Search for low-energy signals from fast radio bursts with the Borexino detector
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 $$\pm \, 1000$$ ± 1000 s corresponding...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
S. Appel [verfasserIn] Z. Bagdasarian [verfasserIn] D. Basilico [verfasserIn] G. Bellini [verfasserIn] J. Benziger [verfasserIn] R. Biondi [verfasserIn] B. Caccianiga [verfasserIn] F. Calaprice [verfasserIn] A. Caminata [verfasserIn] A. Chepurnov [verfasserIn] D. D’Angelo [verfasserIn] A. Derbin [verfasserIn] A. Di Giacinto [verfasserIn] V. Di Marcello [verfasserIn] X. F. Ding [verfasserIn] A. Di Ludovico [verfasserIn] L. Di Noto [verfasserIn] I. Drachnev [verfasserIn] D. Franco [verfasserIn] C. Galbiati [verfasserIn] C. Ghiano [verfasserIn] M. Giammarchi [verfasserIn] A. Goretti [verfasserIn] A. S. Göttel [verfasserIn] M. Gromov [verfasserIn] D. Guffanti [verfasserIn] Aldo Ianni [verfasserIn] Andrea Ianni [verfasserIn] A. Jany [verfasserIn] V. Kobychev [verfasserIn] G. Korga [verfasserIn] S. Kumaran [verfasserIn] M. Laubenstein [verfasserIn] E. Litvinovich [verfasserIn] P. Lombardi [verfasserIn] I. Lomskaya [verfasserIn] L. Ludhova [verfasserIn] G. Lukyanchenko [verfasserIn] I. Machulin [verfasserIn] J. Martyn [verfasserIn] E. Meroni [verfasserIn] L. Miramonti [verfasserIn] M. Misiaszek [verfasserIn] V. Muratova [verfasserIn] R. Nugmanov [verfasserIn] L. Oberauer [verfasserIn] V. Orekhov [verfasserIn] F. Ortica [verfasserIn] M. Pallavicini [verfasserIn] L. Pelicci [verfasserIn] Ö. Penek [verfasserIn] L. Pietrofaccia [verfasserIn] N. Pilipenko [verfasserIn] A. Pocar [verfasserIn] G. Raikov [verfasserIn] M. T. Ranalli [verfasserIn] G. Ranucci [verfasserIn] A. Razeto [verfasserIn] A. Re [verfasserIn] M. Redchuk [verfasserIn] N. Rossi [verfasserIn] S. Schönert [verfasserIn] D. Semenov [verfasserIn] G. Settanta [verfasserIn] M. Skorokhvatov [verfasserIn] A. Singhal [verfasserIn] O. Smirnov [verfasserIn] A. Sotnikov [verfasserIn] R. Tartaglia [verfasserIn] G. Testera [verfasserIn] E. Unzhakov [verfasserIn] A. Vishneva [verfasserIn] R. B. Vogelaar [verfasserIn] F. von Feilitzsch [verfasserIn] M. Wojcik [verfasserIn] M. Wurm [verfasserIn] S. Zavatarelli [verfasserIn] I. Zhutikov [verfasserIn] K. Zuber [verfasserIn] G. Zuzel [verfasserIn] Borexino Collaboration [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 |
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| Übergeordnetes Werk: |
In: European Physical Journal C: Particles and Fields - SpringerOpen, 2017, 82(2022), 3, Seite 13 |
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| Übergeordnetes Werk: |
volume:82 ; year:2022 ; number:3 ; pages:13 |
| Links: |
Link aufrufen |
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| DOI / URN: |
10.1140/epjc/s10052-022-10197-0 |
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DOAJ057833176 |
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| 520 | |a 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 $$\pm \, 1000$$ ± 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. | ||
| 653 | 0 | |a Astrophysics | |
| 653 | 0 | |a Nuclear and particle physics. Atomic energy. Radioactivity | |
| 700 | 0 | |a Z. Bagdasarian |e verfasserin |4 aut | |
| 700 | 0 | |a D. Basilico |e verfasserin |4 aut | |
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10.1140/epjc/s10052-022-10197-0 doi (DE-627)DOAJ057833176 (DE-599)DOAJeeb0eeeff1474632a64d38603275bdf1 DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 S. Appel verfasserin aut Search for low-energy signals from fast radio bursts with the Borexino detector 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 $$\pm \, 1000$$ ± 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. