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Black hole vs Black hole 
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#1
Jan213, 05:51 AM

P: 69

What happens when a black hole devours another black hole? The bigger eats the smaller and increases in mass and size? What happens with the singularities?



#2
Jan213, 07:22 AM

P: 44

The black holes undergo inspiral motion: their orbit decays through gravity wave emission, and then they are thought to merge. The merging phase is very brief (few miliseconds), produces another black hole, and understood primarily through numerical simulations.



#3
Jan213, 01:53 PM

Mentor
P: 11,833

I think Stargazer is correct. The two would merge and exist as one black hole with a mass equal to the mass of the two prior to merger.



#4
Jan213, 04:12 PM

P: 384

Black hole vs Black hole
The end result should generally be a Kerr or Newman black hole. So are the initial black holes (a Schwarzschild or Nordström black hole is the limiting case of a Kerr or Newman black hole of no diametre.)
But what happens to the topology of the ring singularities inside the common event horizon during the merger? Can a ring singularity be, for example, snapped into a singularity with loose ends? Or what happens, geometrically, on a triple junction of two loops of singularities after the two rings have touched? 


#5
Jan313, 06:01 AM

P: 69

"But what happens to the topology of the ring singularities inside the common event horizon during the merger? Can a ring singularity be, for example, snapped into a singularity with loose ends? Or what happens, geometrically, on a triple junction of two loops of singularities after the two rings have touched? " Nicely formulated. This would be the second question. 


#6
Jan613, 03:56 PM

Sci Advisor
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#7
Jan2713, 08:41 PM

P: 193

But what about a black hole colliding with an antimatter black hole?
Does antimattermatter annihilation destroy the mass of both? If yes the collision product should cease being a black hole and remnants would stream out, But wait! Would the radiation produced by annihilation gravitate as much as the mass would? Can we have a radiation only black hole? But wait wait! Because time is frozen at the event horizons maybe the mater and antimatter will never come in contact in finite time. Then it would be no different than two matter black holes merging. It makes my head hurt to think of such things. 


#8
Jan2713, 08:47 PM

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#9
Jan2713, 09:27 PM

P: 193

Whoops, allow me to rephrase.
But wait wait! Because time is frozen at the event horizons maybe to an outside observer the mater and antimatter will never come in contact in finite time. No annihilation would occur in finite time as seen by an external observer. Then it would be no different than two matter black holes merging. 


#10
Jan2813, 08:46 AM

P: 1,857

An antimatter star could not form in a matter dominated universe, therefore you cannot have an antimatter blackhole to encounter a matter blackhole.



#11
Jan2813, 12:50 PM

Sci Advisor
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Since the matter inside a black hole is crushed to a singularity [in classical theory], it appears the collapsed matter would not retain any of its precollapse properties besides gravity. Another issue would be any hypothetical anti gravity effects between an antimatter and normal matter black hole. How could they merge if they repulse each other? If both possess normal gravity, the singularities would not come into contact until they were inside the event horizon. Given nothing can escape the event horizon, any energy released would be trapped inside the event horizon. On that basis it appears antimatter/matter black hole mergers [if possible] would be indistinguishable from a merger between two matter black holes.



#12
Feb713, 06:35 PM

P: 8

I understand why BH orbits decay generating gravitational waves and I agree that from an external observer the two BH seem to merge into one, but I think that from the BH point of view this does not happen.
What I mean is that the bigger BH inglobates the smaller one, but there should remain a tiny (getting ever smaller) space of regular space between the two horizon surfaces. Lets say that we have two BH with horizons that have radii of 1 meter each. If the two BH are distant their horizons are spherical, because in every point of the space surrounding the BH the gravitational effect of the second BH are very small. Now think of drawing a straight line between the two singularities as the two BHs get closer. Don't stop the line at the singularities but extend it so that exits from the other side of each horizons (the two BHs approach each other in a spiral motion, and the direction of the line changes, but as external observers we can always draw a line joining the two singularities and extending it past them). In any given moment of time particles that are on the external portion of the line (the portion that is not between the black holes) feel the gravitational force of the nearest blackhole AND the other BH, this mean that they need an higher escape speed and the final effect is that the event horizon of the nearest BH further extends in space in the direction opposite to the one by which the second blackhole is approaching. Particles in the internal portion of the line feel the opposite effect: because the gravity from the more distant black hole is partially contributing to pull them away from the nearest one: their escape velocity is reduced, so an external observer should see the horizon receding. A particle that is exactly at the midpoint between the blackholes (since the two have the same size) should always be able to escape with a trajectory perpendicular to the line, no matter which is the distance between the two BHs. The singularities will always approach eachother, but I think they will never really merge, the horizons between the BHs will recede and get flatter almost to perfect circular sections and there should always be some regular space between them. If the two BH have sufficiently different masses the smaller BH will be swallowed by the bigger one, but still they will not merge: there will always be a small region of 'regular' space surrounding the event horizon of the smaller BH. The small blackhole will eventually evaporate into the big one, but this is an extremely long process. 


