Zeeman Effect: Splitting of Lyman-α Wavelength

  • Thread starter Thread starter Taylor_1989
  • Start date Start date
  • Tags Tags
    Wavelength Zeeman
Click For Summary
SUMMARY

The discussion focuses on the Zeeman Effect as it pertains to the Lyman-α line (n = 2 → n = 1) with a wavelength of 121.6 nm in the absence of a magnetic field. When subjected to a magnetic field of 1 Tesla, the wavelength splits into 121.6 ± 0.0007 nm, calculated using the formula ΔE = μ_B·B·m and the derived equation for Δλ. Participants debated the correctness of the calculations and the use of the Taylor series method versus the derivative method. They also explored the implications of magnetic quantum numbers and potential additional spectral lines resulting from the splitting.

PREREQUISITES
  • Understanding of the Zeeman Effect and its implications in quantum mechanics.
  • Familiarity with the Lyman series in hydrogen and its spectral lines.
  • Knowledge of quantum mechanics equations, particularly ΔE = μ_B·B·m.
  • Basic proficiency in calculus, specifically derivatives and Taylor series.
NEXT STEPS
  • Research the Zeeman Effect in hydrogen, focusing on its mathematical derivation and implications.
  • Learn about the Lyman series and its transitions in hydrogen atoms.
  • Explore the use of Taylor series in quantum mechanics for approximating functions.
  • Investigate the fine structure of spectral lines and how magnetic fields influence them.
USEFUL FOR

Students of physics, particularly those studying quantum mechanics, educators teaching the Zeeman Effect, and researchers interested in atomic transitions and magnetic field interactions.

Taylor_1989
Messages
400
Reaction score
14

Homework Statement


The Lyman-α line (n = 2 → n = 1) has a wavelength of 121.6nm in the absence of a magnetic field.
When B = 1 Tesla, into how many wavelengths will this split and what are their wavelengths?

(You may need the values
μ B = 9.274 × 10 −24 J/T, h̄ = 1.054 × 10 −34 Js and c = 2.998 × 10 8 m/s.)

Homework Equations


##\Delta E=\mu _B\cdot B\cdot m##

The Attempt at a Solution


Have I done this correctly in my lecture note they use Taylor series which I understand but I have use the derivative method as follows:

$$E=\frac{hc}{\lambda }$$

$$\Delta E=\frac{hc\Delta \lambda }{\lambda ^2}$$

$$\Delta \:\lambda =\:\frac{\mu _B\cdot B\cdot m\cdot \lambda ^2}{hc}$$

subbing in the values

$$\Delta \:\lambda =\:\frac{\left(9.274\cdot 10^{-24}\right)\left(1\right)\left(1\right)\left(121.6\cdot 10^{-9}\right)^2}{\left(6.626\cdot 10^{-34}\right)\left(3\cdot 10^8\right)}=6.89\cdot 10^{-13}m$$

so then my final answer is

$$\lambda \pm \Delta\lambda=121.6 \pm 0.0007 nm$$

is there an advantage to using the Taylor series approach?
 
Last edited:
Physics news on Phys.org
Why did you switch the exponent in ## \mu_B ## from ## 10^{-24} ## to ## 10^{-27} ##? ## \\ ## I think ## 10^{-24} ## is correct, and you introduced a ## 10^{-3} ## error. ## \\ ## And your Taylor series does work very well. (It actually carries the name that you chose on PF). :)
 
Charles Link said:
Why did you switch the exponent in ## \mu_B ## from ## 10^{-24} ## to ## 10^{-27} ##? ## \\ ## I think ## 10^{-24} ## is correct, and you introduced a ## 10^{-3} ## error. ## \\ ## And your Taylor series does work very well. (It actually carries the name that you chose on PF). :)

Sorry I have edited it, when I do latex quickly I tend to mistake thing sorry.
 
And you need to square ## \lambda ##. Clearly a "typo".
 
I have squared ##\lambda## have I not? is what I have done method wise correct?
 
