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Quantum physics
Showing 1–30 of 63 reference entries
c denotes the speed of light in vacuum. Its numerical value is fixed exactly in SI units.
DefinitionPhysics · MeasurementPlanck constanth denotes the Planck constant. Its numerical value is fixed exactly in SI units.
DefinitionPhysicsPhoton energy and frequencyOne photon's energy is proportional to its frequency.
ModelPhysics · Mathematics & logicInvariant spacetime intervalLorentz transformations preserve a combined space-time separation.
ModelPhysicsSchrödinger time evolutionA quantum wavefunction evolves according to its Hamiltonian.
ModelPhysicsBorn position probabilityA normalized wavefunction assigns probabilities to position intervals.
ModelPhysicsQuantum observable expectationsA state and observable determine the mean of repeated outcomes.
ModelPhysicsRobertson uncertainty relationA commutator constrains two outcome spreads in the same state.
ModelPhysicsSpin one-half and Pauli operatorsA spin one-half state has two outcomes along a chosen axis.
ModelPhysics · InformationPure and mixed density operatorsA density operator represents quantum statistical states.
DefinitionPhysicsIdeal projective measurementProjectors determine outcome probabilities and conditional states.
ModelPhysics · InformationComposite states and entanglementA joint pure state can fail to factor into subsystem states.
DefinitionPhysicsExchange symmetry of identical particlesBoson and fermion states respond differently to exchange.
ModelPhysicsHydrogen Coulomb energy levelsThe ideal one-electron atom has discrete bound energies.
ModelPhysics · ChemistryAtomic state labels and Pauli occupancyQuantum labels specify orbitals and spin states.
ModelPhysicsScattering cross sectionNormalize a scattering rate by incident flux.
ModelPhysicsHamiltonian and unitary quantum evolutionA closed quantum system evolves by iħ d|ψ⟩/dt=H(t)|ψ⟩.
ModelPhysicsStationary states and spectral superpositionFor a time-independent Hamiltonian, an energy eigenstate evolves by a phase exp(−iEt/ħ).
ModelPhysicsInfinite one-dimensional potential wellWith zero potential inside 0<x<L and impenetrable walls, normalized eigenfunctions are √(2/L) sin(nπx/L) and energies are n²π²ħ²/(2mL²), n=1,2,… .
ModelPhysicsProbability flux and rectangular-barrier tunnellingA real one-dimensional potential conserves probability current.
ModelPhysicsQuantum harmonic-oscillator spectrumFor H=p²/(2m)+mω²x²/2 on the real line, normalizable states have E_n=ħω(n+½), n=0,1,… .
ModelPhysics · ChemistryOscillator creation and annihilation operatorsFor the canonical oscillator, a=√(mω/(2ħ))x+ip/√(2mħω) and its adjoint satisfy [a,a†]=1.
ModelPhysicsHeisenberg evolution and conserved observablesThe Heisenberg observable A_H=U†A_SU obeys dA_H/dt=(i/ħ)[H_H,A_H]+(∂A_S/∂t)_H.
ModelPhysicsAngular-momentum algebra and ladder spectrumQuantum angular momentum obeys [J_i,J_j]=iħ ε_ijk J_k.
ModelPhysicsAddition of quantum angular momentaIndependent commuting angular momenta combine as J=J₁+J₂.
ModelPhysicsNondegenerate stationary perturbationFor an isolated nondegenerate eigenvalue of H₀ and a small Hermitian perturbation V, the leading energy corrections are ⟨n|V|n⟩ and Σ_{k≠n}|⟨k|V|n⟩|²/(E_n⁰−E_k⁰).
ModelPhysicsDegenerate stationary perturbationInside a degenerate eigenspace of H₀, first-order energy shifts and appropriate zeroth-order states come from diagonalizing the projected Hermitian perturbation PVP.
ModelPhysicsWeak time-dependent transition amplitudesStarting in eigenstate i of fixed H₀, a weak perturbation V(t) gives first-order amplitude c_f(t)=−(i/ħ)∫_{t₀}^t V_fi(t′)exp[i(E_f−E_i)(t′−t₀)/ħ]dt′ for f≠i.
ModelPhysics · ChemistryElectric-dipole transition selection rulesIn the long-wavelength electric-dipole approximation, atomic transition strength depends on the dipole matrix element.
ModelPhysics · ChemistryVariational ground-energy boundFor a self-adjoint Hamiltonian bounded below, every normalized trial state with a finite energy expectation satisfies ⟨ψ_trial|H|ψ_trial⟩≥E₀.
Mathematical statement