Revaz Beradze

Revaz Beradze


Research Focus & Metrics

Academic Career Length

11Years (2016-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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10 May 2019 in Monthly Notices of the Royal Astronomical Society
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Journal Article
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RBRevaz Beradze
Revaz Beradze
MGMerab Gogberashvili
Merab Gogberashvili
We want to explain non-observation of electromagnetic counterpart of currently confirmed 10 gravitational wave signals from the black hole mergers assuming their existence in the hidden mirror universe. Mirror matter, which interacts with our world only through gravity, is a candidate of dark matter and its density can exceed ordinary matter density five times. Since mirror world is considered to be colder, star formation there started earlier and mirror black holes had more time to pick up the mass and to create more binary systems within the LIGO reachable zone. Totally we estimate a factor 10 amplification of black holes merging rate in mirror world with respect to our world, which is consistent with the LIGO observations.

27 March 2019 in Physics
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Journal Article
Open access
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RBRevaz Beradze
Revaz Beradze
MGMerab Gogberashvili
Merab Gogberashvili
In this paper we consider the properties of the 10 confirmed by the LIGO (Laser Interferometer Gravitational-Wave Observatory) Collaboration gravitational wave signals from the black hole mergers. We want to explain non-observation of electromagnetic counterpart and higher then expected merging rates of these events, assuming the existence of their sources in the hidden mirror universe. Mirror matter, which interacts with our world only through gravity, is a candidate of dark matter and its density can exceed ordinary matter density five times. Since mirror world is considered to be colder, star formation there started earlier and mirror black holes had more time to pick up the mass and to create more binary systems within the LIGO reachable zone. In total, we estimate factor of 15 amplification of black holes merging rate in mirror world with respect to our world, which is consistent with the LIGO observations.

9 March 2021 in Monthly Notices of the Royal Astronomical Society
Verified
Journal Article
Closed access
PDF file
RBRevaz Beradze
Revaz Beradze
MGMerab Gogberashvili
Merab Gogberashvili
We consider the possibility that LIGO events GW190521, GW190425, and GW190814 may have emerged from the mirror world binaries. Theories of star evolution predict so-called upper and lower mass gaps and masses of these merger components lie in that gaps. In order to explain these challenging events very specific assumptions are required and we argue that such scenarios are order of magnitude more probable in mirror world, where star formation begins earlier and matter density can exceed five times the ordinary matter density.

1 May 2021 in Physics of the Dark Universe
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Journal Article
Closed access
RBRevaz Beradze
Revaz Beradze
MGMerab Gogberashvili
Merab Gogberashvili

23 September 2025
Verified
Conference Paper
Open access
PDF file
RBRevaz Beradze
Revaz Beradze
Manana SvanidzeManana Svanidze
Manana Svanidze
GMGiorgi Macharashvili
Giorgi Macharashvili
AIAbesalom Iashvili
Abesalom Iashvili
VKValeri Kikvadze
Valeri Kikvadze
CCCREDO Collaboration
CREDO Collaboration
The GELATICA project (GEorgian Large-area Angle and TIme Coincidence Array) consists of several cosmic ray detector arrays located in two cities in Georgia. Designed to detect Extensive Air Showers (EAS) with high-precision timing, these observatories aim to reconstruct the arrival directions of cosmic ray showers. GELATICA is the part of the international CREDO collaboration (Cosmic Ray Extremely Distributed Observatory), with a primary goal of searching for Cosmic Ray Ensembles (CRE)—correlated cosmic ray events potentially originating from a common astrophysical or exotic source. This paper presents an overview of GELATICA's instrumentation and methodology, along with an analysis of multi-year data. We evaluate detector performance, characterize the distribution of recorded signals, and assess the potential for detecting CREs via coincident signals across spatially separated arrays. We report the detection of two pairs of events coinciding in time with 0.5 millisecond accuracy. However, the arrival directions of these coincident events do not suggest a common origin. Nevertheless, further data collection and an increased number of observatories could enhance the likelihood of identifying true CRE candidates.

15 June 2019 in arXiv
Verified
Preprint
Open access
PDF file
RBRevaz Beradze
Revaz Beradze
MGMerab Gogberashvili
Merab Gogberashvili
We want to explain non-observation of electromagnetic counterpart of currently confirmed ten gravitational wave signals from the black hole mergers assuming their existence in the hidden mirror universe. Mirror matter, which interacts with our world only through gravity, is a candidate of dark matter and its density can exceed ordinary matter density five times. Since mirror world is considered to be colder, star formation there started earlier and mirror black holes had more time to pick up the mass and to create more binary systems within the LIGO reachable zone. Totally we estimate a factor 10 amplification of black holes merging rate in mirror world with respect to our world, which is consistent with the LIGO observations.