Schwarzschild black hole

Related Overviews

Karl Schwarzschild (1873—1916)


'Schwarzschild black hole' can also refer to...

Schwarzschild black hole

Schwarzschild black hole

Schwarzschild Spacetime and Black Holes

The structure of black hole magnetospheres — I. Schwarzschild black holes

Stability of Higher-Dimensional Schwarzschild Black Holes

Critical properties of spherically symmetric black hole accretion in Schwarzschild geometry

Thermally driven outflows from pair-plasma pressure-mediated shock surfaces around Schwarzschild black holes

Covariant Self-Force Regularization of a Particle Orbiting a Schwarzschild Black Hole Mode Decomposition Regularization

Gravitational Waves by a Particle in Circular Orbits around a Schwarzschild Black Hole 5.5 Post-Newtonian Formula

Oscillations of Static Discs around Schwarzschild Black Holes: Effect of Self-Gravitation

Stationary axisymmetric configuration of the resistive thick accretion tori around a Schwarzschild black hole

Disc formation from tidal disruptions of stars on eccentric orbits by Schwarzschild black holes

Axisymmetric Bondi–Hoyle accretion on to a Schwarzschild black hole: shock cone vibrations

A Structure Model for Black Holes: Atomic-Like Structure, Quantization and the Minimum Schwarzschild Radius

Self-Force on a Scalar Charge in Circular Orbit around a Schwarzschild Black Hole

Gravitational frequency shift of light in equatorial plane of a radially moving Schwarzschild black hole

Gravitational Waves from a Particle in Circular Orbits around a Schwarzschild Black Hole to the 22nd Post-Newtonian Order

Stability of the Schwarzschild–de Sitter black hole in the dRGT massive gravity theory

Exploring the effects of pressure on the radial accretion of dark matter by a Schwarzschild supermassive black hole


More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics


Show Summary Details

Quick Reference

A non-rotating black hole with no electrical charge. This is the simplest case of a black hole, predicted by K. Schwarzschild in 1916, but is unlikely to be found in reality. The most likely form for black holes is the rotating Kerr black hole.

Subjects: Astronomy and Astrophysics.

Reference entries

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.