Calculating Initial Energy Level for Emitted Photons

In summary: I don't think I can get the actual value. I measured the angles using a protractor, it was a bit difficult to get the angles right as the readings were quite close.The energies were 2.1, 2.2, 2.3 eV.Sorry, I don't think I understand. You must have used some method to determine the grating parameter, how did you do that?The grating parameter is the distance between the slits (d in the formula). How did you measure it?I'm not sure, I think you might be misunderstanding me. I only have a few values to work with and I was using the formulas given to get the answer, I did not have to
  • #1
oldspice1212
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Homework Statement


Using the energies, determine from which initial energy level (n) the electrons decayed when it emitted photons at each of these wavelengths.

Homework Equations


[itex]E = - \frac{ me^4 }{ 8\epsilon_0^2h^2 }\frac{ 1 }{ n^2 }[/itex]

[itex]Delta E = E_f-E_i= - \frac{ me^4 }{ 8\epsilon_0^2h^2 }\left( \frac{ 1 }{ n^2_f}-\frac{ 1 }{ n^2_i } \right)[/itex]

The Attempt at a Solution


I have the energy and wavelengths for this question but I'm not exactly sure what formula to use, this is for an hydrogen atom, so that's where my question lies but I have two equations (above)I just need guidance on which one to use.
 
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  • #2
I was thinking to use the second equation but I don't have the the final energy I just have energy which is delta E.
 
  • #3
Or also, would rydberg formula work, where nf is 2 as it's the hydrogen atom?
 
  • #4
oldspice1212 said:
I was thinking to use the second equation but I don't have the the final energy I just have energy which is delta E.
ni and nf are positive integers. Find an ni so as the given delta E-s correspond to positive integers less than ni.

ehild
 
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  • #5
ehild said:
ni and nf are positive integers. Find an ni so as the given delta E-s corresponds to positive integers less than ni.

ehild

Sorry, I don't quite understand what you mean? Could you interpret in different terms.

What I think you're saying...

[itex]E = - (13.6eV)\left( \frac{ 1 }{ n^2_f }-\frac{ 1 }{ n^2_i } \right)[/itex] so just solve for [itex]n_i[/itex]?
 
  • #6
oldspice1212 said:
Sorry, I don't quite understand what you mean? Could you interpret in different terms.

What I think you're saying...

[itex]E = - (13.6eV)\left( \frac{ 1 }{ n^2_f }-\frac{ 1 }{ n^2_i } \right)[/itex] so just solve for [itex]n_i[/itex]?
What are the delta E-s? How many are given?

You need to try different ni-s so as the delta E values can be fit to the equation. In case ni=2 there is only one possibility to decay, from the excited level 2--->1.
 
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  • #7
Well for each wavelength I had, I had to calculate the energy of the photons in eV. So that's what I'm assuming are my delta E's. So for 1 I have E=2.1eV. So for the equation above, I would just put random n's for both [itex]n_f[/itex] and [itex]n_i[/itex] where n is 1,2,3..etc, and see if those correspond to the following E?

Thanks for you help btw, really appreciate it.
 
  • #8
What are the other delta E-s and how many are given? Is 2.1 eV the smallest or the greatest?
 
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  • #9
Three, and they're all similar, one is 2.4, the other 2.1, and 2.3. It's also the resulting wavelengths were all similar as well that's why the results are pretty weird.
 
  • #10
Can you cite the whole original problem text, please?
 
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  • #11
It's part of a lab, so, just this was the part troubling me I did everything else.

Hydrogen Spectrum

Use the difference between these angles and the central maximum to determine the wavelengths of these colors. Use the grating line separation that you determined with the Sodium Spectrum.
Which I used [itex]|right angle - central maximum|+|left angle-central maximum|[/itex]
Using this value for theta I calculated the wavelength, [itex]lambda = \frac{ d sin theta }{ m }[/itex] m=1

Then for each wavelengths, I had to calculate the energy of the photons in eV. Which I used
[itex]\frac{ 1.24 times 10^-6 eV }{ lambda times 10^{-9} }[/itex]

there are only three colours we used, so this the part which was sort of confusing for me.

Now using these energies, determine from which initial energy level (n) the electron decayed when it emitted photons at each of these wavelengths.

Energies: 2.1, 2.2, 2.3 eV
 
  • #12
oldspice1212 said:
It's part of a lab, so, just this was the part troubling me I did everything else.

