizon is reached. It appears that singularities are not possible. The answer may be obvious, and I simply lack the understanding to see it. |
| Sep28-12, 03:00 PM | #13 |
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Welcome to PF,
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| Sep28-12, 03:18 PM | #14 |
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| Sep28-12, 03:25 PM | #15 |
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Mentor
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| Sep28-12, 03:34 PM | #16 |
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Another thing is, in the frame of reference of the infalling observer, time passes at the normal rate, and all indications from theory are that such an observer would continue to fall in, be torn apart by tidal forces, and then smash into the "singularity" (or whatever is in there). Either this happens or it doesn't, the only cause for disagreement can be over when it happens. So I'm pretty dubious about your claim that matter would get "frozen" at the event horizon. This is really not how gravity works. You keep falling in until you die. For what it is worth, here is the relevant section of the Wikipedia article on black holes:
http://en.wikipedia.org/wiki/Black_hole#Singularity |
| Sep28-12, 03:43 PM | #17 |
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I agree with you that infinite density would be unphysical. Which is why I began to ponder how such an impossibility could in fact exist. I keep hearing physicists say that physics breaks down at the singularity and that quantum gravity will provide the answers that neither quantum machanics nor general relativity can. But as I thought about it and read about it I was struck with the question I have asked. It appears that singularities are mathematical artifacts, and can't actually happen in nature (by my understanding). And yet physicists continue to talk about them as if they exist so I'm probably missing something. I don't claim to have thought of something nobody has thought of before. Undoubtedly this question has been asked and answered long before I stumbled on it. |
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