Neutron stars not sustained by degeneracy force?

Therefore, the remaining strong force is the residual force that sustains the neutron star in a stable state.In summary, the speaker at the talk claimed that neutron stars are sustained by residual strong forces, specifically the exchange of pions. This is in contrast to the mainstream belief that neutron stars are sustained by neutron degeneracy forces. However, both explanations are correct as the nuclear strong force only applies to atomic nuclei and the remaining strong force is what keeps the neutron star stable.
  • #1
dalcde
166
0
I have just attended a talk, where the speaker (a professor in Hong Kong University) claims that neutron stars don't collapse due to "nuclear forces". He further explains that those nuclear forces are residual strong forces (i.e. exchange of pions). However, the mainstream saying (according to Wikipedia) I've heard is that they are sustained by neutron degeneracy forces. Which is correct? And if it is indeed sustained by nuclear force, how does it work since as far as I know, nuclear forces are attractive.
 
Astronomy news on Phys.org
  • #2
Both are correct. The nuclear strong force only applies to atomic nuclei. It is what binds protons to neutrons and quarks to quarks. The pressure in a neutron star is great enough to disassemble atomic nuclei, and protons but, not enough to dismantle neutrons.
 

1. What is a neutron star?

A neutron star is a celestial object that is formed when a massive star dies in a supernova explosion. It is an incredibly dense object, with a mass greater than the sun packed into a sphere with a diameter of only a few kilometers. It is composed almost entirely of neutrons, hence the name "neutron star."

2. How are neutron stars sustained?

Neutron stars are sustained by the degeneracy force, which is a quantum mechanical effect that prevents the neutrons from collapsing under their own gravity. This force is similar to the force that prevents electrons from collapsing into the nucleus of an atom.

3. What happens when a neutron star is not sustained by the degeneracy force?

When a neutron star is not sustained by the degeneracy force, it begins to collapse under its own gravity. This collapse can result in the formation of a black hole, or in some cases, a supernova explosion.

4. How can degeneracy force be overcome?

The degeneracy force can be overcome if the neutron star becomes too massive or if it is affected by an external force, such as a collision with another object. This can cause the star to collapse and potentially form a black hole.

5. Are there any other factors that could cause a neutron star to lose its degeneracy force?

Yes, there are other factors that could cause a neutron star to lose its degeneracy force. For example, if a neutron star is rotating too rapidly, it can lose stability and collapse. Additionally, changes in temperature or density could also affect the degeneracy force and potentially cause the star to collapse.

Similar threads

  • Beyond the Standard Models
Replies
3
Views
2K
  • Atomic and Condensed Matter
Replies
5
Views
1K
  • Astronomy and Astrophysics
3
Replies
77
Views
7K
  • High Energy, Nuclear, Particle Physics
Replies
4
Views
2K
  • Astronomy and Astrophysics
Replies
15
Views
5K
  • High Energy, Nuclear, Particle Physics
Replies
14
Views
3K
  • Astronomy and Astrophysics
Replies
10
Views
4K
  • Astronomy and Astrophysics
Replies
8
Views
5K
Replies
1
Views
3K
  • Astronomy and Astrophysics
Replies
6
Views
5K
Back
Top