Understanding the Effects of Black Hole Collisions

Click For Summary

Discussion Overview

The discussion centers on the effects and dynamics of black hole collisions, exploring the outcomes when black holes of differing masses collide. Participants examine various aspects of these collisions, including the nature of the interaction, potential merging processes, and the implications of gravitational laws.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions whether a high-mass black hole will "suck" a low-mass black hole or if they will merge to form a larger black hole.
  • Another participant emphasizes that the nature of the collision is crucial, asking if it involves direct impact or if the black holes are orbiting each other.
  • Concerns are raised about the potential destruction resulting from such collisions.
  • Some participants note that black hole collisions typically occur through inspiralling rather than direct hits, suggesting that head-on collisions are rare.
  • It is mentioned that when black holes merge, their event horizons combine, and the resulting black hole's surface area must be greater than or equal to the sum of the original black holes' surface areas, referencing Hawking's second law of black hole mechanics.
  • There is a discussion about the concept of "spiraling in," with some participants questioning the applicability of this term and suggesting that black holes should follow conic sections instead.
  • Participants discuss the implications of gravitational radiation in the context of black hole mergers and how this relates to orbital decay.
  • Clarifications are made regarding the definition of conic sections and their relevance to the motion of objects under central forces.
  • One participant expresses confusion about the mathematical complexities involved in calculating areas related to hyperbolas in the context of black hole dynamics.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the dynamics of black hole collisions, particularly concerning the nature of their interactions and the terminology used to describe their motion. There is no consensus on the specifics of how black holes collide or merge.

Contextual Notes

Some discussions involve assumptions about the nature of gravitational forces and the conditions under which black holes interact, which may not be fully resolved. The complexity of the mathematical models and the observational limitations of black hole collisions are also acknowledged.

praveena
Messages
69
Reaction score
1
Hai pf,
I had a doubt? we were well known about black holes still it act as a mysterious one.
Well my question is about collision of two black holes. what happens if a highmass of black hole colloide with lowmass of black hole? Is the highmass black hole will suck the low mass black hole? Or else they two combine to form a massive one?If the gravitation is more for both what will happen?what may be the resultant? Is there any possibility to measure the force excerted in the black hole?
 
Astronomy news on Phys.org
The nature of the collision is key. Is it a direct hit (trajectories of centers coincide), or will the black holes be orbiting each other in the process?
 
  • Like
Likes   Reactions: praveena
Is the destruction will be more?
 
Based on known physics, black hole collisions should occur via inspiralling and head on collisions should be exceedingly rare. The cosmos is a very big place and black holes are vanishingly small on cosmic scales. That aside the consequences should be remarkably similar - the two will coallesce into a combined sum mass black hole. a BH is not a solid body like a star or planet and offers no 'surface' to collide with. There would likely be some nominal increase in accretion disc emissions in a high speed'collision', but, it otherwise is expected to be quite unremarkable. Interstellar collisions are exceptionally rare events, be it stars or black holes. It is highly unlikely any such event between unbound bodies [e.g. other than within gravitationally bound star sytems] has ever been observed.
 
  • Like
Likes   Reactions: Generator Gawl and praveena
Chronos said:
Based on known physics, black hole collisions should occur via inspiralling and head on collisions should be exceedingly rare. The cosmos is a very big place and black holes are vanishingly small on cosmic scales. That aside the consequences should be remarkably similar - the two will coallesce into a combined sum mass black hole. a BH is not a solid body like a star or planet and offers no 'surface' to collide with. There would likely be some nominal increase in accretion disc emissions in a high speed'collision', but, it otherwise is expected to be quite unremarkable. Interstellar collisions are exceptionally rare events, be it stars or black holes. It is highly unlikely any such event between unbound bodies [e.g. other than within gravitationally bound star sytems] has ever been observed.
Thank you.
 
Why "spiraling in"? Black Holes would still obey gravitational laws and so must at least approximate conic sections. "Spirals" don't seem to be possible.
 
  • Like
Likes   Reactions: praveena
HallsofIvy said:
Why "spiraling in"? Black Holes would still obey gravitational laws and so must at least approximate conic sections. "Spirals" don't seem to be possible.
May i know what does the conic section refers?
 
Orbital decay
 
  • Like
Likes   Reactions: praveena
Chronos said:
Orbital decay
Thank you
 
  • #10
When two black holes "collide", they merge, i.e., when they get close enough, their event horizons merge. This happens in accordance with Hawking's second law of black hole mechanics, which means that the surface area of the resulting black hole cannot be smaller than the sum of the surface areas of the original black holes. This is a special case of the second law of thermodynamics, entropy never decreases.

This is state-ot-the-art research stuff for an important astrophysical phenomenon (black hole mergers) that has been, and is being, studied extensively. As a (post)grad student in 1992, I attended a relativity conference, and Kip Thorne gave a talk on this. He said that the race was on for which occur first: 1) LIGO would observe this experimentally; 2) theorists would calculate the details of the expected signal. In 2005, the theorists won, but there still are loads of research calculations that need to be done.

