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ProfRob
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The diproton is in fact unstable. The two protons must have anti-aligned spins and the spin-dependence of the strong force leaves it unbound. In order for fusion to occur, the protons must get close together and one of them must undergo a weak interaction and change into a neutron (and form a bound deuteron with aligned proton and neutron spins). It is this combination that is very unlikely.

The Coulomb repulsion alone is not a particularly high barrier to fusion. For example, the fusion of two deuterons will occur at temperatures an order of magnitude lower than the fusion of protons inside a star, despite identical Coulomb repulsion.

The diproton is in fact unstable. In order for fusion to occur, the protons must get close together and one of them must undergo a weak interaction and change into a neutron. It is this combination that is very unlikely.

The Coulomb repulsion alone is not a particularly high barrier to fusion. For example, the fusion of two deuterons will occur at temperatures an order of magnitude lower than the fusion of protons inside a star, despite identical Coulomb repulsion.

The diproton is in fact unstable. The two protons must have anti-aligned spins and the spin-dependence of the strong force leaves it unbound. In order for fusion to occur, the protons must get close together and one of them must undergo a weak interaction and change into a neutron (and form a bound deuteron with aligned proton and neutron spins). It is this combination that is very unlikely.

The Coulomb repulsion alone is not a particularly high barrier to fusion. For example, the fusion of two deuterons will occur at temperatures an order of magnitude lower than the fusion of protons inside a star, despite identical Coulomb repulsion.

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ProfRob
  • 136.4k
  • 16
  • 302
  • 486

The diproton is in fact unstable. In order for fusion to occur, the protons must get close together and one of them must undergo a weak interaction and change into a neutron. It is this combination that is very unlikely.

The Coulomb repulsion alone is not a particularly high barrier to fusion. For example, the fusion of two deuterons will occur at temperatures an order of magnitude lower than the fusion of protons inside a star, despite identical Coulomb repulsion.