  • Like
Likes   Reactions: Charles Link
Taylor_1989 said:
I have squared ##\lambda## have I not? is what I have done method wise correct?
I checked the arithmetic quickly=I get about ## .7 \cdot 10^{-12}## m=.0007 nm . I'll recheck the arithmetic, but that's what I got. (I'm working without a calculator). ## \\ ## Edit: Your answer looks correct ! :) ## \\ ## Additional item: You get ## m_l=\pm 1, n=2 ## going to ## m_l=0, n=1 ##, accounting for the splitting. I think you can also get ## m_l=0, n=2 ##, going to ## m_l=0, n=1 ##. How many spectral lines does that give? One question that would take additional research is if there is any ## m_s ## splitting. It could be worthwhile to google the Zeeman effect in hydrogen. ## \\ ## And you are on the right track, but it appears this one gets slightly complicated. See https://chem.libretexts.org/Core/Physical_and_Theoretical_Chemistry/Quantum_Mechanics/Zeeman_Effect/5:_Zeeman_Effect_in_Hydrogen_atom (Some of the detail is hard to read in this "link"). This one is ## n=3 ## to ## n=2 ##, but may also be helpful. https://www.scribd.com/document/262518364/Zeeman-Effect-in-Hydrogen ## \\ ## See also: http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/zeeman.html ## \\ ## And here's what may be the best, and most applicable of the bunch: https://en.wikipedia.org/wiki/Zeeman_effect#Example:_Lyman_alpha_transition_in_hydrogen It looks like it gets a little complicated sorting out the different allowed transitions, as well as perhaps determining since you have a relatively strong magnetic field, that some of the fine structure that occurs might be considered to be the same spectral line, even though there may be additional fine splittings.
 
Last edited:
Charles Link said:
And you need to square ## \lambda ##. Clearly a "typo".

Charles Link said:
I checked the arithmetic quickly=I get about ## .7 \cdot 10^{-12}## m=.0007 nm . I'll recheck the arithmetic, but that's what I got. (I'm working without a calculator). ## \\ ## Edit: Your answer looks correct ! :) ## \\ ## Additional item: You get ## m_l=\pm 1, n=2 ## going to ## m_l=0, n=1 ##, accounting for the splitting. I think you can also get ## m_l=0, n=2 ##, going to ## m_l=0, n=1 ##. How many spectral lines does that give? One question that would take additional research is if there is any ## m_s ## splitting. It could be worthwhile to google the Zeeman effect in hydrogen. ## \\ ## And you are on the right track, but it appears this one gets slightly complicated. See https://chem.libretexts.org/Core/Physical_and_Theoretical_Chemistry/Quantum_Mechanics/Zeeman_Effect/5:_Zeeman_Effect_in_Hydrogen_atom (Some of the detail is hard to read in this "link"). This one is ## n=3 ## to ## n=2 ##, but may also be helpful. https://www.scribd.com/document/262518364/Zeeman-Effect-in-Hydrogen ## \\ ## See also: http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/zeeman.html ## \\ ## And here's what may be the best, and most applicable of the bunch: https://en.wikipedia.org/wiki/Zeeman_effect#Example:_Lyman_alpha_transition_in_hydrogen It looks like it gets a little complicated sorting out the different allowed transitions, as well as perhaps determining since you have a relatively strong magnetic field, that some of the fine structure that occurs might be considered to be the same spectral line, even though there may be additional fine splittings.

Thank you very much, and I will start reading the information you link now, much apprecatied :)
 
  • Like
Likes   Reactions: Charles Link

Similar threads

Replies
15
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
Replies
3
Views
3K
  • · Replies 2 ·
Replies
2
Views
7K
Replies
3
Views
5K
  • · Replies 16 ·
Replies
16
Views
3K
  • · Replies 4 ·
Replies
4
Views
4K
  • · Replies 3 ·
Replies
3
Views
4K
  • · Replies 2 ·
Replies
2
Views
2K