This is very difficult computational stuff; see the Physics Today article "Binary black hole mergers",
http://w.astro.berkeley.edu/~gmarcy/astro160/papers/binary_black_hole_mergers.pdf

This article is intended for folks who have a university physics background, but, by skipping the maths, I think much of the article can be appreciated by a wider audience.

Figure 2 shows a merger.

HallsofIvy said:
Why "spiraling in"? Black Holes would still obey gravitational laws and so must at least approximate conic sections. "Spirals" don't seem to be possible.

What happens in the classical model of a hydrogen atom, i.e., an electron orbiting a proton? The electron spirals into the proton, because the system radiates away energy as electromagnetic radiation. A system of two black holes emits gravitational radiation, hence the in-spiral. This effect has been observed for the orbits of binary pulsars.

praveena said:
May i know what does the conic section refers?

"Conic section" is the name given to a curve that is either a hyperbola, parabola, or ellipse. They are given this name because these are the types of curves that result when planes intersect cones.
 
  • Like
Likes   Reactions: praveena
  • #11
praveena said:
May i know what does the conic section refers?
Chronos said:
Orbital decay
Careful now, I am not sure if Chronos is responding to praveena's post or mine.

"Conic sections" are circles, ellipses, parabolas, and hyperbolas (a single point, single line or two crossed lines are "degenerate" comics).
They are so called because if you slice a cone, at different angles, with a plane, the cross section is some form of "conic section".

It can be shown that an object moving under a central force, that falls off as the distance to that center, squared, with NO other force, moves along a "conic section". In order to get something like a spiral, which is not a conic section, there must be some other force, such as air resistance, that "decays" the orbit.

However, we are talking about black hole collisions. Where would the decaying force come from?
 
  • Like
Likes   Reactions: praveena
  • #12
An orbital decay trajectory is a 3 dimensional conic section.
 
  • #13
George Jones said:
When two black holes "collide", they merge, i.e., when they get close enough, their event horizons merge. This happens in accordance with Hawking's second law of black hole mechanics, which means that the surface area of the resulting black hole cannot be smaller than the sum of the surface areas of the original black holes. This is a special case of the second law of thermodynamics, entropy never decreases.

This is state-ot-the-art research stuff for an important astrophysical phenomenon (black hole mergers) that has been, and is being, studied extensively. As a (post)grad student in 1992, I attended a relativity conference, and Kip Thorne gave a talk on this. He said that the race was on for which occur first: 1) LIGO would observe this experimentally; 2) theorists would calculate the details of the expected signal. In 2005, the theorists won, but there still are loads of research calculations that need to be done.

This is very difficult computational stuff; see the Physics Today article "Binary black hole mergers",
http://w.astro.berkeley.edu/~gmarcy/astro160/papers/binary_black_hole_mergers.pdf

This article is intended for folks who have a university physics background, but, by skipping the maths, I think much of the article can be appreciated by a wider audience.

Figure 2 shows a merger.
What happens in the classical model of a hydrogen atom, i.e., an electron orbiting a proton? The electron spirals into the proton, because the system radiates away energy as electromagnetic radiation. A system of two black holes emits gravitational radiation, hence the in-spiral. This effect has been observed for the orbits of binary pulsars.
"Conic section" is the name given to a curve that is either a hyperbola, parabola, or ellipse. They are given this name because these are the types of curves that result when planes intersect cones.

How can you say that it may be a hyperbola? For hyperbola the two ends become infinity and there is no area existed. while calculating the conic section area, the mathematical expression could become complex?
 
  • #14
praveena said:
How can you say that it may be a hyperbola? For hyperbola the two ends become infinity and there is no area existed. while calculating the conic section area, the mathematical expression could become complex?

Look at the figures

http://math2.org/math/algebra/conics.htm

and imagine that the cones extend up and down forever.
 
  • #15
HallsofIvy said:
Why "spiraling in"? Black Holes would still obey gravitational laws and so must at least approximate conic sections. "Spirals" don't seem to be possible.
I can't understand your above lines? can you explain it detail?
 
  • #16
praveena said:
I can't understand your above lines? can you explain it detail?

Newtonian gravity is an inverse-square force, i.e., its strength is inversely proportion to the square of the distance between the masses. For inverse square forces, unbound orbits are either hyperbolas or parabolas, and bound orbits are ellipses or circles.

Even though this is correct, this does not apply to case of two black holes (unless they are very far apart) for two reasons.

1) Newton's theory of gravity does no apply to the case of two black holes, Einstein's theory of gravity, general relativity, must be used. For Einstein's theory of gravity, orbits are not conic sections. Even bound orbits do not close, they look something like a Spirograph pattern.

2) The above does not take into account radiation. The Coulomb force between an electron and a proton is also an inverse-square force, but (classically) the orbit of an electron is not a conic section, because accelerating charges radiate away energy in the form of electromagnetic radiation. This cause the electron's orbit to spiral into the proton. Similarly, Einstein's theory of gravity predicts that a two-black hole system will emit gravitational radiation, causing orbits to spiral in.
 

Similar threads

  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 11 ·
Replies
11
Views
4K
  • · Replies 27 ·
Replies
27
Views
6K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K