How come stable isotopes have more neutrons than protons?

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SUMMARY

The discussion centers on the relationship between neutrons and protons in stable isotopes, emphasizing that stable nuclei often contain more neutrons than protons due to the balance of nuclear forces. The nuclear force, which binds nucleons together, diminishes more rapidly with distance than the Coulomb force, which repels protons. As nuclei increase in size, a greater number of neutrons is required to counteract the repulsive forces among protons, ensuring stability. Additionally, an excess of neutrons can lead to instability as free neutrons decay into protons, further complicating the stability of larger nuclei.

PREREQUISITES
  • Understanding of nuclear forces and Coulomb repulsion
  • Familiarity with the concept of isotopes and nuclear stability
  • Basic knowledge of fermions and quantum states
  • Awareness of nuclear decay processes
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  • Study the stability of isotopes using the liquid drop model
  • Explore the concept of neutron-to-proton ratios in different elements
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Students of nuclear physics, physicists interested in nuclear stability, and anyone seeking to understand the fundamental forces governing atomic structure.

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So, watching the chart of isotopes (or nuclides), where I have isotopes put according to how stable they are, I have seen that the stable elements have more neutrons than protons.

And I wonder why that is?

Is it because neutrons are responsible for binding the nucleus with nuclear force (because protons would just repel each other due to Coulomb force), and contribute to higher binding energy or is it something else?

I'm taking nuclear physics class, but we only deal with mathematical side like transitional matrix elements and quadrupole moment etc. Plus the professor is kinda boring. And I'd like some nice explanations to why some things are. So if you can help me understand this a bit better I'd be grateful :)
 
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There are a lot of ways to answer this question but the bottom line is that the nuclear force dies off quicker as a function of distance than does the electric force. With a larger nuclear radius, opposite sides are farther apart and therefore the electric force repelling protons is, per nucleon, stronger than the nuclear force attracting everything. To get a stable nucleus, you have to compensate for this by adding more neutrons so that that total nuclear binding force balances the repellant force. If you look closely, stable elements with small diameters (He, Li, etc.) have roughly equal amounts of neutrons and protons. As you go to bigger and bigger nuclei, you need disproportionally more neutrons to keep the nucleus stable.
 
So basically it's all because of the force, that is competition between Coulomb repulsion and nuclear force.

Thanks for the clarification :)
 
Also, note that for lighter elements, isotopes with equal numbers of protons and neutrons are typically stable, as is Helium-3 (and, trivially, Hydrogen-1).
 
Hmm, this explains why too few neutrons is unstable, but why is too many neutrons unstable?
 
Khashishi said:
Hmm, this explains why too few neutrons is unstable, but why is too many neutrons unstable?

I am guessing, but it may be related to the fact that free neutrons are unstable.
 
Protons and neutrons are fermions, therefore they cannot have identical quantum numbers in the nucleus. This means that only two neutrons can occupy the lowest state (with spin up and down), the following two neutrons have to use a state with higher energy and so on. If you have too many neutrons and too few protons, the highest occupied neutron state has a higher energy than the lowest free proton state (plus electron plus neutrino energy), and a neutron can decay into a proton.
This is the main reason why the total number of stable nuclei with fixed sum of protons+neutrons is very small - usually just one. The coulomb forces just increase the proton energy levels a bit and therefore reduce the proton to neutron ratio for large nuclei, but they do not make every nucleus with some additional protons unstable.
 

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