Linked from

The 64 pages that link to Zeeman effect, each with the reason it gives.

• Nuclear magnetic resonance spectroscopyRelated: Field-induced nuclear energy-level separation sets the conditions for resonance.

• Spectral lineRelated: Resolved line splitting can reveal the strength and orientation of magnetic fields.

• Nuclear magnetic resonanceRelated: The field separates nuclear spin energy levels, allowing radiofrequency transitions between them.

• Stellar spectroscopyRelated: Magnetically affected stellar lines reveal surface field strengths and structure.

• Laser coolingRelated: Magnetic-field shifts make position-dependent resonance possible in magneto-optical traps.

• Hendrik LorentzBroader topic: Lorentz’s theoretical explanation of Zeeman’s observation helped earn their shared Nobel Prize.

• Electron spinRelated: Electron magnetic moments make spin states shift in an applied field.

• Energy levelRelated: A magnetic field changes level energies according to their magnetic properties.

• ParamagnetismRelated: Field-induced energy shifts favor magnetic moment orientations aligned with the field.

• Fine structureCompared with: It also splits spectral lines, but requires an applied magnetic field.

• Atomic spectrumBroader topic: Magnetic fields split atomic energy levels and reveal structure within a line pattern.

• Angular momentum operatorRelated: Magnetic interactions couple angular-momentum operators to the field and split their eigenstates.

• Magnetic anisotropyRelated: The field’s directional energy competes with a material’s anisotropy energy.

• Electron paramagnetic resonanceRelated: The applied field separates spin energy levels before resonance.

• Old quantum theoryRelated: Its complex patterns challenged simple quantization and prompted further model extensions.

• Orbital angular momentumRelated: Orbital angular momentum couples to magnetic fields and contributes to the splitting.

• 21-centimeter lineRelated: Magnetic fields can subtly split the hydrogen line and reveal cosmic magnetism.

• Hyperfine structureCompared with: Unlike hyperfine splitting, it arises from an applied field, though both effects can shape atomic spectra.

• Microwave spectroscopyRelated: Magnetic resonance measurements detect field-dependent splitting in microwave spectra.

• Solar magnetic fieldRelated: Solar astronomers use its spectral signatures to measure magnetic-field strength and direction.

• Nuclear spinRelated: A magnetic field splits nuclear spin states into distinct energy levels.

• Stern–Gerlach experimentRelated: Both phenomena arise from interactions between magnetic fields and quantized atomic angular momentum.

• SunspotRelated: Solar spectral-line splitting reveals the intense magnetic fields within sunspots.

• Optical pumpingRelated: Magnetic fields separate sublevels that circularly polarized light can populate selectively.

• Solar prominenceRelated: Its signatures help estimate magnetic fields in prominence plasma.

• Stark effectCompared with: It is the magnetic-field counterpart to the Stark effect.

• Hund's rulesRelated: Ground-term angular momenta help explain an atom's magnetic-field response.

• Laser spectroscopyRelated: Laser-resolved Zeeman features measure magnetic fields and probe atomic structure.

• Magneto-optical trapRelated: The field gradient shifts atomic transitions with position, selecting the restoring beam.

• Spin quantum numberRelated: Spin projection contributes to the magnetic splitting of energy levels.

• Faraday effectRelated: Field-shifted optical transitions help create different responses to the two circular polarizations.

• George Ellery HaleRelated: Hale used this spectral signature to detect magnetism in sunspots.

• Spectral line broadeningRelated: Magnetic fields can produce broadened profiles when separate components are unresolved.

• Electron magnetic momentRelated: Its spectral shifts expose magnetic moments of electrons in atoms.

• Magnetic quantum numberRelated: Magnetic-field energy shifts depend on angular-momentum projection.

• Optical atomic clockRelated: Magnetic fields can displace clock transitions and must be measured or suppressed.

• Atomic physicsBroader topic: Its line splitting measures how atomic angular momentum couples to magnetic fields.

• Bohr magnetonRelated: Its energy shifts are often expressed using the Bohr magneton.

• Larmor precessionRelated: The same field that drives precession also separates magnetic energy states.

• Solar spectrumRelated: Changes in solar line shapes reveal magnetic fields on the Sun.

• Sommerfeld modelRelated: Sommerfeld’s expanded quantum numbers helped classify some magnetic spectral patterns.

• Circular polarizationRelated: Radiation viewed along the field can contain oppositely handed circularly polarized spectral components.

• Faraday rotationCompared with: Unlike line splitting, rotation measure probes the integrated field through polarized radio emission.

• Hamiltonian operatorRelated: A magnetic-field term added to the Hamiltonian predicts the level splitting.

• Interstellar magnetic fieldRelated: Zeeman measurements can estimate the field component along the line of sight.

• Landau levelCompared with: It shifts spin or orbital energies, unlike Landau quantization of free transverse motion.

• Nuclear magnetic momentRelated: A field couples to the nuclear moment and shifts nuclear energy levels.

• Pauli paramagnetismRelated: It shifts opposite-spin electron energies in opposite directions, creating the occupation imbalance.

• Gyromagnetic ratioRelated: The ratio helps determine how angular-momentum states shift in a field.

• Degenerate energy levelsRelated: A magnetic field lifts degeneracies among states with different angular momentum projections.