Rotating black holes can have short bristles

DOI10.1016/j.physletb.2014.10.062zbMath1306.83046arXiv1411.2609OpenAlexW2054433098MaRDI QIDQ2257238

Shahar Hod

Publication date: 24 February 2015

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1411.2609

Mathematics Subject Classification ID

Black holes (83C57)

Related Items (6)

Kerr-Newman black holes with scalar hair ⋮ Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime ⋮ Stationary scalar clouds around a BTZ black hole ⋮ Onset of superradiant instabilities in rotating spacetimes of exotic compact objects ⋮ Extremal Kerr-Newman black holes with extremely short charged scalar hair ⋮ Inside black holes with synchronized hair

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• Regular and black hole solutions of Einstein-Yang-Mills dilaton theory
• A MINIMAL MODEL FOR DILATONIC GRAVITY
• Spherically symmetric static SU(2) Einstein–Yang–Mills fields
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Do collapsed boson stars result in new types of black holes?
• Black Holes Have No Short Hair
• A simple proof of a no-hair theorem in Einstein-Higgs theory

This page was built for publication: Rotating black holes can have short bristles