A metric solution for rotating black holes embedded in dark matter halos with central spikes

TL;DR

This paper introduces an exact analytic metric for rotating black holes embedded in dark matter halos with central density spikes, extending previous models to include rotation and anisotropy.

Contribution

It provides a novel exact solution of Einstein's field equations that models rotating black holes with dark matter halos featuring central spikes, generalizing prior spherically symmetric metrics.

Findings

The metric is asymptotically flat and reduces to known solutions in specific limits.

It models anisotropic spacetime due to the dark matter spike and metric discontinuity.

Application to various gravitational systems demonstrates its physical relevance.

Abstract

We propose an analytic metric describing rotating black holes surrounded by generic dark matter halos. This metric is an exact solution of the field equations that incorporates a dark matter halo with a central density spike in the vicinity of the black hole. The dark matter profile is truncated at a radius close to the horizon, in accordance with analyses based on adiabatic invariants, so that the energy density as well as the radial and tangential pressures vanish identically beyond this point. The presence of the spike and the associated metric discontinuity implies that the spacetime is intrinsically anisotropic. The resulting geometry is asymptotically flat and reduces to several well-known cases under suitable limits. In particular, it generalizes the spherically symmetric metric proposed by Cardoso {\it et al.} to the case of rotating black holes. We discuss the physical interpretation of the model parameters and illustrate the metric by applying it to several specific gravitational systems.