Classical and Quantum GravityNo Access

Gravitational wave detector OGRAN as multi-messenger project of RAS-MSU

V. N. Rudenko

Sternberg Astronomical Institute, Lomonosov State University, Universitetskii prospect 13, Moscow 119234, Russia

Baksan Neutrino Observatory of INR RAS, Neutrino village, Elbrus district, 361609, Kabardino-Balkar Republic, Russia

E-mail Address: valentin.rudenko@gmail.com

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Yu. M. Gavrilyuk

Baksan Neutrino Observatory of INR RAS, Neutrino village, Elbrus district, 361609, Kabardino-Balkar Republic, Russia

Sternberg Astronomical Institute, Lomonosov State University, Universitetskii prospect 13, Moscow 119234, Russia

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A. V. Gusev

Sternberg Astronomical Institute, Lomonosov State University, Universitetskii prospect 13, Moscow 119234, Russia

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D. P. Krichevskiy

Bauman Moscow State Technical University, Physics Department, 2-nd Baumanskaya street 5, building 1, Moscow 105005, Russia

Sternberg Astronomical Institute, Lomonosov State University, Universitetskii prospect 13, Moscow 119234, Russia

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S. I. Oreshkin

Sternberg Astronomical Institute, Lomonosov State University, Universitetskii prospect 13, Moscow 119234, Russia

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S. M. Popov

Sternberg Astronomical Institute, Lomonosov State University, Universitetskii prospect 13, Moscow 119234, Russia

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I. S. Yudin

Moscow Institute of Physics and Technology, Institutskiy per. 9, Dolgoprudny, 141701, Moscow Region, Russia

Sternberg Astronomical Institute, Lomonosov State University, Universitetskii prospect 13, Moscow 119234, Russia

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https://doi.org/10.1142/S0217751X20400072Cited by:4 (Source: Crossref)

This article is part of the issue:

SPECIAL ISSUE — Selected papers from the Tenth Alexander Friedmann International Seminar on Gravitation and Cosmology, Peter the Great Saint Petersburg Polytechnic University, Saint Petersburg, Russia, 24–28 June 2019
Editors: V. M. Mostepanenko and E. N. Velichko

Abstract

Modernized version of the combined opto-acoustical gravitational wave detector OGRAN is presented. Located in the deep underground of the Baksan Neutrino Observatory this setup is aimed to work on the program of collapsing stars searching for in multi-channel manner with the neutrino telescope BUST. The both instruments have the sensitivity allowing a registration of collapses in our Galaxy as rare events with the estimated probability $0.03$ $0.03$ year $^{-} 1$ $^{-} 1$ . The OGRAN narrow band sensitivity at the kilohertz frequency is limited by its acoustical mode thermal noise achieving $1 0^{- 20}$ $1 0^{- 20}$ in term of metric perturbations. A possible algorithm of the joint data analysis for the both instruments is developed and resulting formulae of the right detection probability are given. A future increasing of the OGRAN sensitivity associated with the moderate cooling (nitrogen temperature) of the acoustical mode is also discussed.

Keywords:

PACS: 04.08.Nn, 95.55.Vj

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