nLab Kerr-Newman spacetime

Context

Gravity

gravity, supergravity

Formalism

Definition

Spacetime configurations

Properties

Spacetimes

Quantum theory

Physics

physics, mathematical physics, philosophy of physics

Surveys, textbooks and lecture notes


theory (physics), model (physics)

experiment, measurement, computable physics

Contents

Idea

(…)

black hole spacetimesvanishing angular momentumpositive angular momentum
vanishing chargeSchwarzschild spacetimeKerr spacetime
positive chargeReissner-Nordstrom spacetimeKerr-Newman spacetime


black hole spacetimes
with dark energy
vanishing angular momentumpositive angular momentum
vanishing chargeSchwarzschild-de Sitter spacetimeKerr-de Sitter spacetime
positive chargeReissner-Nordström-de Sitter spacetimeKerr-Newman-de Sitter spacetime


wormhole spacetimesvanishing angular momentum
vanishing chargeSchwarzschild wormhole
positive chargeReissner-Nordström wormhole

References

General

Matching KN black holes to elementary particles

On the similarity between Kerr-Newman black holes (charged and spinning “black 0-branes”) and elementary particles (sigma-model 0-branes) like electrons.

Historical precursor discussion on the possibility of geometrodynamics for fundamental particles:

Seminal observation that the gyromagnetic ratio of the Kerr-Newman black hole is 2, just as the for electron (cf. at anomalous magnetic moment):

Further discussion:

See also:

Last revised on June 24, 2024 at 15:27:38. See the history of this page for a list of all contributions to it.