A long time ago, in a galaxy far, far away, electric charge had not yet been invented, and atoms were held together by gravitational forces. Compute the Bohr radius (a0) and the
n = 5 to n = 4
transition energy
(E5 − E4)
in a gravitationally bound hydrogen atom.
a0 |
= m |
E5 − E4 |
= eV |
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