http://arxiv.org/abs/1911.03773
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 year-1. The OGRAN narrow band sensitivity at the kilohertz frequency is limited by its acoustical mode thermal noise achieving 10^{-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.
V. Rudenko, Y. Gavrilyuk, A. Gusev, et. al.
Tue, 12 Nov 19
1/84
Comments: 15 pages, 4 figures, for Proceedings of 10th Freedman Seminar Conference, accepted for publication in IJMP_A