Physics, 23.11.2019 04:31 helpmewithmath70
Planetary orbits around a star can be modeled with the following potentialu(r) =ar+br2(1)(a) show that the equilibrium position for this potential is equal tore= 2b=a.(b) use the taylor expansion on the potential about the equilibrium position to show thatthe \spring" constant of small oscillations around this equilibrium position isa4=8b3
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Planetary orbits around a star can be modeled with the following potentialu(r) =ar+br2(1)(a) show th...
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