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity Z. Bagdasarian verfasserin aut D. Basilico verfasserin aut G. Bellini verfasserin aut J. Benziger verfasserin aut R. Biondi verfasserin aut B. Caccianiga verfasserin aut F. Calaprice verfasserin aut A. Caminata verfasserin aut A. Chepurnov verfasserin aut D. D’Angelo verfasserin aut A. Derbin verfasserin aut A. Di Giacinto verfasserin aut V. Di Marcello verfasserin aut X. F. Ding verfasserin aut A. Di Ludovico verfasserin aut L. Di Noto verfasserin aut I. Drachnev verfasserin aut D. Franco verfasserin aut C. Galbiati verfasserin aut C. Ghiano verfasserin aut M. Giammarchi verfasserin aut A. Goretti verfasserin aut A. S. Göttel verfasserin aut M. Gromov verfasserin aut D. Guffanti verfasserin aut Aldo Ianni verfasserin aut Andrea Ianni verfasserin aut A. Jany verfasserin aut V. Kobychev verfasserin aut G. Korga verfasserin aut S. Kumaran verfasserin aut M. Laubenstein verfasserin aut E. Litvinovich verfasserin aut P. Lombardi verfasserin aut I. Lomskaya verfasserin aut L. Ludhova verfasserin aut G. Lukyanchenko verfasserin aut I. Machulin verfasserin aut J. Martyn verfasserin aut E. Meroni verfasserin aut L. Miramonti verfasserin aut M. Misiaszek verfasserin aut V. Muratova verfasserin aut R. Nugmanov verfasserin aut L. Oberauer verfasserin aut V. Orekhov verfasserin aut F. Ortica verfasserin aut M. Pallavicini verfasserin aut L. Pelicci verfasserin aut Ö. Penek verfasserin aut L. Pietrofaccia verfasserin aut N. Pilipenko verfasserin aut A. Pocar verfasserin aut G. Raikov verfasserin aut M. T. Ranalli verfasserin aut G. Ranucci verfasserin aut A. Razeto verfasserin aut A. Re verfasserin aut M. Redchuk verfasserin aut N. Rossi verfasserin aut S. Schönert verfasserin aut D. Semenov verfasserin aut G. Settanta verfasserin aut M. Skorokhvatov verfasserin aut A. Singhal verfasserin aut O. Smirnov verfasserin aut A. Sotnikov verfasserin aut R. Tartaglia verfasserin aut G. Testera verfasserin aut E. Unzhakov verfasserin aut A. Vishneva verfasserin aut R. B. Vogelaar verfasserin aut F. von Feilitzsch verfasserin aut M. Wojcik verfasserin aut M. Wurm verfasserin aut S. Zavatarelli verfasserin aut I. Zhutikov verfasserin aut K. Zuber verfasserin aut G. Zuzel verfasserin aut Borexino Collaboration verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 82(2022), 3, Seite 13 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:82 year:2022 number:3 pages:13 https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/article/eeb0eeeff1474632a64d38603275bdf1 kostenfrei https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 3 13 |
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10.1140/epjc/s10052-022-10197-0 doi (DE-627)DOAJ057833176 (DE-599)DOAJeeb0eeeff1474632a64d38603275bdf1 DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 S. Appel verfasserin aut Search for low-energy signals from fast radio bursts with the Borexino detector 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 $$\pm \, 1000$$ ± 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. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity Z. Bagdasarian verfasserin aut D. Basilico verfasserin aut G. Bellini verfasserin aut J. Benziger verfasserin aut R. Biondi verfasserin aut B. Caccianiga verfasserin aut F. Calaprice verfasserin aut A. Caminata verfasserin aut A. Chepurnov verfasserin aut D. D’Angelo verfasserin aut A. Derbin verfasserin aut A. Di Giacinto verfasserin aut V. Di Marcello verfasserin aut X. F. Ding verfasserin aut A. Di Ludovico verfasserin aut L. Di Noto verfasserin aut I. Drachnev verfasserin aut D. Franco verfasserin aut C. Galbiati verfasserin aut C. Ghiano verfasserin aut M. Giammarchi verfasserin aut A. Goretti verfasserin aut A. S. Göttel verfasserin aut M. Gromov verfasserin aut D. Guffanti verfasserin aut Aldo Ianni verfasserin aut Andrea Ianni verfasserin aut A. Jany verfasserin aut V. Kobychev verfasserin aut G. Korga verfasserin aut S. Kumaran verfasserin aut M. Laubenstein verfasserin aut E. Litvinovich verfasserin aut P. Lombardi verfasserin aut I. Lomskaya verfasserin aut L. Ludhova verfasserin aut G. Lukyanchenko verfasserin aut I. Machulin verfasserin aut J. Martyn verfasserin aut E. Meroni verfasserin aut L. Miramonti verfasserin aut M. Misiaszek verfasserin aut V. Muratova verfasserin aut R. Nugmanov verfasserin aut L. Oberauer verfasserin aut V. Orekhov verfasserin aut F. Ortica verfasserin aut M. Pallavicini verfasserin aut L. Pelicci verfasserin aut Ö. Penek verfasserin aut L. Pietrofaccia verfasserin aut N. Pilipenko verfasserin aut A. Pocar verfasserin aut G. Raikov verfasserin aut M. T. Ranalli verfasserin aut G. Ranucci verfasserin aut A. Razeto verfasserin aut A. Re verfasserin aut M. Redchuk verfasserin aut N. Rossi verfasserin aut S. Schönert verfasserin aut D. Semenov verfasserin aut G. Settanta verfasserin aut M. Skorokhvatov verfasserin aut A. Singhal verfasserin aut O. Smirnov verfasserin aut A. Sotnikov verfasserin aut R. