Neutron Star to Black Hole Via OMG?

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Discussion Overview

The discussion revolves around the hypothetical scenario of a high-energy particle, specifically the OMG particle, impacting a neutron star and its potential to initiate the formation of a black hole. Participants explore the conditions under which a neutron star might transition to a black hole, focusing on mass, density, and the implications of particle impacts.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • One participant suggests that the impact of an OMG particle could create sufficient density to initiate an embryonic black hole that might consume the neutron star.
  • Several participants argue that a neutron star requires a significant increase in total mass to become a black hole, implying that a single high-energy proton is unlikely to suffice.
  • There is a discussion about the necessity of both mass and density, with some participants questioning whether local peak density from the particle impact could lead to a mini-black hole.
  • One participant posits the idea of a neutron star being "one neutron short" of becoming a black hole, prompting further exploration of the implications of particle capture by dense objects.
  • Another participant emphasizes that energy density alone is insufficient for black hole formation, insisting that total mass is the critical factor.
  • There is a contention regarding the conditions under which compression could lead to black hole formation, with references to the Schwarzschild radius and the importance of density in this context.

Areas of Agreement / Disagreement

Participants express differing views on the conditions necessary for a neutron star to become a black hole, with no consensus reached on the role of high-energy particle impacts or the sufficiency of mass versus density. The discussion remains unresolved with multiple competing perspectives.

Contextual Notes

Participants highlight the complexity of the conditions required for black hole formation, including the interplay of mass, density, and external factors. There are references to astrophysical constraints and implications for dark matter, but these remain speculative and not fully resolved within the discussion.

Islam Hassan
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If a super-duper-hyper-energetic particle like the OMG particle (refer http://en.wikipedia.org/wiki/Oh-My-God_particle) were to impact the surface of a neutron star, could the tremendous impact density it creates lead to the beginnings of an embryonic black hole that would (slowly/quickly?) swallow the neutron star?

IH
 
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In order for a neutron star to turn into a black hole it needs to add sufficient mass. It is highly unlikely one high energy proton would do the job.
 
mathman said:
In order for a neutron star to turn into a black hole it needs to add sufficient mass. It is highly unlikely one high energy proton would do the job.

Sufficient mass within a sufficiently small volume, ie sufficient density too, no? In that case, would the local peak density created by the particle impact be sufficient to initiate a mini-black hole and the "gobbling" up of adjacent (and very high-density) matter of the neutron star by such mini-BH? In that case, the embyonic BH may graduate to higher status via gobbling up of more and more neutron star matter.

IH
 
mathman said:
In order for a neutron star to turn into a black hole it needs to add sufficient mass. It is highly unlikely one high energy proton would do the job.
What if the neutron star is one neutron short of a black hole?
 
Jimmy Snyder said:
What if the neutron star is one neutron short of a black hole?

Unusual, but not ridiculously absurd. However what's the point? What exactly are you trying to ask?

However you have stumbled upon an important astrophysical constraint on the spatial density of heavy particles, by looking at the implications of their capture by degenerate objects. Both white-dwarfs and neutron stars have been studied carefully in this fashion to see what they tell us about Dark Matter and other cosmic exotica. If too much Dark Matter was captured, then more white-dwarfs would supernova and more neutron stars would become black holes.
 
Islam Hassan said:
Sufficient mass within a sufficiently small volume, ie sufficient density too, no?

No. You need sufficient total mass. Energy density won't make a difference.

I suppose you could have a neutron star that is right at the tipping point, at which point you could sneeze and it turns into a black hole, but that seems unlikely since you have stuff falling into neutron stars constantly.

In that case, would the local peak density created by the particle impact be sufficient to initiate a mini-black hole and the "gobbling" up of adjacent (and very high-density) matter of the neutron star by such mini-BH?

No. That's a misconception. Black holes don't gobble things up. Things fall into black holes, but things fall onto the earth.
 
twofish-quant said:
No. You need sufficient total mass. Energy density won't make a difference.

I thought you could compress something far enough to cause it to turn into a black hole?
 
twofish-quant said:
No. You need sufficient total mass. Energy density won't make a difference.
That is not accurate. A Black-hole results anytime the rest-mass is confined to a region smaller than the Schwartzschild radius for that mass. If there are other important factors (e.g. charge, spin), then there are analogous results---its always a question of density.
Clearly there is more than a black-hole's worth of mass in the galaxy... yet its not a black-hole, because its low density.
 
Twofish, were you saying that if the impact location was already so close to forming a black hole that the impact would cause it to collapse, then there would be way too much mass overall in the star for it to not be a black hole already?
 

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