Neutron Star to Black Hole Via OMG?

In summary, a neutron star can potentially transform into a black hole through a process known as OMG (Oppenheimer, Snyder, and Mitra mechanism). This occurs when the neutron star, which is already incredibly dense and has a strong gravitational pull, collapses even further due to the accumulation of mass. This increased density and gravitational force can eventually overcome the neutron star's neutron degeneracy pressure, causing it to collapse into a singularity, thus becoming a black hole. This process is still not fully understood and remains a topic of ongoing research and debate in the scientific community.
  • #1
Islam Hassan
237
5
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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  • #2
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.
 
  • #3
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
 
  • #4
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?
 
  • #5
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.
 
  • #6
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.
 
  • #7
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?
 
  • #8
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.
 
  • #9
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?
 

FAQ: Neutron Star to Black Hole Via OMG?

1. What is a neutron star?

A neutron star is a type of celestial object that forms when a massive star dies in a supernova explosion. It is incredibly dense, with a mass greater than our sun packed into a sphere less than 20 kilometers in diameter.

2. How does a neutron star turn into a black hole?

A neutron star can turn into a black hole if it accumulates enough mass through accretion or merging with another neutron star. Once the mass of the neutron star surpasses a certain threshold, known as the Chandrasekhar limit, it will collapse under its own gravity and form a black hole.

3. What is the process of a neutron star turning into a black hole called?

The process of a neutron star turning into a black hole is called gravitational collapse. This is when the core of the neutron star collapses under its own gravity, creating a singularity and forming a black hole.

4. What is the significance of "OMG" in the phrase "Neutron Star to Black Hole Via OMG"?

"OMG" stands for Oppenheimer, Volkoff, and Snyder, the names of the scientists who first proposed the concept of neutron stars and black holes in the 1930s. This phrase is often used to describe the process of a neutron star turning into a black hole as it pays homage to these pioneering scientists.

5. Can a neutron star turn into a black hole without a supernova explosion?

It is unlikely for a neutron star to turn into a black hole without a supernova explosion. The supernova explosion provides the necessary energy and pressure to initiate the gravitational collapse of the neutron star's core. However, there have been some theories proposed that suggest it may be possible for a neutron star to directly collapse into a black hole without a supernova explosion under certain conditions.

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