The Yilmaz-Rosen and Janis-Newman-Winicour metric solutions in the scalar-Einstein-Gauss-Bonnet $4d$ gravitational model
K.K. Ernazarov

TL;DR
This paper explores scalar-Einstein-Gauss-Bonnet solutions for Yilmaz-Rosen and Janis-Newman-Winicour metrics, revealing exotic matter properties and deriving analytical solutions within scalar-tensor frameworks.
Contribution
It applies a reconstruction method to find new solutions in the sEGB model for specific metrics, highlighting the nature of the scalar field and energy conditions.
Findings
Potential U vanishes for the Yilmaz-Rosen metric.
Scalar field is phantom-like and violates energy conditions.
Derived exact solutions in scalar-tensor theory for JNW metric.
Abstract
We consider the scalar-Einstein-Gauss-Bonnet (sEGB) gravitational model with a scalar field , Einstein and Gauss-Bonnet terms. The model action contains a potential term , a Gauss-Bonnet coupling function and a parameter , where corresponds to the ordinary scalar field, and to the phantom field. In this paper we applied the sEGB reconstruction procedure from our previous work \cite{Er_Ivash} to the Y{\i}lmaz-Rosen metric, a solution potentially describing a quasi-black hole without an event horizon. Within this framework, we also derived analytical solutions based on scalar-tensor theory with minimal coupling. Our results indicate that for this configuration, the potential vanishes and the scalar field is phantom-like. Furthermore, an analysis of the…
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