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Showing 91–120 of 365 reference entries
Clocks at different radii measure different light frequencies.
ModelPhysics · Earth & cosmosFriedmann cosmological evolutionHomogeneity and isotropy reduce gravitational expansion to two balances.
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.
ModelPhysics · Earth & cosmosNuclear binding energyA bound nucleus has less rest mass than its separated nucleons.
ModelPhysics · Earth & cosmosExponential radioactive decayA fixed decay probability per time gives a population timescale.
ModelPhysics · Earth & cosmosFission, fusion and reaction energyNuclear rearrangement can release or require energy.
ModelPhysicsScattering cross sectionNormalize a scattering rate by incident flux.
ModelPhysicsStandard Model matter familiesQuarks and leptons form three generations.
ModelPhysicsStandard Model interactionsGauge fields mediate three interactions; the Higgs is a scalar sector.
ModelPhysicsInteraction-specific quantum-number balancesA balance rule must name the interaction where it applies.
ModelPhysics · ChemistryBloch states and electronic bandsA periodic crystal potential organizes energies by wavevector and band.
ModelPhysics · ChemistrySemiconductor electrons and holesBand occupancy and doping control mobile carriers.
ModelPhysicsBose and Fermi thermal occupationsIndistinguishable particles have different equilibrium state populations.
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 statementPhysics · ChemistryFundamental thermodynamic relation and chemical potentialFor a simple compressible equilibrium system, U(S,V,{N_i}) has differential dU=T dS−p dV+Σ_i μ_i dN_i.
ModelPhysics · ChemistryEnthalpy and Helmholtz thermodynamic potentialsThe Legendre transforms H=U+pV and F=U−TS change the natural state variables: dH=T dS+V dp and dF=−S dT−p dV at fixed composition.
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