Determine energy levels of a electron in a hydrogen atom

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SUMMARY

The discussion focuses on determining the principal quantum numbers n1 and n2 for an electron transition in a hydrogen atom that emits light with a wavelength of 658.1 nm, using the Bohr model and the Rydberg formula. The energy of the emitted photon is calculated as E = hc/λ = 3.022 x 10-19 J. The Rydberg formula, λ = (n12 - n22)/R, is employed to relate the quantum numbers, with R being the Rydberg constant (RH = 0.010972 nm-1). The solution involves trial and error to find suitable integer values for n1 and n2, particularly focusing on the Balmer series where n' = 2.

PREREQUISITES
  • Understanding of the Bohr model of the hydrogen atom
  • Familiarity with the Rydberg formula for spectral lines
  • Knowledge of quantum numbers and their significance in atomic structure
  • Basic principles of photon energy calculation (E = hc/λ)
NEXT STEPS
  • Study the Balmer series of hydrogen emissions and their corresponding wavelengths
  • Learn about the Rydberg constant and its application in spectral analysis
  • Explore the derivation of the Rydberg formula and its limitations
  • Investigate other quantum mechanical models of the hydrogen atom beyond the Bohr model
USEFUL FOR

Students of quantum mechanics, physics educators, and anyone interested in atomic structure and electron transitions in hydrogen atoms.

Jonas Persson
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Homework Statement


When an electron in a hydrogen atom makes a transiton between two levels with prinicipal quantum numbers n1 and n2, light is emitted with wavelength of 658.1 nm. If we assume that the energy levels of the atom are in agreement with the Bohr model, what are n1 and n2?

Homework Equations




The Attempt at a Solution

I tried to calculate:
E = hc/λ = 3.022 * 10-19
which is the Energy for the wavelength.

E = -hcR/n^2

n^2 = -hcR/E
n^2 = -R/λ
which result in negative value(?)

Then I tried with
λ = (n1^2 - n2^2)/R

but then I always get two unknowns, and can't really come any further than that. Maybe I am looking in the wrong way or missing some theory.
 
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Jonas Persson said:
Assignment
When an electron in a hydrogen atom makes a transiton between two levels with prinicipal quantum numbers n1 and n2, light is emitted with wavelength of 658.1 nm. If we assume that the energy levels of the atom are in agreement with the Bohr model, what are n1 and n2?

Attempt
I tried to calculate:
E = hc/λ = 3.022 * 10-19
which is the Energy for the wavelength.

E = -hcR/n^2

n^2 = -hcR/E
n^2 = -R/λ
which result in negative value(?)

Then I tried with
λ = (n1^2 - n2^2)/R

but then I always get two unknowns, and can't really come any further than that. Maybe I am looking in the wrong way or missing some theory.

First, get straight what the story is of how the photon is produced:

  1. The electron originally has energy E_1 (which can be written in terms of the quantum number n_1)
  2. It emits a photon of energy E (which you calculate above).
  3. Afterward, the electron has energy E_2 (which can be written in terms of n_2)
So by conservation of energy, what is the relationship between E_1, E_2 and E?

You're right, you will have two unknowns, n_1 and n_2. But they are positive integers. So you can just try various values for n_1 and n_2 to see which combination works.
 
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Jonas Persson said:
Assignment
When an electron in a hydrogen atom makes a transiton between two levels with prinicipal quantum numbers n1 and n2, light is emitted with wavelength of 658.1 nm. If we assume that the energy levels of the atom are in agreement with the Bohr model, what are n1 and n2?
Jonas Persson said:
Attempt
I tried to calculate:
E = hc/λ = 3.022 * 10-19
which is the Energy for the wavelength.

E = -hcR/n^2

n^2 = -hcR/E
n^2 = -R/λ
which result in negative value(?)

Then I tried with
λ = (n1^2 - n2^2)/R

but then I always get two unknowns, and can't really come any further than that. Maybe I am looking in the wrong way or missing some theory.
You use wrong formula. The wavelength is attributed to two levels, according to the Rydberg formula.
25b1437b6d7203b25493f3a6b399aaf2c591e352

where Z is the atomic number (1 for Hydrogen atom) and n , n' are the energy levels, n'<n. R is the Rydberg constant. (RH = 0.010972 nm-1)
 
I tried adjacent orbits - no luck!
 
rude man said:
I tried adjacent orbits - no luck!
Don't expect the equation is exactly valid for any pair of n and n', but the emitted light is visible, what can be n'?
 
ehild said:
Don't expect the equation is exactly valid for any pair of n and n', but the emitted light is visible, what can be n'?
Once n is picked, n' is easy to determine - but how to pick n other than by trial and error?
 
rude man said:
Once n is picked, n' is easy to determine - but how to pick n other than by trial and error?
You know the wavelength ranges of the emission lines of Hydrogen atom. They are well separated according to the lower level. Emission in the visible range corresponds to the Balmer series, with n'=2 as lower level.
 
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stevendaryl said:
You're right, you will have two unknowns, n1n1n_1 and n2n2n_2. But they are positive integers. So you can just try various values for n1n1n_1 and n2n2n_2 to see which combination works.
I think this solution is the simplest. If you are learning about electron transitions, then you must surely have learned about the different series. Either you can check your textbook (or online) for the energy values of the different transitions from different "n" states.

The value you calculate, E, is simply the difference between energy states. If you still don't understand what the value of E really is, take a look at this link:
http://www.kentchemistry.com/links/AtomicStructure/waveenergy.htm
 
Re search: something like this perhaps. Spot the 'candidate' !

## \begin{array}{|c|c|c|c|c|c|}
\hline & m & 1 & 2 & 3 & 4 & 5 \\
\hline n \\
\hline 1 & & & 0.750 & 0.889 & 0.938 & 0.960\\
\hline 2 & & & & 0.139 & 0.188 & 0.210\\
\hline 3 & & & & &0.049 & 0.071\\
\hline 4 & & & & & & 0.023\\
\hline
\end{array}##
 
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