Quick question about Rydberg Constant Equations

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The discussion revolves around deriving the Rydberg constant equation and understanding the relationship between photon emission and energy levels in an atom. The equation 1/lambda = R(1/(n^2) - 1/(m^2)) is used to describe the wavelength of emitted photons when an electron transitions between energy levels. To connect this to energy, the conservation of energy principle is applied, leading to the equation E = hc/lambda = E_n - E_m. The conversation also references Bohr's model of the hydrogen atom to derive the necessary energy expressions for the energy levels E_n and E_m. Overall, the thread seeks guidance on how to approach these derivations and clarify the concepts involved.
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So I have the equation

1/lambdamn = R(1/(n^2) - 1/(m^2))

Where m > n, and lambda is the energy emitted by a photon from m going down to n. And I have to get show that this formula can be explained by

1.) Requiring that light occurs in quanta

2.) And to get a formula for Energy in terms of R.

I had previously derived this forumula

E = - e^2 / 4*pi*eo*an + n^2*(hbar)/^2/2m*an

where a is the radius of the electron orbit, n will be 1 for our purposes, etc. How do I go about getting an equation for part 2...and how do I even begin part 1?

Any help is appreciated, thanks!
 
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It maybe helps to notice that lambda is not the energy but the wavelength of the emitted photon.
 
How did u get that formula,exactly...?I mean,expressed as a sum of 2 terms,what does each stand for...?

Daniel.
 
Conservation of energy requires:

\frac{hc}{\lambda}=E_n-E_m
where E_n>E_m.

Use the expression for the nth energy to find R.
 
But what equations do I have for En and Em?
 
Do you know Bohrs model of the hydrogen atom?
 
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