Hydrogen Spectrum

Use the difference between these angles and the central maximum to determine the wavelengths of these colors. Use the grating line separation that you determined with the Sodium Spectrum.
Which I used [itex]|right angle - central maximum|+|left angle-central maximum|[/itex]

You should have used the average deflection: half of the angle above. If you used the same formula when determining the grating parameter, it was wrong, too.

oldspice1212 said:
I
Using this value for theta I calculated the wavelength, [itex]lambda = \frac{ d sin theta }{ m }[/itex] m=1

Then for each wavelengths, I had to calculate the energy of the photons in eV. Which I used
[itex]\frac{ 1.24 times 10^-6 eV }{ lambda times 10^{-9} }[/itex]

there are only three colours we used, so this the part which was sort of confusing for me.

Now using these energies, determine from which initial energy level (n) the electron decayed when it emitted photons at each of these wavelengths.

Energies: 2.1, 2.2, 2.3 eV

As the angles were wrong, the energies are not correct.
The hydrogen spectrum consists of 4 lines, 656.3 nm, 486.1 nm, 434.0 nm, 410.2 nm. a the last two lines are very close, the resolution of your set-up was not enough to show them as different lines. And the visible range corresponds to the Balmer series, so you know the final n.

ehild
 
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  • #13
ignore.
 
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  • #14
Why is the formula wrong for the grating parameter, I was only given that formula for it unless you mean the angle I used to calculate d was wrong, but there was not much I could do for that as it was very close to the central maximum angle. And my first thought was to use the average of the angles I mentioned on the previous post but it didn't instruct me to do so, but I think I will do that anyways as I get a more clear result.

I took the average of the angles and got different energies, being 3, 2.5, 2.

And yes the final n is 2, so I just calculate the initial n now right? Using the formula I mentioned above.
 
  • #15
So the grating parameter was given? Then it must be correct. What was it?
What were the angles? How did you measure the angles?
The energies seem a bit inaccurate. What were the wavelengths ?
Yes, the final level is n=2. Just calculate the initial ones.

ehild
 
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  • #16
The grating parameter wasn't given I had to calculate that myself, using the lambda = dsintheta/m but the central maximum was 80 degrees as was the average of the angles. Lambda was 589.3 nm for the grating line used to measure grating parameter. The measured wavelengths weren't very good haha, I know the experiment failed but I won't try to edit it as that would be bad science! But the wavelengths measured were 560nm, 600nm, 600nm.

Once again, tyvm for the help.
 
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  • #17
The energies you wrote are acceptable. What you get for the initial n? Round them to the nearest integer.

ehild
 
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  • #18
Alright so I got,
(Rounded energy levels)
3eV - 1
2.5 eV - 2
2 eV - 2
 
  • #19
NO! You have to get numbers greater than 2! The hydrogen atoms are excited in the lamp and they return to the level n=2 from higher levers when emitting a certain wavelength light.
The formula is ##\Delta E = 13.6 (\frac{1}{2^2}-\frac{1}{n^2}) ##
 
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  • #20
I just realized that haha, I found the mistake, I had -13.6 so that screwed up my whole calculation, thank you! So now, I have,

3eV - 6
2.5eV - 4
2eV - 3

Haha, thanks again ehild, you made this very fun for me xD.
 
  • #21
It is all right now. :) The negative sign refers to the energies of the Hydrogen atoms, but the photons have positive energies.
That 3 eV is a mixture of the 5th and 6th level, it is really difficult to resolve the two blue lines in the spectrum.

ehild
 
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  • #22
That makes a lot of sense, I understand this now.

Thanks again and thank you very much for making this a fun experience!
 
  • #23
Oh my, you sent a bunch of likes... Thank you, but one would have been enough!
 
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  • #24
Haha, well every post you made was helpful, so why not :)! And it doesn't take much effort to click the like, so I'll share the love hehe.
 

1. How is the initial energy level for emitted photons calculated?

The initial energy level for emitted photons is calculated using the formula E = hf, where E is the energy, h is Planck's constant (6.626 x 10^-34 joule seconds), and f is the frequency of the emitted photon.

2. What is Planck's constant and how is it related to calculating the initial energy level for emitted photons?

Planck's constant, denoted as h, is a fundamental constant in quantum mechanics that relates the energy of a photon to its frequency. It is used in the formula E = hf to calculate the initial energy level for emitted photons.

3. How does the frequency of an emitted photon affect the initial energy level?

The frequency of an emitted photon directly affects the initial energy level, as shown in the formula E = hf. Higher frequencies correspond to higher energy levels, while lower frequencies correspond to lower energy levels.

4. Can the initial energy level for emitted photons be calculated for all types of light?

Yes, the initial energy level for emitted photons can be calculated for all types of light, including visible light, infrared light, ultraviolet light, and even X-rays and gamma rays.

5. What is the significance of calculating the initial energy level for emitted photons in scientific research?

The calculation of the initial energy level for emitted photons is crucial in understanding the properties and behavior of light and its interaction with matter. It is also important in various fields of scientific research, such as astrophysics, quantum mechanics, and spectroscopy.

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