What Happens to Matter Before a Black Hole Collapses?

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Discussion Overview

The discussion revolves around the processes and phenomena occurring to matter before it collapses into a black hole. Participants explore theoretical implications, the nature of stellar collapse, and the limits of current understanding in astrophysics.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • One participant questions the certainty of astrophysicists regarding the inevitability of black hole formation from stars with critical mass, suggesting the possibility of other types of stellar collapse beyond white dwarfs and neutron stars.
  • Another participant notes that while general relativity predicts collapse to a point, quantum theory introduces conflicts that remain unresolved.
  • It is proposed that time distortion near a black hole's event horizon may prevent the collapse from being observed as reaching a singularity from an external perspective.
  • A participant explains that if a star's mass is insufficient, electron degeneracy pressure can stabilize it as a white dwarf or neutron star, while excessive mass leads to collapse into a black hole due to overwhelming gravitational forces.
  • One participant expresses uncertainty about their understanding of astrophysics but believes their explanation of degeneracy pressure is accurate.

Areas of Agreement / Disagreement

Participants express differing views on the nature of stellar collapse and the implications of mass on the formation of black holes. There is no consensus on the certainty of current theories or the existence of alternative collapse scenarios.

Contextual Notes

Participants acknowledge limitations in current theories, particularly regarding the interplay between general relativity and quantum mechanics, as well as the conditions under which different forms of stellar remnants may exist.

japam
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My question is related to black holes, well there are many books and writings that explain what a black hole is and all AFTER collapse but i have seen few that explains the BEFORE collapse; exactly how is that matter can be squeezed to an infintesimal point, ¿what effects could one expect to see before the collapse?
¿why are astrophysicists so sure that if a star has the critical mass , then it would inexorably colapse to a black hole, why can't be that could exist other types of star collapses apart of white dwars and neutron stars?
¿if black holes really exists , doesn't this imply that electrons and all elemental particles can be splittered infinitely ? so they are not elemental
 
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The question of what happens to matter inside a black hole is still open. Collapsing to a point is preducted by general relativity theory, but quantum theory which also has to hold is in conflict.

The densist form of matter outside black holes is that of a neutron star (no electrons). If a neutron star is big enough, its Schwarzschild radius will be greater than the radius of the star. This is the point where current theory breaks down.
 
My understanding is that current theory implies that time would be distorted to such an extent that any collapse that has been initiated could not have proceeded to a singularity relative to us. Collapsing matter would be frozen at the event horizon, from our point of view.
 
japam said:
¿why are astrophysicists so sure that if a star has the critical mass , then it would inexorably colapse to a black hole, why can't be that could exist other types of star collapses apart of white dwars and neutron stars?
l

They believe this because a stars mass (in general) will tell us what a star is composed of - and when it runs out of elements to fuse it will collapse under gravity to form an extremely dense object.
 
If the mass is small enough when the star begins to 'collapse' electrons in the star will get 'claustraphobic' and start vibrating very rapidly, which is known as electron degeneracy, therefore it exerts a pressure pushing outwards, if there is not enough mass (gravity) to counter this, then they live in a cute little equilibrium as a white dwarf or neutron star.

If the star is too massive, then the gravity is too strong and will overcome the pressure of the degeneracy (i think the is neutron degeneracy too) and it will collapse into a black hole.

It's been years since I've read an astrophysics book though, but I am sure that is fairly accurate.
 
That sounds very familiar from some thermal physics lecture last year Riogho!

I think you're correct :)
 

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