DeBroglie Wavelength Comparison

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SUMMARY

The deBroglie wavelength for an electron in the n=6 orbit of He+ is derived to be three times larger than that in the n=2 orbit. This conclusion is based on the quantization of paths of electrons, represented by the equation 2 pi r = n (lambda), and the Bohr radius formula, rn = n² aB. By substituting the appropriate values and using Z = 2 for Helium ion, the relationship between the orbits and their corresponding wavelengths is established. The Bohr model is applicable in this context as it relates to the deBroglie wavelength.

PREREQUISITES
  • Understanding of quantum mechanics principles
  • Familiarity with the Bohr model of the atom
  • Knowledge of deBroglie wavelength calculations
  • Basic algebra and manipulation of equations
NEXT STEPS
  • Study the derivation of deBroglie wavelength in various atomic orbits
  • Explore the implications of the Bohr model in modern quantum mechanics
  • Learn about the quantization of angular momentum in quantum systems
  • Investigate the differences between classical and quantum descriptions of electron behavior
USEFUL FOR

Students of quantum mechanics, physics educators, and anyone interested in atomic structure and wave-particle duality.

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Homework Statement


Compare the deBroglie wavelength for an electron in the n=6 orbit of He+ compared to the n=2 orbit. Is the deBroglie wavelength the same, smaller, or larger? Derive this.

Homework Equations



Quantization of Paths of Electrons:
2 pi r = n (lambda)

Bohr Radius:
rn=n2 aB

The Attempt at a Solution



So plugging eqn 2 into eqn 1 and solving for lambda (and using Z = 2 for He+) gives:
wavelength = pi n aB

So using this, the deBroglie wavelength of n=6 would be 3 times larger than the n=2 wavelength?
I really don't know if this is correct. I don't know if the Bohr model can be used with deBroglie (they are kind of related right?)

Edit:
Ok the math symbol stuff is kind of messed up, I fixed what I could but it kept showing things wrong.
 
Last edited:
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Looks right to me.
 

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