Journal Article

FZJ-2022-04634

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Search for low-energy signals from fast radio bursts with the Borexino detector

Appel, S. ; Bagdasarian, Z. ; Basilico, D. ; Bellini, G. ; Benziger, J. ; Biondi, R. ; Caccianiga, B. ; Calaprice, F. ; Caminata, A. ; Chepurnov, A. ; D’Angelo, D. ; Derbin, A. (Corresponding author) ; Giacinto, A. D. ; Marcello, V. D. ; Ding, X. F. ; Ludovico, A. D. ; Noto, L. D. ; Drachnev, I. ; Franco, D. ; Galbiati, C. ; Ghiano, C. ; Giammarchi, M. ; Goretti, A. ; Göttel, A. S.FZJ* ; Gromov, M. ; Guffanti, D. ; Ianni, A. ; Ianni, A. ; Jany, A. ; Kobychev, V. ; Korga, G. ; Kumaran, S.FZJ* ; Laubenstein, M. ; Litvinovich, E. ; Lombardi, P. ; Lomskaya, I. ; Ludhova, L.FZJ* ; Lukyanchenko, G. ; Machulin, I. ; Martyn, J. ; Meroni, E. ; Miramonti, L. ; Misiaszek, M. ; Muratova, V. ; Nugmanov, R. ; Oberauer, L. ; Orekhov, V. ; Ortica, F. ; Pallavicini, M. ; Pelicci, L.FZJ* ; Penek, Ö.FZJ* ; Pietrofaccia, L. ; Pilipenko, N. ; Pocar, A. ; Raikov, G. ; Ranalli, M. T. ; Ranucci, G. (Corresponding author) ; Razeto, A. ; Re, A. ; Redchuk, M. ; Rossi, N. ; Schönert, S. ; Semenov, D. ; Settanta, G. ; Skorokhvatov, M. ; Singhal, A.FZJ* ; Smirnov, O. ; Sotnikov, A. ; Tartaglia, R. ; Testera, G. ; Unzhakov, E. ; Vishneva, A. ; Vogelaar, R. B. ; Feilitzsch, F. v. ; Wojcik, M. ; Wurm, M. ; Zavatarelli, S. ; Zhutikov, I. ; Zuber, K. ; Zuzel, G.

2022
Springer Heidelberg

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Please use a persistent id in citations: http://hdl.handle.net/2128/32582  doi:10.1140/epjc/s10052-022-10197-0

Abstract: 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.

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Contributing Institute(s):

1. Experimentelle Hadrondynamik (IKP-2)

Research Program(s):

1. 612 - Cosmic Matter in the Laboratory (POF4-612) (POF4-612)

Appears in the scientific report 2022

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