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<p>proton to be added, according to <a href="page.php?w=Coulomb%27s_law">Coulomb's law</a>. In the context of nuclear reactions this is called a <a href="page.php?w=Coulomb_barrier">Coulomb barrier</a>. The higher the Coulomb barrier, the more <a href="page.php?w=kinetic_energy">kinetic energy</a> a proton requires to get close to a nucleus and be captured by it. The average energy of the available protons is given by the <a href="page.php?w=temperature">temperature</a> of the stellar plasma. Even if this temperature could be increased arbitrarily</p><p>
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