#14
Feb2613, 05:51 PM

P: 12

I have a few issues concerning black holes and this seems to be an appropriate thread to address them. The following are my understandings, inferences based on those understandings, and a few questions. I would welcome any corrections and answers which you can provide.
1. For a massive star, if one traverses a straight path from the surface toward the center, the strength of the gravitational field steadily increases, reaches a maximum value, near the boundary of the core or perhaps a short distance within the core, then rapidly drops to zero at the center of mass. The locus of points at which this maximum occurs will form a spherical shell, centered at the center of mass of the star. 2. When this star undergoes gravitational collapse, the general shape of the fieldstrength curve remains the same. Although the core collapse proceeds very rapidly and, for a while, leaves the upper layers behind, and this gap may introduce a glitch in the shape of the curve, there will still be a radius at which the field strength is maximal followed by a rapid decline to zero. 3. As the collapse proceeds, the density of the core material increases, the radius of the fieldmax sphere decreases, and, therefore, the maximum field strength increases. When this max field strength reaches the value which corresponds to an escape velocity of C, the fieldmax sphere becomes the event horizon and a black hole is born. [*note below] 4. In subsequent paragraphs, events, observations, and time are as experienced by an Observer at rest well away from the event horizon. 5. My conjecture is that the radius of the event horizon and mass of the black hole are frozen and never, ever change following initial appearance of the event horizon. My understanding is that velocity of any subsequent infalling matter, as seen by the Observer, rapidly declines as it closely approaches the horizon (due to gravitational time dilation) and, in fact, becomes zero at the horizon, never actually entering the black hole. 6. Therefore, although an accretion disk can form and can grow in mass, the Observer can never detect, in principle, actual ingestion of any matter from that disk. In particular, this implies that two black holes can never actually coalesce. 7. Finally, unless a different mechanism for blackhole creation is proposed, all "giant black holes" must actually consist of a dense cluster of separate, but tightly bound, holes. 8. My conjecture, however, seems to contradict what I read in many places about "dynamical" black holes which are undergoing, or have recently undergone, ingestion of infalling material or merger with another hole. My Questions: 1. Is my description of the collapse and the invariance of the initial event horizon correct, and if not, where is my error? 2. If strength of the gravitational field is not the cause of the event horizon (per the note below), then what is? 3. What is the final result, as seen by the Observer, of an "encounter" (I won't say "merger") of (a) a black hole and a 10Solarmass star, and (b) of two black holes? I do see the earlier discussion of this proposing a distortion of the horizons of the approaching holes. But if time (at the horizon as seen by my Observer) essentially stops, would even that distortion be seen? *Note: In a 1994 book by Kip Thorne, I have read about a distinction between the "apparent event horizon" (the one I describe above) and an "absolute event horizon". The latter is said to appear initially as a point at the center of the collapsing star (in "anticipation" of its subsequent phase as a black hole) and then expand as the collapse continues until it reaches the stage that I describe above. Assuming that my description of the fieldstrength curve is correct (zero at the star's center), what then is the condition that precipitates initial formation of the absolute horizon at a point of zero gravity? I hope that someone can supply explanations which do not require a PhD in math to comprehend. Thanks. 


#15
Feb2613, 07:02 PM

PF Gold
P: 171

@ CSSLEmaker
The loophole in your reasoning understandings 58 or so is your assumption that the horizon stays fixed. in fact, it "jumps out" and gobbles up the infalling material. So you don't ever see the infalling material make it through the old event horizon, but it makes it through the new expanded event horizon very quickly. The 'Point" (pun intended) of your note about the black hole starting at a point of zero gravity, is simply a matter of a mathematical definition. The black hole (event horizon) is defined to be the trapped surface, ie the set of points from which a light ray or null geodesic never makes it to future infinity. This set starts with the point right in the center of the black hole and it depends on what happens in the future, and not on the zero force at the point itself at that instant. This is a little bit sloppy, but hopefully you get the idea. Best, Jim Graber 


#16
Feb2613, 09:10 PM

P: 12

to: jimgraber Thanks, Jim, for the quick reply. However, I'm still somewhat dissatisfied. You state that the infalling material isn't seen to pass through the horizon; rather, that the horizon "jumps out" and engulfs the material. But either of these constitutes a change in the relative spatial relationship of the "infalling" material and the horizon, and an absolutely essential dimension of change is time. If it is true that time stops at the horizon as seen by the Observer, and progresses extremely slowly very near the horizon, then it would seem that no such change could be observed.
With respect to the absolute horizon's beginning as a "point", let's alter that a slight amount and consider two epsilons: a tiny elapsed time after the "point beginning" and a consequent tiny increase in the horizon radius. We now are no longer dealing with mathematical abstractions (a dimensionless point, and the instant of time zero), but the problem remains. If the epsilons are small enough, the region will still have very nearly zero net gravity. It would seem that the only escape from this problem is if the horizon depended, not upon the strength of the gravitational field, but somehow directly upon the density of the material at the center. Best regards, Carroll Slemaker 


#17
Feb2713, 12:40 AM

P: 895

you are using the wrong coordinate system. it so happens that t is the coordinate for time in approximately flat spacetimes but that is not necessarily so in other spacetimes. proper time, the time measured by an infalling observer, is unaffected.
let me make an analogy with electromagnetics. I say that magnetic fields are relative and some observers see a magnetic field, and others don't. Ridiculous? No  if you have a point charge and you are stationary with respect to it, it has a uniform radial electrical field and no magnetic field. However, if you change to a moving frame, the charge is actually a CURRENT which creates a magnetic field and simultaneously makes the electrical field nonuniform. A rough analogy can be made for spacetime; what time actually is, depends on where you are and how fast you are moving. 


#18
Feb2713, 01:15 AM

P: 12

Good evening Chill Factor. I must be missing something here. Are you saying that it is impossible in principle to station an observer at a position and in a manner such that he is at rest with respect to the black hole? Am I missing something when I read in the textbooks that to an observer not falling into the black hole and in a location well beyond the strongly curved spacetime near the hole that time will appear to slow in the close vicinity of the hole? Are you saying that if, someday, we discover a black hole within, say, a few hundred lightyears and its orientation is such that with the future's greatly improved space telescopes we can actually resolve the space occupied by the event horizon, that we will, in fact, be able to see infalling matter actually pass through the horizon? I think I understand the electromagnetics you mention, but I'm afraid I cannot see the analogy. But thanks.
Regards, Carroll Slemaker 


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