How Do You Calculate the Wavelength of an Electron Transition in a Helium Ion?

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SUMMARY

The discussion focuses on calculating the wavelength of an electron transition in a helium ion (He+). The expression for the electron state energies is derived as E = (-4R)/(n²), where R is the Rydberg constant. For the wavelength associated with a transition between the lowest two energy states, the relevant equation is ΔE = RchZ²(1/n²(1) - 1/n²(2)), utilizing constants such as the speed of light (c = 2.9979 x 10E8 m s⁻¹) and Planck's constant (h = 6.626 x 10E-34 J s).

PREREQUISITES
  • Understanding of quantum mechanics principles
  • Familiarity with the Rydberg formula
  • Knowledge of Planck's constant and its application
  • Basic grasp of electron transitions and energy levels
NEXT STEPS
  • Study the Rydberg formula for hydrogen-like atoms
  • Learn about quantum numbers and their significance in electron transitions
  • Explore the concept of energy level diagrams for ions
  • Investigate the relationship between energy and wavelength in photon emissions
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Students studying quantum mechanics, physicists focusing on atomic structure, and educators teaching advanced topics in chemistry and physics.

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Homework Statement



He+ ion consists of a nucleus which is an alpha particle plus one orbiting electron.Hence it has a net positive charge.
a)Derive an expression for the electron state energies
b)what is the wavelength associated with a transition between the lowest two energy states?

Homework Equations


The Attempt at a Solution


For part a) i figured it out to be E=(-4R)/(n^2) where R is the rydbergs constant
for part b) I am having trouble not sure where to begin
 
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Don't forget, the wavelength of a photon emitted, for a drop in energy level, is proportional to the difference in energies between the two levels.

I think that will be useful.
 
should i use this

ΔE = RchZ²{1/n²(1) - 1/n²(2)}

where R is the Rydberg constant (1.0974 x 10E7 m-¹); c the speed of light in vacuum (2.9979 x 10E8 m s-¹); h Planck's constant (6.626 x 10E-34 J s); Z nuclear charge; n(1) & n(2) are the principal quantum numbers of the electron transition
 

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