Lifespan of Neutrons Adhering Together

  • Thread starter jayaramas
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In summary: They're composed of neutrons and they have a lot of protons but not enough electrons, so they're superconducting.
  • #1
jayaramas
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life of a single free neutron is nearly 15 min. what is the life if 2 are more neutrons adhering together? will it increase or same?
 
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  • #2
Two or more neutrons don't adhere together unless you add some protons. If you add protons, you get atomic nuclei, and each nucleus has its own stability, which you can look up.
 
  • #3
if neutrons are not adhering, how can there be a neutron star?
 
  • #4
A neutron star has so many neutrons they are held together by gravity!
 
  • #5
so, how is the life of neutron star more than a free neutron?
 
  • #6
Well, I don't understand the maths, but the neutrons in a neutron star are prevented from collapsing indefinitely by what is called degeneracy pressure. This results from the Pauli exclusion principle - neutrons are fermions so no two can exist in the same state. The same condition applies to the protons and electrons they would have to decay into, and it must turn out that those states would have higher energy.

Actually, thinking about this now prompts a question in my mind: are neutron stars composed solely of neutrons, or are there still a limited number of proton and electron states available, with the numbers in each state determined by the respective energy levels?
 
  • #7
AdrianTheRock said:
Well, I don't understand the maths, but the neutrons in a neutron star are prevented from collapsing indefinitely by what is called degeneracy pressure. This results from the Pauli exclusion principle - neutrons are fermions so no two can exist in the same state. The same condition applies to the protons and electrons they would have to decay into, and it must turn out that those states would have higher energy.

Actually, thinking about this now prompts a question in my mind: are neutron stars composed solely of neutrons, or are there still a limited number of proton and electron states available, with the numbers in each state determined by the respective energy levels?

In the core of a neutron star there are a few percent electrons and protons. This is why the core is superconducting. I imagine that the percentage decreases towards the center of the star.

According to the experts the neutrons are a superfluid, the protons are a superfluid, the electrons are an ordinary fluid. How they can be a superfluid I don't know.
 
  • #8
The neutrons will do Cooper pairing with each other, and likewise with the protons. http://physicsworld.com/cws/article/news/45296

Cooper pairing is what's behind metal superconductivity and He-3 superfluidity.Neutron stars' neutrons don't decay because they are in equilibrium with the surrounding protons and electrons, just like neutrons in stable nuclei.

Neutron stars' protons are balanced out by their electrons, and that affects their composition. In a neutron-star interior, if protons were about as abundant as neutrons, the electrons would be squeezed together enough to bump their Fermi energies up to something not much less than proton and neutron rest masses. This tips the balance in favor of neutrons, and a neutron star's interior is thus mostly neutrons.

A nontechnical intro to NS's in general: Neutron stars
 

Related to Lifespan of Neutrons Adhering Together

1. What is the lifespan of neutrons adhering together?

The lifespan of neutrons adhering together varies depending on the specific circumstances and environment. In free space, the average lifespan is about 880 seconds (or around 14 and a half minutes). However, in the nucleus of an atom, the lifespan can be significantly shorter due to the presence of other particles.

2. How do neutrons adhere together?

Neutrons adhere together through the strong nuclear force, which is one of the four fundamental forces in physics. This force acts between nucleons (protons and neutrons) and is responsible for holding the nucleus of an atom together. The strong nuclear force is incredibly powerful but only acts over very short distances.

3. What happens to the lifespan of neutrons adhering together in different elements?

The lifespan of neutrons adhering together can vary depending on the element they are a part of. This is because the number of protons and neutrons in an atom affects the stability of the nucleus. Elements with a higher number of protons and neutrons tend to have shorter lifespans for their neutrons, while elements with a more balanced number of nucleons may have longer lifespans.

4. Can the lifespan of neutrons adhering together be extended?

Yes, the lifespan of neutrons adhering together can be extended through nuclear reactions such as fission and fusion. In these reactions, the nuclei of atoms split apart or combine, releasing energy and potentially creating new elements. This process can also result in the creation of more stable isotopes with longer-lived neutrons.

5. How does the lifespan of neutrons adhering together impact nuclear reactions?

The lifespan of neutrons adhering together plays a crucial role in nuclear reactions. In fission reactions, the lifespan of a neutron can determine if it will cause a chain reaction and release more energy. In fusion reactions, the lifespan of neutrons can affect the stability of the resulting element and whether or not it will undergo further reactions. Understanding the lifespan of neutrons is essential in controlling and harnessing nuclear energy.

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