Two Protons Colliding- Stable Nuclei?

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    Nuclei Protons Stable
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SUMMARY

Two protons can collide and form a stable nucleus under specific conditions, primarily through the process of proton-proton fusion, which occurs in the sun. This fusion requires substantial energy to overcome the electrostatic repulsion between protons, necessitating temperatures around 15 million K. Once the protons are close enough, the strong nuclear force can bind them together, resulting in stable nuclei such as deuterium and helium. Quantum tunneling also plays a crucial role, allowing protons to bypass energy barriers that would otherwise prevent fusion.

PREREQUISITES
  • Understanding of strong nuclear force and electrostatic repulsion
  • Basic knowledge of nuclear fusion processes
  • Familiarity with quantum mechanics concepts, particularly quantum tunneling
  • Knowledge of temperature scales relevant to nuclear reactions
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  • Research the process of proton-proton fusion in stellar environments
  • Study the role of quantum tunneling in nuclear reactions
  • Explore the conditions necessary for nuclear fusion on Earth
  • Investigate the stability of various isotopes, including deuterium and helium-4
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Students of physics, particularly those studying nuclear physics, astrophysicists, and anyone interested in the mechanisms of stellar fusion and nuclear stability.

axel65
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Hi, I'm new to this forum, so I'm sorry if I've posted this in he wrong catergory.

Anyway, I'm studying AS physics at the moment and my teacher was giving the class some lessons about the strong nuclear force and electrostatic repulsion of nucleons making the nucleus stable.

To get to the point, we started woundering whether two protons could collide with each other, providing they had sufficient energy, to become a stable nuclei- i.e. the protons could get close enough for the electrostatic repulsion and the strong nuclear force to balance. The physics teacher was unsure, and the chemistry teacher told me it wasn't possible, but didn't have time to give an explanation, so I still don't understand why. Can anybody help me out? :confused:

Thanks, Alex
 
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Yes, they can.

It takes substantial energy - but it does happen, it's just difficult to achieve on earth.

However, the process of proton-proton fusion is one of the key reactions that takes place in the sun. 2 Hydrogen nuclei (protons) fuse to produce a deuterium nucleus (1 proton, 1 neutron) and a positron (positive electron). Subsequently, the deuterium nuclei can fuse with protons to form helium.

The electrostatic force provides substantial repulsion, hence the need for very high temperatures (about 15 million K). It is only at high temperatures that the KE of the protons is sufficient to overcome the electrostatic repulsion.

However, once you overcome electrostatics then the strong force will bind the 2 nucleons together - and produce a new nucleus. In the case of deuterium, and helium-3 and helium-4 the nuclei are stable. Tritium can also be produced, this is unstable and decays into helium-3.

There is a final catch - in that the temperatures of the sun aren't quite high enough to overcome the electrostatic repulsion between protons, so how can the reaction take place.

The solution is 'quantum tunneling' - A simple explanation: according to classical physics, if a particle doesn't has less energy than a barrier then the barrier acts like a brick wall - the particle can't cross it. In quantum mechanics, things are probability based - it's possible, for a particle to cross any barrier - the height of the barrier and the energy of the particle determine the probability that particle can cross. Occasionally, this means a particle can cross a barrier that is higher than its energy level - the particle appears to 'tunnel' through the barrier, instead of going over it.
 

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