# Rotating Black Holes in Higher Order Gravity

**Authors:** Christos Charmousis, Marco Crisostomi, Ruth Gregory, Nikolaos, Stergioulas

arXiv: 1903.05519 · 2019-10-16

## TL;DR

This paper introduces a new method for constructing rotating black hole solutions with stealth scalar hair in higher order gravity theories, revealing novel scalar-dressed black holes with finite scalar fields at horizons.

## Contribution

It develops a technique for finding black hole solutions with stealth hair and presents a new rotating black hole solution with finite scalar fields at horizons in scalar-tensor theories.

## Key findings

- Existence of Einstein metrics with stealth hair under specific geodesic conditions
- Construction of a scalar-dressed rotating black hole with finite scalar field at horizons
- New insights into black hole solutions in higher order gravity theories

## Abstract

We develop a new technique for finding black hole solutions in modified gravity that have "stealth" hair, i.e., hair whose only gravitational effect is to tune the cosmological constant. We consider scalar-tensor theories in which gravitational waves propagate at the speed of light, and show that Einstein metrics can be painted with stealth hair provided there exists a family of geodesics always normal to spacelike surfaces. We also present a novel scalar-dressed rotating black hole that has finite scalar field at both the black hole and cosmological event horizons.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1903.05519/full.md

## References

25 references — full list in the complete paper: https://tomesphere.com/paper/1903.05519/full.md

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Source: https://tomesphere.com/paper/1903.05519