%0 Journal Article
%A Appel, S.
%A Bagdasarian, Z.
%A Basilico, D.
%A Bellini, G.
%A Benziger, J.
%A Biondi, R.
%A Caccianiga, B.
%A Calaprice, F.
%A Caminata, A.
%A Chepurnov, A.
%A D’Angelo, D.
%A Derbin, A.
%A Giacinto, A. Di
%A Marcello, V. Di
%A Ding, X. F.
%A Ludovico, A. Di
%A Noto, L. Di
%A Drachnev, I.
%A Franco, D.
%A Galbiati, C.
%A Ghiano, C.
%A Giammarchi, M.
%A Goretti, A.
%A Göttel, A. S.
%A Gromov, M.
%A Guffanti, D.
%A Ianni, Aldo
%A Ianni, Andrea
%A Jany, A.
%A Kobychev, V.
%A Korga, G.
%A Kumaran, S.
%A Laubenstein, M.
%A Litvinovich, E.
%A Lombardi, P.
%A Lomskaya, I.
%A Ludhova, L.
%A Lukyanchenko, G.
%A Machulin, I.
%A Martyn, J.
%A Meroni, E.
%A Miramonti, L.
%A Misiaszek, M.
%A Muratova, V.
%A Nugmanov, R.
%A Oberauer, L.
%A Orekhov, V.
%A Ortica, F.
%A Pallavicini, M.
%A Pelicci, L.
%A Penek, Ö.
%A Pietrofaccia, L.
%A Pilipenko, N.
%A Pocar, A.
%A Raikov, G.
%A Ranalli, M. T.
%A Ranucci, G.
%A Razeto, A.
%A Re, A.
%A Redchuk, M.
%A Rossi, N.
%A Schönert, S.
%A Semenov, D.
%A Settanta, G.
%A Skorokhvatov, M.
%A Singhal, A.
%A Smirnov, O.
%A Sotnikov, A.
%A Tartaglia, R.
%A Testera, G.
%A Unzhakov, E.
%A Vishneva, A.
%A Vogelaar, R. B.
%A Feilitzsch, F. von
%A Wojcik, M.
%A Wurm, M.
%A Zavatarelli, S.
%A Zhutikov, I.
%A Zuber, K.
%A Zuzel, G.
%T Search for low-energy signals from fast radio bursts with the Borexino detector
%J The European physical journal / C
%V 82
%N 3
%@ 1434-6044
%C Heidelberg
%I Springer
%M FZJ-2022-04634
%P 278
%D 2022
%X The search for neutrino events in correlation with 42 most intense fast radio bursts (FRBs) has been performed using the Borexino dataset from 05/2007 to 06/2021. We have searched for signals with visible energies above 250 keV within a time window of ±1000 s corresponding to detection time of a particular FRB. We also applied an alternative approach based on searching for specific shapes of neutrino-electron scattering spectra in the full exposure data of the Borexino detector. In particular, two incoming neutrino spectra were considered: the monoenergetic line and the spectrum expected from supernovae. The same spectra were considered for electron antineutrinos detected through inverse beta-decay reaction. No statistically significant excess over the background was observed. As a result, the strongest upper limits on FRB-associated neutrino fluences of all flavors have been obtained in the 0.5–50 MeV neutrino energy range.
%F PUB:(DE-HGF)16
%9 Journal Article
%U <Go to ISI:>//WOS:000776965300001
%R 10.1140/epjc/s10052-022-10197-0
%U https://juser.fz-juelich.de/record/911342