nLab black ring

Redirected from "black rings".
Contents

Context

Gravity

gravity, supergravity

Formalism

Definition

Spacetime configurations

Properties

Spacetimes

Quantum theory

Contents

Idea

The Einstein equations for gravity in dimension 5\geq 5 admit black hole solutions whose event horizon is not homeomorphic to an n-sphere, but has different topology. In particular in 5d-gravity and 5d supergravity there are solutions with topology S 1×S 2S^1 \times S^2. These are called black rings.

Their KK-reduction down to 4 dimensions yields again ordinary black holes. This plays a central role in the discussion of black holes in string theory.

References

The first black ring solution was found, in D=5 gravity, in

The first black ring solution was found, in D=5 supergravity, in:

Review:

Dimensional reduction to black holes in D=4 gravity:

On non-uniqueness:

As intersecting black M5-branes wrapped on a 4-manifold times the black ring’s circle:

following

More in the context of D1-D5-brane bound states

See also:

  • Pavan Dharanipragada, Gurmeet Singh Punia, Amitabh Virmani: Non-supersymmetric F1-P black rings [arXiv:2601.04623]

  • Pavan Dharanipragada, Gurmeet Singh Punia, Amitabh Virmani: Index saddle for supersymmetric F1-P black ring [arXiv:2601.04624]

Last revised on January 9, 2026 at 08:19:46. See the history of this page for a list of all contributions to it.