Magnetic solutions to 2+1 dimensional gravity with dilaton field
Takao Koikawa, Takuya Maki, Atsushi Nakamula

TL;DR
This paper presents a general method for solving 2+1 dimensional dilatonic Maxwell-Einstein equations with cosmological constant, identifying solutions with horizons that differ from non-dilatonic cases.
Contribution
It introduces a systematic approach to find solutions in 2+1D dilaton gravity with magnetic fields, revealing new horizon-bearing solutions.
Findings
Some solutions possess horizons unlike non-dilatonic cases
All solutions are static and rotationally symmetric with magnetic and dilaton fields
The method applies to both positive and negative cosmological constants
Abstract
We show a general method to solve 2+1 dimensional dilatonic Maxwell-Einstein equation with a positive or negative cosmological constant. All the physical solutions are listed with assumptions that they are static, rotationally symmetric, and has a nonzero magnetic field and a nonzero dilaton field. On the contrary to the magnetic solution without a dilaton field, some of the present solutions with a dilaton field possess a horizon.
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