Why is Proton Radiation this Rare in Nuclear Fission Decay?

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SUMMARY

Proton radiation is rare in nuclear fission decay, primarily due to the energetics involved in nuclear binding. While beta radiation (electron emission) and neutron radiation occur, alpha radiation (helium ion emission) is favored because alpha particles are tightly bound, requiring less energy to emit compared to protons. The discussion highlights that for proton decay to be energetically favorable, a nucleus must exist that is more stable than the proton, which is not typically the case. Instead, alpha decay is more common due to the lower energy threshold associated with helium-4 nuclei.

PREREQUISITES
  • Understanding of nuclear fission processes
  • Knowledge of alpha, beta, and neutron radiation
  • Familiarity with nuclear binding energy concepts
  • Basic principles of quantum mechanics related to nuclear stability
NEXT STEPS
  • Research the energetics of nuclear binding, focusing on binding energy calculations
  • Study the mechanisms of alpha decay and its implications for nuclear fusion
  • Explore the concept of cluster decay and its rarity in nuclear reactions
  • Investigate the role of ligands in nuclear processes, particularly in relation to hydrogen fusion
USEFUL FOR

Physicists, nuclear engineers, and researchers interested in nuclear decay processes and fusion energy. This discussion is particularly beneficial for those studying the energetics of nuclear reactions and the stability of atomic nuclei.

consuli
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The atomic nuclei consist out electrons, protons and neutrons (with only exception of hydrogen, that does have a neutron).

Thus, it would be straightforward, that there existed a corresponding radiation for each nucleus component, when a nucleus decays.

There is an electron radiation (beta radiation).

There is a neutron radiation.

But proton radiation is very rare. Instead there is usually alpha radiation in nuclear fission decay, which is an accelerated helium ion.

On the other hand, the element hydrogen (one proton + one electron) is much more common than helium. Thus, a single proton nucleus cannot be too unstable.

What is the quantum-mechanic explanation for there is helium-ion radiation (alpha radiation) instead of proton radiation, when a nucleus gets fissioned?
 
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Both proton and neutron emission from a single nucleus are rare, usually these nuclei do beta decays.
Fission releases neutrons as heavier nuclei are more neutron-rich than the stable or long-living isotopes of the fission products.

Alpha particles are quite tightly bound for a light nucleus, their emission is favorable in terms of energy. Often nuclei can emit an alpha particle but not a proton or a neutron.
 
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consuli said:
What is the quantum-mechanic explanation for there is helium-ion radiation (alpha radiation) instead of proton radiation, when a nucleus gets fissioned?

mfb said:
Alpha particles are quite tightly bound for a light nucleus, their emission is favorable in terms of energy.

Would you say this graph is a good visualization for the alpha emission being "favorable in terms of energy?" According to the graph the alpha/helium-4 nuclei has less mass per nuclear particle than the proton.

mass-per-particle.jpg
 

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Yes.
The emission of larger nuclei like carbon can release even more energy but it is less likely that so many nucleons leave at the same time. It is called cluster decay and a very rare phenomenon.
 
consuli said:
What is the quantum-mechanic explanation for there is helium-ion radiation (alpha radiation) instead of proton radiation, when a nucleus gets fissioned?

Mfb is right. You need to think about energetics. Typical binding energies are 8 MeV/nucleon. For proton decay to be energetically favorable, that means there neds to be nucleus one proton away that is bound by more than than that. An alpha, however, is already bound by 7 MeV per nucleon. So you only need to find a nucleus 2 protons and 2 neutrons away bound by 4 MeV more. ( [8 MeV - 7 MeV] * 4 nucleons)
 
To get this straight. Because a proton (hydrogen-ion) does contain too much nuclear energy, a less energized helium-ion is released instead, right?

Does that also imply, I could study alpha-decay for the reason how to easierst start a nuclear fusion process of hydrogen-ion (deuterium-ion) ? Spoken otherwise, would liganding hydrogen (deuterium) to an atomic mass number heavy metal effectively be the easierst way to produce a hydrogen (deuterium) fusion to helium (ion)?
 
It's a statement about the energy difference between the parent and daughter nuclei.

I don't know what "liganding" is in this context.
 
consuli said:
The atomic nuclei consist out electrons, protons and neutrons

No, it consists of protons and neutrons (except the hydrogen-1 nucleus which is just a protons). The fact that some nuclei can emit electrons in beta decay does not mean the electrons are constituent particles of nuclei.
 
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consuli said:
Does that also imply, I could study alpha-decay for the reason how to easierst start a nuclear fusion process of hydrogen-ion (deuterium-ion) ? Spoken otherwise, would liganding hydrogen (deuterium) to an atomic mass number heavy metal effectively be the easierst way to produce a hydrogen (deuterium) fusion to helium (ion)?
No. Why should something fuse with something else just because some heavy atom is nearby?
 

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