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A long time ago, in a galaxy far, far away, electric charge had not yet been invented, and atoms were heid together by gravitational forces. Compute the Bohr radius (ag) and the n=3 to n2 transition energy (E-E) in a gravitationaly bound hydrogen atom. m

A long time ago, in a galaxy far, far away, electric charge had not yet been invented, and atoms were heid together by gravitational forces. Compute the Bohr radius (ag) and the n=3 to n2 transition energy (E-E) in a gravitationaly bound hydrogen atom. m

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A long time ago, in a galaxy far, far away, electric charge had not yet been invented, and atoms were heid together by gravitational forces. Computa the Bohr radius (ag) and the n=3 to n= 2 transition energy (E- E) in a gravitationally bound hydrogen atom. ev Additional Materials etlook
Transcribed Image Text:A long time ago, in a galaxy far, far away, electric charge had not yet been invented, and atoms were heid together by gravitational forces. Computa the Bohr radius (ag) and the n=3 to n= 2 transition energy (E- E) in a gravitationally bound hydrogen atom. ev Additional Materials etlook
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