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In a Newtonian isolated two-body Keplerian model, the host star's line-of-sight orbital velocity has semi-amplitude K=(2πG/P)^(1/3) Mp sin i/[(Mstar+Mp)^(2/3)√(1−e²)].
MethodEarth & cosmosInitial mass functions and stellar population accountingFor a specified birth population, an initial mass function ξ(m) defines dN=ξ(m)dm on a stated initial-mass interval.
DefinitionEarth & cosmosWhite-dwarf mass–radius relation and ideal limiting massCold noninteracting electron support and spherical Newtonian hydrostatic balance give a nonrelativistic n=3/2 polytrope with R proportional to μₑ^(−5/3)M^(−1/3).
ModelEarth & cosmosRotation-powered pulsars and spin-down inferenceNeutron-star pulsars have rotating magnetized stellar remnants whose emission can sweep past the observer.
ModelEarth & cosmosCore collapse and thermonuclear stellar explosionsCore-collapse supernovae involve loss of support in an evolved stellar core, rapid contraction and an explosion whose energy transfer involves dense matter and neutrinos.
ModelEarth & cosmosAccretion energy, efficiency and angular-momentum transportMatter moving inward in a gravitational field can release binding energy if energy is dissipated.
ModelEarth & cosmosEddington luminosity as a conditional force balanceFor isotropic luminosity L and a constant flux-weighted opacity per mass κ, outward radiative acceleration is κL/(4πr²c).
ModelEarth & cosmosRoche geometry and binary mass transferIn a circular two-point-mass binary's corotating frame, the effective potential per mass is Φ_eff=−GM₁/r₁−GM₂/r₂−Ω²(x²+y²)/2, with origin at the barycentre and Ω²=G(M₁+M₂)/a³.
ModelEarth & cosmosAccretion-powered galactic nuclei and observational inferenceActive galactic nuclei can radiate strongly as matter accretes around a central supermassive black hole.
ModelEarth & cosmosPrimordial nuclear freeze-out and the deuterium bottleneckIn hot Big-Bang nucleosynthesis, neutron–proton conversion initially approaches chemical equilibrium.
ModelEarth & cosmosRecombination, last scattering and reionizationAtomic recombination binds many previously free electrons and lowers photon-scattering opacity.
ModelEarth & cosmosIonized hydrogen regions and the Strömgren photon budgetAn ionization-bounded pure-hydrogen region in steady balance equates absorbed external ionizing photons to net recombinations: Q_H=∫α_B nₑnₚ dV.
ModelEarth & cosmosJeans instability of a local gas modelLinear perturbations in a uniform Newtonian gas model obey ω²=c_s²k²−4πGρ₀.
ModelEarth & cosmosThermal free–free radio emissionElectron–ion acceleration produces continuum emission without capture.
ModelEarth & cosmosSynchrotron emission and electron energy lossA magnetically deflected electron radiates P=2σ_TcU_Bβ²γ²sin²α.
ModelEarth & cosmosThomson inverse-Compton electron lossAn electron in an isotropic soft-photon field loses net power P_IC=(4/3)σ_TcU_radβ²γ² in the Thomson limit.
ModelEarth & cosmosRepresentative stellar fusion isotope pathwaysThe ppI branch builds deuterium and helium-3 before combining two helium-3 nuclei.
ModelEarth & cosmosConserved fluxes across a normal gas shockA steady planar normal shock conserves mass, momentum and total-enthalpy flux across its thin transition: [ρu]=[ρu²+P]=[ρu(h+u²/2)]=0.
ModelEarth & cosmosSolar wind and magnetospheric energy transferThe solar wind carries charged particles, including protons and electrons, and solar magnetic field into interplanetary space.
ModelEarth & cosmosCosmic-ray composition and secondary-particle evidenceIn charged-particle usage, cosmic rays include energetic nuclei and electrons from space.
Empirical findingEarth & cosmosClassical event horizon and Schwarzschild radiusA classical black-hole event horizon is a causal boundary: signals from its interior cannot reach distant future observers in the exterior.
DefinitionEarth & cosmosPoint-mass deflection and Einstein angular radiusA point mass in the weak-field geometric-optics limit deflects light by magnitude α̂=4GM/(c²b).
MethodEarth & cosmosPhoton–baryon acoustic structure in the CMBBefore recombination, scattering tightly coupled photons and baryons.
ModelBiologyCohort survival and net reproductionA cohort life table follows individuals born together.
ModelBiologyEuler–Lotka growth and age structureIn a fixed density-independent age model, the growth factor λ satisfies Σ_{x≥1}λ^(−x)l_xm_x=1.
ModelBiologyLevins patch occupancy and persistenceA simple internally colonized metapopulation tracks the occupied fraction p of equivalent habitat patches.
ModelBiologyOccupancy and imperfect species detectionFailure to detect a species does not establish absence.
MethodBiologyIndividual-based rarefaction and richness samplingFor a collection containing N individuals with N_i in each observed species, the expected species count in a uniformly drawn subset of n individuals without replacement is E[S_n]=Σ_i[1−C(N−N_i,n)/C(N,n)].
MethodBiologyPerturbation, rescue and gene-function evidenceA genetic perturbation tests a causal prediction when the intended change and relevant phenotype are measured against appropriate controls.
MethodChemistryGreen chemistry design principles and lifecycle scopeGreen chemistry evaluates product and process design to reduce hazardous inputs, releases and waste over a stated lifecycle.
Method