riassunto2

BH1-2-3 - (BH1) Binary Black Holes as Sources of Multi-messenger Astronomy - (BH2) Black holes in binary stellar systems - (BH3) Black holes in galactic nuclei

Speaker

Zakharov, Alexander

Coauthors

Talk Title

The Galactic Center: possible interpretations of observational data

Abstract

Now there are two basic observational techniques to investigate a gravitational potential at the Galactic Center, namely, a) monitoring the orbits of bright stars near the Galactic Center to reconstruct a gravitational potential; b) measuring a size and a shape of shadows around black hole giving an alternative possibility to evaluate black hole parameters in mm-band with VLBI-technique. At the moment one can use a small relativistic correction approach for stellar orbit analysis (however, in the future the approximation will not be not precise enough due to enormous progress of observational facilities) while now for smallest structure analysis in VLBI observations one really needs a strong gravitational field approximation. We discuss results of observations, their conventional interpretations, tensions between observations and models and possible hints for a new physics from the observational data and tensions between observations and interpretations.

Talk view

BH1-2-3-937ZA1088ER.pdf

 

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