Reissner–Nordström Penrose diagram

E68111

The Reissner–Nordström Penrose diagram is a causal spacetime diagram depicting the global structure of a charged, non-rotating black hole, including its multiple horizons and extended regions.


Statements (46)
Predicate Object
instanceOf Penrose diagram
causal spacetime diagram
conformal diagram
assumes electrovacuum solution of Einstein–Maxwell equations
spherical symmetry
describes Reissner–Nordström spacetime
charged non-rotating black hole
distinguishes extremal Reissner–Nordström case
non-extremal Reissner–Nordström case
encodes causal connectivity between different regions
possibility of travel between asymptotic regions in idealized solution
includes maximally extended Reissner–Nordström spacetime
regions separated by Cauchy horizons
regions separated by event horizons
models spacetime of a point charge with mass and electric charge
relatedTo Kerr Penrose diagram
Penrose–Carter diagram
Schwarzschild Penrose diagram
represents Cauchy horizons of a charged black hole
asymptotically flat regions
event horizons of a charged black hole
future null infinity
global causal structure of Reissner–Nordström spacetime
inner horizon of a charged black hole
outer horizon of a charged black hole
past null infinity
spacelike infinity
timelike infinity
timelike singularity
shows black hole regions
causal relationships between events
infinite sequence of black hole and white hole regions
multiple asymptotic regions
null geodesics as 45-degree lines
spacelike curves as horizontal-like curves
timelike geodesics as vertical-like curves
white hole regions
usedFor studying determinism breakdown at Cauchy horizons
studying geodesic completeness
visualizing horizons and singularities
usedIn black hole physics
causal structure analysis
general relativity
theoretical astrophysics
uses conformal compactification
null coordinates

Referenced by (3)
Subject (surface form when different) Predicate
Schwarzschild Penrose diagram
contrastsWith
Kerr Penrose diagram ("Schwarzschild Penrose diagram by having inner and outer horizons")
differsFrom
Kerr Penrose diagram
relatedTo

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