Part of JPH-01 — Modern Physics: Photoelectric Effect & Matter Waves

de Broglie Wavelength — Special Scenarios

by Notetube Official133 words5 views
  • Tags: de-broglie, thermal, relativistic
  • Difficulty: Advanced

Thermal de Broglie wavelength: For a particle at temperature T with average KE = 3kT/2: λ = h/√(3mkT). For thermal neutrons at room temperature (300 K): λ ≈ 1.45 Å — comparable to interatomic spacing, enabling neutron diffraction.

Relativistic correction: When KE is comparable to rest mass energy (mc2mc^{2}): p = √(KE2KE^{2} + 2KEc2Ec^{2}m)/c... More precisely, for a particle with total energy E and rest mass m: p = √(E2E^{2} - (mc2mc^{2})^{2})/c, and λ = hc/√(E2E^{2} - (mc2mc^{2})^{2}). For non-relativistic particles (KE << mc2mc^{2}), this reduces to the standard λ = h/√(2mKE).

Electron in nth Bohr orbit: 2πr = nλ (Bohr's quantization is equivalent to fitting n de Broglie wavelengths in the orbit circumference). This provides a beautiful connection between wave nature and atomic structure.

Like these notes? Save your own copy and start studying with NoteTube's AI tools.

Sign up free to clone these notes