Schwarzschild metric (when charge is zero)

GPTKB entity

Statements (50)
Predicate Object
gptkbp:instanceOf solution to Einstein field equations
spacetime metric
gptkbp:appliesTo black holes
stars
planets
gptkbp:coordinates gptkb:Schwarzschild_coordinates
gptkbp:describes gptkb:Schwarzschild_black_hole
gptkb:gravitational_time_dilation
gptkb:perihelion_precession_of_Mercury
gptkb:Shapiro_time_delay
gptkb:innermost_stable_circular_orbit_(ISCO)
gptkb:photon_sphere
gravitational collapse
event horizon
gravitational redshift
singularity
deflection of light by gravity
gravitational field outside a spherically symmetric, non-rotating, uncharged mass
coordinate time for distant observer
escape velocity from massive objects
geodesics in curved spacetime
proper time for infalling observer
gptkbp:hasApplication gptkb:cosmology
astrophysics
gravitational lensing
orbital mechanics
gptkbp:hasEventHorizon gptkb:Schwarzschild_radius
gptkbp:hasEventHorizonAt r = 2GM/c^2
gptkbp:hasNoAngularMomentum true
gptkbp:hasNoElectricCharge true
gptkbp:hasNoMagneticField true
gptkbp:hasSingularityAt r = 0
gptkbp:hasSpecialCase gptkb:Reissner–Nordström_metric
gptkb:Kerr_metric_(when_angular_momentum_is_zero)
https://www.w3.org/2000/01/rdf-schema#label Schwarzschild metric (when charge is zero)
gptkbp:isAsymptoticallyFlat true
gptkbp:isExactSolution true
gptkbp:isLorentzianManifold true
gptkbp:isNonRotating true
gptkbp:isSphericallySymmetric true
gptkbp:isTimeIndependent true
gptkbp:isUncharged true
gptkbp:isVacuumSolution true
gptkbp:metricTensor ds^2 = -(1-2GM/rc^2)c^2dt^2 + (1-2GM/rc^2)^{-1}dr^2 + r^2(dθ^2 + sin^2θ dφ^2)
gptkbp:namedAfter gptkb:Karl_Schwarzschild
gptkbp:publishedIn 1916
gptkbp:staticMethod true
gptkbp:usedIn gptkb:general_relativity
gptkbp:bfsParent gptkb:Reissner–Nordström_metric
gptkbp:bfsLayer 5