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Is then gravitation expressed at the event horizon of the black hole as a result of the in falling matter. If so then what part would the original mass play? Or is this looking at it wrong?
To collapse below the Schwarzchild radius some of the mass is already contained within this volume.
Mass outside this region, when collapsing inwards, will approach the radius with escape velocity increasing proportionally.
Has anyone tried working this through during the collapse event to calculate the effects on gravity as the process evolves?
Quote from: jeffreyHTo collapse below the Schwarzchild radius some of the mass is already contained within this volume.As observed from outside the event horizon, nothing can pass through the event horizon and go inside.Quote from: jeffreyHMass outside this region, when collapsing inwards, will approach the radius with escape velocity increasing proportionally.Actually, as matter approaches the event horizon it slows down and comes to a stop at the event horison and never crosses it.Quote from: jeffreyHHas anyone tried working this through during the collapse event to calculate the effects on gravity as the process evolves?I don't understand what you mean by "the effects on gravity." Can you clarify this for me please?
Quote from: jeffreyH on 05/10/2013 08:22:28Is then gravitation expressed at the event horizon of the black hole as a result of the in falling matter. If so then what part would the original mass play? Or is this looking at it wrong?I'm sorry but I don't understand this question. Can you rephrase it for me please?
The effects on gravitational field strength. Does it increase or decrease overall? This is assuming a Kerr black hole.
Quote from: Supercryptid on 05/10/2013 06:29:13Interesting...can the effect of added pressure increase gravity significantly? Does that make the "replace the Sun with a black hole" analogy I mentioned earlier wrong then?No. That remains correct.Each case must really be analzed individually. It's dangerous to form general conclusions. Let me give you an example; you've heard of cosmic strings, right? A straight cosmic string has an enormous linear mass density. It's extremely thin, less than the width of an atom but never ends in an open universe. It has an equally large tension too. Tesion is like pressure but is negative. They contribute equally in the case of the cosmic string. The end effect is that you could be standing right next to a cosmic string and not know it from its gravitational field. The only gravitational effect a cosmic string has is to change tghe topology of the surrounding space from planar to conical. Amazing stuff, isn't it? A vacuum domain wall is another example. In this case the wall is a two dimensional object rather than a one dimensional object like the string. The tension contributes twice as much so the wall has a replusive gravitational field. Interesting thing about the vacuum domain wall is that the gravitaitonal field it generates has zero spacetime curvature.In three dimensions there is even more repulsion and this is how the accelerating expansion of the universe works.On the other hand the effective active gravitational mass density of radiation is that the (positive) contribution of the raditation pressure contributes a significant amount to the active-grav-mass.
Interesting...can the effect of added pressure increase gravity significantly? Does that make the "replace the Sun with a black hole" analogy I mentioned earlier wrong then?
Forgive me for taking this a bit off topic, but I find these conclusions rather fascinating. I've heard of domain walls before, but never that they were gravitationally-repulsive. If only we could prove their existence and duplicate them on a tiny, controlled scale.
You sound fairly confident about the gravitational repulsion that causes the Universe's expansion.
Yet I've never heard of that explanation before. It does sound like a nice model, as it doesn't invoke a mysterious "dark energy" to explain it. Is this a mainstream theory?
This accelerating expansion effect is sometimes labeled "gravitational repulsion", which is a colorful but possibly confusing expression. In fact a negative pressure does not influence the gravitational interaction between masses—which remains attractive—but rather alters the overall evolution of the universe at the cosmological scale, typically resulting in the accelerating expansion of the universe despite the attraction among the masses present in the universe.
I have often thought that collapsing systems such as black holes and neutron stars can only exist in an expanding system.
If the system were collapsing we should see white holes.
I This is why white holes are unstable ...
Quote from: jeffreyHI have often thought that collapsing systems such as black holes and neutron stars can only exist in an expanding system. I can't see why? What leads you to believe this?Quote from: jeffreyHIf the system were collapsing we should see white holes.What system are you referring to and why would you expect to see white holes. There's no evidence that such objects even exist.Quote from: jeffreyHI This is why white holes are unstable ...Do you have a source for this assertion? I can't imagine why it would be so.Jeff - You seem to enjoy black holes. You should consider reading Exploring Black Holes - 2nd Ed by Taylor, Wheeler and Bertschinger at http://exploringblackholes.com/I think you'd also get a great deal of satisfaction reading Black Holes and Time Warps - Einstein's Outrageous Legacy by Kip Thorne. Thorne is the worlds leading theorist on black holes.
I was wondering if the Pauli exclusion principle could be one of the principle mechanisms of gravitational interaction.
Astronomy provides a spectacular demonstration of the effect of the Pauli principle, in the form of white dwarf and neutron stars. In both types of body, atomic structure is disrupted by large gravitational forces, leaving the constituents supported by "degeneracy pressure" alone. This exotic form of matter is known as degenerate matter. In white dwarfs atoms are held apart by electron degeneracy pressure. In neutron stars, subject to even stronger gravitational forces, electrons have merged with protons to form neutrons. Neutrons are capable of producing an even higher degeneracy pressure, albeit over a shorter range. This can stabilize neutron stars from further collapse, but at a smaller size and higher density than a white dwarf. Neutrons are the most "rigid" objects known; their Young modulus (or more accurately, bulk modulus) is 20 orders of magnitude larger than that of diamond. However, even this enormous rigidity can be overcome by the gravitational field of a massive star or by the pressure of a supernova, leading to the formation of a black hole.
In my mental musings over the past few days it appears to me that the most crucial component of e=mc^2 is actually the distance c. This distance bears a direct relationship to Planck scales which is critical to the understanding of forces in the universe.We can rewrite this as e=m(Planck length)^2.
Quote from: jeffreyH on 09/10/2013 10:13:39In my mental musings over the past few days it appears to me that the most crucial component of e=mc^2 is actually the distance c. This distance bears a direct relationship to Planck scales which is critical to the understanding of forces in the universe.We can rewrite this as e=m(Planck length)^2.That "c" is the speed of light, which is not a distance.