Nucleus stability: Neutron & Proton Ratio

In summary, the stability of an atom depends on the ratio of protons to neutrons in its nucleus. Single neutrons are unstable when they are alone, but in a nucleus, they contribute to the strong force that holds protons together. However, as more neutrons are added, the nucleus reaches a point where it has excess energy and needs to release it, resulting in the decay of the atom. This is due to the exclusion principle and the electrical interaction between protons, which becomes unfavorable as more protons are added. This explains the curved shape of the line of stability for heavy nuclei.
  • #1
quinteboy
2
0
Hi

I'm looking for a good description (high-school to 1st year level) why the ratio of protons to neutrons matters for stability. Single neutrons are unstable, but in a nucleus they are stable and the more nucleons you have the greater the strong force. So why can't you have stable isotopes say uranium where excess neutrons increase the binding energy per nucleon ratio to a point to make the atom stable?
 
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  • #3
Here is my possibly incorrect understanding:

A neutron is made up of 1 up quark and 2 down quarks. Down quarks are slightly more massive than up quarks. Matter in general wants to be in the lowest energy state it can be in. Normally, when the neutron is in free space (Not in a nucleus), there is no reason for it to stay in that slightly more energetic form, therefore it decays into a proton, which is made up of 2 up quarks and 1 down quark, in order to reach that lower energy state. (As far as we know Protons are completely stable and never decay at normal temps/energies)

Now, an atomic nucleus requires neutrons to provide extra Strong Force to hold protons together against their repulsive positive charges. Staying together inside a nucleus means that the protons and neutrons have a lower combined energy than their combined individual energies if they were alone by themselves. Once you start adding neutrons to a nucleus, you reach a certain point, which varies with each different element, that the energy of the nucleus exceeds that breakeven limit and the nucleus now wants to do something to reach a lower level of energy. It does this by decaying by the various methods to form another element. One of these is the Beta decay method, which is also the exact method that a free neutron decays into a proton while by itself in space.

Hope this helps.
 
  • #4
Thanks for your responses, I think I understand (enough) what's happening :approve:
 
  • #5
Yea, Drakkith's reasoning appears correct.
 
  • #6
Drakkith's argument doesn't seem correct to me, because it never invokes the exclusion principle, and I don't think you can explain this without the exclusion principle. Also, it invokes the mass difference between up and down quarks, which I don't think is necessary in order to understand why the line of stability has the general shape it does. (The low-mass line of stability is N=Z, so clearly the asymmetry in mass doesn't matter there.)

First let's consider the case without electrical interactions, which is relevant for low masses. If you add more and more neutrons, you have to put them in states more and more energy, because the low-energy states are full. Same if you add more and more protons. At any given point as you're filling the states, your best option is to add a neutron if the lowest empty state is a neutron state, a proton if the lowest is a proton state.

For heavy nuclei, the line of stability curves away from N=Z. This is because of the electrical interaction, which is unfavorable to adding more protons.
 
  • #7
bcrowell said:
Drakkith's argument doesn't seem correct to me, because it never invokes the exclusion principle, and I don't think you can explain this without the exclusion principle. Also, it invokes the mass difference between up and down quarks, which I don't think is necessary in order to understand why the line of stability has the general shape it does. (The low-mass line of stability is N=Z, so clearly the asymmetry in mass doesn't matter there.)

First let's consider the case without electrical interactions, which is relevant for low masses. If you add more and more neutrons, you have to put them in states more and more energy, because the low-energy states are full. Same if you add more and more protons. At any given point as you're filling the states, your best option is to add a neutron if the lowest empty state is a neutron state, a proton if the lowest is a proton state.

For heavy nuclei, the line of stability curves away from N=Z. This is because of the electrical interaction, which is unfavorable to adding more protons.

That's pretty much what my post was saying, but not in so elequant language. =)
 

1. What is the neutron and proton ratio in a nucleus?

The neutron and proton ratio in a nucleus is the number of neutrons divided by the number of protons in the nucleus. This ratio can vary depending on the element and is an important factor in determining the stability of a nucleus.

2. How does the neutron and proton ratio affect nucleus stability?

The neutron and proton ratio plays a crucial role in determining the stability of a nucleus. Nuclei with a higher neutron to proton ratio tend to be more stable, as the extra neutrons help to balance out the repulsive force between protons. However, if the ratio becomes too high, the nucleus can become unstable and undergo radioactive decay.

3. What is the ideal neutron and proton ratio for a stable nucleus?

The ideal neutron and proton ratio for a stable nucleus varies depending on the element, but typically falls between 1:1 and 1.5:1. This means that for every proton, there should be at least one neutron and up to one and a half neutrons to maintain stability.

4. Can the neutron and proton ratio be changed in a nucleus?

Yes, the neutron and proton ratio in a nucleus can be changed through nuclear reactions. For example, in nuclear fission, the nucleus of an atom is split into smaller fragments, changing the ratio of neutrons and protons. Similarly, in nuclear fusion, two nuclei combine to form a larger nucleus, altering the ratio.

5. How do scientists study and measure the neutron and proton ratio in a nucleus?

Scientists use a variety of experimental techniques to study and measure the neutron and proton ratio in a nucleus. One common method is through mass spectrometry, which measures the mass of different isotopes of an element to determine the neutron and proton ratio. Other techniques include nuclear reactions and scattering experiments.

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