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Astrophysics > High Energy Astrophysical Phenomena

arXiv:1607.05649 (astro-ph)
[Submitted on 19 Jul 2016 (v1), last revised 20 Oct 2016 (this version, v2)]

Title:A search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts with Borexino

Authors:M. Agostini, K. Altenmeuller, S. Appel, V. Atroshchenko, G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, B. Caccianiga, F. Calaprice, A. Caminata, M. Carlini, P. Cavalcante, A. Chepurnov, K. Choi, D. D'Angelo, S. Davini, H. de Kerret, A. Derbin, L. Di Noto, I. Drachnev, A. Etenko, K. Fomenko, D. Franco, F. Gabriele, C. Galbiati, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, M. Gromov, C. Hagner, E. Hungerford, Aldo Ianni, Andrea Ianni, A. Jany, K. Jedrzejczak, D. Jeschke, V. Kobychev, D. Korablev, G. Korga, D. Kryn, M. Laubenstein, B. Lehnert, E. Litvinovich, F. Lombardi, P. Lombardi, L. Ludhova, G. Lukyanchenko, I. Machulin, S. Manecki, W. Maneschg, G. Manuzio, S. Marcocci, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, M. Montuschi, P. Mosteiro, V. Muratova, B. Neumair, L. Oberauer, M. Obolensky, F. Ortica, M. Pallavicini, L. Papp, A. Pocar, G. Ranucci, A. Razeto, A. Re, A. Romani, R. Roncin, N. Rossi, S. Scheonert, D. Semenov, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, J. Thurn, M. Toropova, E. Unzhakov, A. Vishneva, R.B. Vogelaar, F. von Feilitzsch, H. Wang, S. Weinz, J. Winter, M. Wojcik, M. Wurm, Z. Yokley, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel
View a PDF of the paper titled A search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts with Borexino, by M. Agostini and 99 other authors
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Abstract:A search for neutrino and antineutrino events correlated with 2,350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ($\bar{\nu}_e$) that inverse beta decay on protons with energies from 1.8\,MeV to 15\,MeV and set the best limit on the neutrino fluence from GRBs below 8\,MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino fluence of all flavors and species below 7\,MeV. Finally, time correlations between GRBs and bursts of events are investigated. Our analysis combines two semi-independent data acquisition systems for the first time: the primary Borexino readout optimized for solar neutrino physics up to a few MeV, and a fast waveform digitizer system tuned for events above 1\,MeV.
Comments: 10 pages, 6 figures
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE)
Cite as: arXiv:1607.05649 [astro-ph.HE]
  (or arXiv:1607.05649v2 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.1607.05649
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1016/j.astropartphys.2016.10.004
DOI(s) linking to related resources

Submission history

From: Livia Ludhova [view email]
[v1] Tue, 19 Jul 2016 16:20:50 UTC (216 KB)
[v2] Thu, 20 Oct 2016 08:02:47 UTC (217 KB)
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