Physics · Glossary

What is The Coulomb barrier?

Also known as: Coulomb barrier · plasma

Definition 33.18 High School Physics · Chapter 33 — Nuclear Energy: Fission, Fusion, E=mc2

Two nuclei are both positive: to touch, they must first climb the hill of their electric repulsion (Chapter 14) — the Coulomb barrier. Only near 1×108K1 \times 10^{8}\,\mathrm{K} do collisions carry the energy to cross it; the fuel is then a plasma of bare nuclei and electrons. Fission pays no such toll: its trigger, the neutron, is neutral, and works cold.

Examples

Example 33.19 (The Sun runs on it)

The Sun’s core, at 1.5×107K1.5 \times 10^{7}\,\mathrm{K}, fuses ordinary hydrogen step by step — the proton–proton chain, of net effect 411H24He+2+10e+radiation4\,{}^{1}_{1}\mathrm{H} \to {}^{4}_{2}\mathrm{He} + 2\,{}^{0}_{+1}\mathrm{e} + \text{radiation}, about 26MeV26\,\mathrm{MeV} per helium: 0.7%0.7\% of the hydrogen’s mass leaves as energy. The sunlight whose spectrum we read in Chapter 2 is this mass, arriving eight minutes late; every star shines by walking the curve toward iron.

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