pith. sign in

arxiv: gr-qc/0309082 · v1 · pith:NTSFYJU6new · submitted 2003-09-17 · 🌀 gr-qc

Stationary Black Holes with Static and Counterrotating Horizons

Burkhard Kleihaus , Jutta Kunz , Francisco Navarro-L\'erida This is my paper
classification 🌀 gr-qc
keywords blackholesstaticcounterrotatinghorizonhorizonsangularbifurcate
0
0 comments X
read the original abstract

We show that rotating dyonic black holes with static and counterrotating horizon exist in Einstein-Maxwell-dilaton theory when the dilaton coupling constant exceeds the Kaluza-Klein value. The black holes with static horizon bifurcate from the static black holes. Their mass decreases with increasing angular momentum, their horizons are prolate.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Charged, rotating black holes in Einstein-Maxwell-dilaton theory

    gr-qc 2025-06 unverdicted novelty 7.0

    Numerical construction of asymptotically flat charged rotating black holes in EMd theory for arbitrary dilaton coupling gamma, with analysis of parameter space, zero-temperature limits, and hints of non-uniqueness.

  2. Twisted doughnuts: Thick disk torus around equatorial asymmetric black hole

    gr-qc 2026-04 unverdicted novelty 6.0

    Equatorial asymmetry in black hole spacetimes twists thick tori, displacing their centers and cusps away from the equatorial plane in the same direction as Keplerian orbits.