skip to main content

Title: Model predictions of the results of interferometric observations for stars under conditions of strong gravitational scattering by black holes and wormholes

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.
Authors:
; ;  [1]
  1. Russian Academy of Sciences, Astro Space Center, Lebedev Physical Institute (Russian Federation)
Publication Date:
OSTI Identifier:
22472265
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Experimental and Theoretical Physics; Journal Volume: 120; Journal Issue: 5; Other Information: Copyright (c) 2015 Pleiades Publishing, Inc.; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; AMPLITUDES; BLACK HOLES; GRAVITATIONAL FIELDS; INFRARED RADIATION; INTERFEROMETRY; MILKY WAY; RADIOWAVE RADIATION; SCATTERING; STARS; VISIBILITY; VISIBLE RADIATION; WHITE HOLES