Photon Sphere for a Dilatonic Dyonic Black Hole in a Model with an Abelian Gauge Field and a Scalar Field

2025

Full text Open access: Green Metadata (CSL-JSON)
DOI 10.1134/s0202289325700471
Data confidence 70 medium
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

A dilatonic dyonic black hole solution with the gravitational radius $$2\mu$$ and two charges $$Q_{1}$$ and $$Q_{2}$$ (electric and magnetic ones) is considered in a gravitational 4D model with one scalar field and one 2-form, with the dilatonic coupling constant $$\lambda=\pm 1/\sqrt{2}$$ . Circular null geodesics are explored. The 3rd order polynomial master equation for the radius $$R_{0}$$ of photon sphere is studied. There is only one solution with $$R_{0}>2\mu$$ . The circular null geodesics are shown to be unstable. The black hole shadow is studied, and relations for the shadow angle and critical impact parameter are obtained.