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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All labels observed (3)

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's equations
surface form: Maxwell 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–Maxwell equations self-linksurface differs
surface form: 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 field equations
surface form: Einstein equations

Einstein–Yang–Mills equations
Kaluza–Klein theory
Maxwell's equations
surface form: Maxwell equations

classical field theory
satisfies Bianchi identities through Einstein tensor
local charge conservation
usedFor Kerr–Newman black hole
surface form: Kerr–Newman solution

Reissner–Nordström metric
surface form: 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

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Input
Subject: Einstein–Maxwell equations
Description of subject: 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.

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 equations
this entity surface form: Einstein–Maxwell theory
Einstein–Maxwell equations hasPart Einstein–Maxwell equations self-linksurface differs
this entity surface form: Einstein field equations with electromagnetic stress–energy tensor
Einstein–Yang–Mills equations generalizes Einstein–Maxwell equations
Kaluza–Klein theory generalizationOf Einstein–Maxwell equations
this entity surface form: Einstein–Maxwell theory