Reference library
Foundations
Explore concepts, laws, equations and methods, with clear explanations of their use and sources. Choose an area of study or find a specific entry.
More filters
Reference entries
Showing 721–750 of 1709 reference entries
The minimal Standard Model has gauge group SU(3)_C×SU(2)_L×U(1)_Y with strong and electroweak gauge sectors.
ModelPhysicsCoherent vacuum neutrino mixing and oscillationIn a unitary light-neutrino mixing model |ν_α⟩=Σ_iU_αi*|ν_i⟩.
ModelPhysicsElastic neutron energy transfer and bounded moderationA nonrelativistic neutron of mass m and kinetic energy E scattered elastically from a free stationary nucleus of mass M retains E′/E=(η²+1+2ηcosθ_cm)/(η+1)², η=M/m.
ModelPhysicsFission generations and effective multiplicationFission can emit neutrons that induce further fissions, while capture without fission and leakage remove neutrons from the chain.
ModelPhysics · Earth & cosmosThermal two-body nuclear reaction rateIn a dilute nondegenerate gas of independently distributed reacting nuclei at common temperature T, reaction events per volume/time are R_ab=n_an_b⟨σv⟩/(1+δ_ab), where δ_ab=1 for the same species and 0 otherwise.
ModelPhysics · Earth & cosmosCoulomb penetration, astrophysical S factor and Gamow windowFor repulsively charged nuclei with κ=Z_aZ_be²/(4πε₀)>0 and relative speed v, the Sommerfeld parameter is η=κ/(ħv) and the leading low-energy Coulomb penetration exponential is exp(−2πη)=exp[−√(E_G/E)], E_G=2μ(πκ/ħ)².
ModelPhysicsNearly-free electron gap at a zone boundaryFor a real periodic one-dimensional potential of period a, define V_G=a⁻¹∫₀ᵃV(x)e^(−iGx)dx, G=2π/a, and ε_k=ħ²k²/(2m).
ModelPhysicsNearest-neighbour tight-binding chainFor a periodic chain of N orthonormal localized orbitals, one per site with spacing a, take H_nm=ε₀δ_nm−t(δ_(n+1,m)+δ_(n−1,m)).
ModelEarth & cosmosGeological time units and correlationGeological history is organized into nested eons, eras, periods, epochs and ages.
DefinitionEarth & cosmosEarly-Earth heating and differentiationAccretion, impacts, gravitational redistribution and radioactive decay contributed to early-Earth heating.
ModelEarth & cosmosBiological oxygen production and geological sinksOxygenic photosynthesis supplied oxygen while chemical reactions with reduced material consumed it.
ModelEarth & cosmos · Chemistry · MeasurementStable-isotope ratio reporting and fractionationAn isotope delta compares a specified sample isotope ratio with the same ratio in a stated reference.
DefinitionEarth & cosmosSlope forces, material strength and waterGravity supplies both downslope shear and normal loading on a slope.
ModelEarth & cosmosCoastal sediment supply and redistributionCoastal landforms reflect sediment supply, wave/current transport, erosion and deposition.
ModelEarth & cosmosMoist adiabatic ascent and orographic precipitationAn ascending air parcel expands as pressure falls and can cool toward saturation.
ModelEarth & cosmosLuminosity and received fluxFor an isotropic source in transparent Euclidean space, bolometric flux decreases as luminosity divided by the area of a sphere.
ModelEarth & cosmosLogarithmic astronomical magnitudesA magnitude difference encodes a flux ratio on a logarithmic scale: brighter objects have smaller magnitudes.
DefinitionEarth & cosmosStellar spectra as physical evidenceContinuum shape and spectral-line patterns constrain temperature, composition and the physical conditions in a stellar atmosphere.
ModelEarth & cosmosAstronomical detector and spectrometer measurementsA CCD records photo-generated charge in pixels over an exposure.
MethodEarth & cosmosDiffraction scale and atmospheric seeingA circular aperture has a diffraction angular scale proportional to wavelength divided by diameter.
ModelEarth & cosmosInterstellar extinction and reddeningDust absorbs and scatters radiation along a line of sight.
ModelEarth & cosmosCalibrated distance indicators and selectionA distance ladder transfers geometric calibrations to luminosity-based indicators such as Cepheids and standardized supernovae.
MethodEarth & cosmosSpecific intensity and radiative transferAlong a ray, local emission adds and extinction removes specific intensity.
ModelEarth & cosmosSpherical stellar mass and pressure structureFor a spherical quasistatic Newtonian star, enclosed mass increases with shell volume and density, while the pressure gradient balances gravity due to enclosed mass.
ModelEarth & cosmosRadiative diffusion inside an opaque starIn an optically thick stellar region close to local thermodynamic equilibrium, radiative diffusion relates luminosity to the temperature gradient through density and an appropriate mean opacity.
ModelEarth & cosmosStellar energy conservation during evolutionA stellar shell's luminosity divergence accounts for local energy production, change in specific internal energy and compression or expansion work.
ModelEarth & cosmosStellar convection and the Schwarzschild criterionA displaced parcel that adjusts pressure rapidly but exchanges little heat can continue rising when it becomes less dense than its environment.
ModelEarth & cosmosHydrogen and helium fusion pathways in starsThe proton–proton chains and CNO cycles convert hydrogen into helium through different reaction sequences; CNO nuclei participate in a catalytic cycle.
ModelEarth & cosmosHertzsprung–Russell diagram and stellar interpretationAn HR diagram compares luminosity with effective temperature or a related spectral classification.
MethodEarth & cosmosBinary stars as stellar-mass measurementsA resolved relative orbit and period can constrain a binary's total mass through Newtonian two-body dynamics.
Method