Einstein–Maxwell equations

E78014

The Einstein–Maxwell equations are the coupled set of field equations in general relativity that describe how spacetime curvature and electromagnetic fields interact and influence each other.

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Generate an image of the Einstein–Maxwell equations (The Einstein–Maxwell equations are the coupled set of field equations in general relativity that describe how spacetime curvature and electromagnetic fields interact and influence each other.)

All labels observed (3)

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Statements (51)

Predicate Object
instanceOf equations of motion ⓘ
field equations ⓘ
system of partial differential equations ⓘ
theory in theoretical physics ⓘ
appliesTo curved spacetime ⓘ
spacetimes with charged matter ⓘ
vacuum with electromagnetic fields ⓘ
assumes classical (non-quantum) fields ⓘ
general covariance ⓘ
minimal coupling between gravity and electromagnetism ⓘ
basedOn Einstein field equations ⓘ
Maxwell equations ⓘ
linked to: Maxwell's equations
describes coupling of gravity and electromagnetism ⓘ
interaction between spacetime curvature and electromagnetic fields ⓘ
expressedAs G_{μν} = 8π T_{μν}^{(EM)} + 8π T_{μν}^{(matter)} ⓘ
∇_{[α} F_{βγ]} = 0 ⓘ
∇_{μ} F^{μν} = 4π J^{ν} ⓘ
field classical electromagnetism ⓘ
general relativity ⓘ
gravitational physics ⓘ
relativistic field theory ⓘ
formulatedIn differential geometry ⓘ
tensor calculus ⓘ
hasPart Einstein field equations with electromagnetic stress–energy tensor ⓘ
Maxwell equations with covariant derivatives ⓘ
source-free Maxwell equations in curved spacetime ⓘ
involvesQuantity Ricci curvature tensor R_{μν} ⓘ
current four-vector J^{μ} ⓘ
electromagnetic field tensor F_{μν} ⓘ
electromagnetic stress–energy tensor T_{μν}^{(EM)} ⓘ
metric tensor g_{μν} ⓘ
scalar curvature R ⓘ
relatedTo Einstein equations ⓘ
Einstein–Yang–Mills equations ⓘ
Kaluza–Klein theory ⓘ
Maxwell equations ⓘ
linked to: Maxwell's equations

classical field theory ⓘ
satisfies Bianchi identities through Einstein tensor ⓘ
local charge conservation ⓘ
usedFor Kerr–Newman solution ⓘ
Reissner–Nordström solution ⓘ
electrovacuum solutions ⓘ
modeling charged black holes ⓘ
relativistic stellar models with charge ⓘ
studying gravitational waves with electromagnetic fields ⓘ
uses Einstein tensor ⓘ
Levi-Civita connection ⓘ
Lorentzian metric ⓘ
covariant derivative ⓘ
electromagnetic field tensor ⓘ
stress–energy tensor ⓘ

How these facts were elicited

Referenced by (6)

Full triples — surface form annotated when it differs from this entity's canonical label.

Reissner–Nordström metric → solves → Einstein–Maxwell equations ⓘ
Kerr–Newman black hole → solutionOf → Einstein–Maxwell equations ⓘ
Israel–Carter–Robinson uniqueness theorems → assumes → Einstein–Maxwell theory ⓘ
linked to: Einstein–Maxwell equations
Einstein–Maxwell equations → hasPart → Einstein field equations with electromagnetic stress–energy tensor ⓘ
linked to: Einstein–Maxwell equations
Einstein–Yang–Mills equations → generalizes → Einstein–Maxwell equations ⓘ
Kaluza–Klein theory → generalizationOf → Einstein–Maxwell theory ⓘ
linked to: Einstein–Maxwell equations