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Fusion in the sun
•Have lots of hydrogen (p+ and e-) – what can we make from it?
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•If  2He (2 protons, 0 neutrons) were stable, fusion would be “easy”
–Run two protons into each other at fast enough to overcome Coulomb repulsion
–Once they get close enough strong force takes over, and holds them as nucleus
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•“Unfortunately” 2He isn’t stable
–To get stable He need to add one or two neutrons to:
•Increase Strong Force, without increasing Coulomb force
–Not really “unfortunate” – If 2He were stable:
•Sun would burn energy way too fast – and would have gone out by now
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•Weak force converts proton to neutron–fusion will be slow
–In solar fusion no excess neutrons lying around
–Hydrogen bombs use deuterium: 2H = (p+ n) or tritium:  3H = (p+ n n) to provide it