Model Predictions of the Results of Interferometric Observations for Stars under Conditions of Strong Gravitational Scattering by Black Holes and Wormholes

TL;DR

This paper models the interferometric visibility amplitude features of stars near the Galactic center to distinguish between black holes, wormholes, and black_white holes based on strong gravitational scattering effects.

Contribution

It introduces a theoretical framework for predicting interferometric observation signatures of different compact objects, aiding in their identification.

Findings

Distinct visibility features for black holes, wormholes, and black_white holes.

Potential to determine the topological nature of the central Galactic object.

Applicability to optical, infrared, and radio interferometric data.

Abstract

The characteristic and distinctive features of the visibility amplitude of interferometric observations for compact objects like stars in the immediate vicinity of the central black hole in our Galaxy are considered. These features are associated with the specifics of strong gravitational scattering of point sources by black holes, wormholes, or black_white holes. The revealed features will help to determine the most important topological characteristics of the central object in our Galaxy: whether this object possesses the properties of only a black hole or also has characteristics unique to wormholes or black_white holes. These studies can be used to interpret the results of optical, infrared, and radio interferometric observations.