SUMMARY
The shortest wavelength of light that an atom can radiate due to electron shell transitions is determined by the energy levels of the atom, with Fermium (Z=100) exhibiting a Kβ energy of 136.08 keV, corresponding to a wavelength of approximately 9.11 picometers. The longest wavelength is not fixed but is limited by practical considerations, with transitions between high energy shells yielding lower energy emissions. Gamma rays, which have wavelengths less than 10 picometers, are produced from nuclear transitions rather than electronic transitions. The Lyman series provides a formula for the limit of wavelengths for hydrogenic atoms, specifically for single-electron ions, represented as λ = 1/(91.175Z²) in nanometers.
PREREQUISITES
- Understanding of atomic structure and electron shell configurations
- Familiarity with photon energy and wavelength calculations
- Knowledge of the Lyman series and its significance in atomic physics
- Basic principles of gamma ray production and nuclear transitions
NEXT STEPS
- Study the Lyman series and its applications in atomic physics
- Research the properties and applications of gamma rays in nuclear physics
- Explore X-ray fluorescence (XRF) techniques and their relevance to electron transitions
- Investigate the electron configurations and transition energies of heavy elements like Fermium
USEFUL FOR
Students and professionals in physics, particularly those focused on atomic and nuclear physics, as well as researchers interested in electron transitions and photon emissions.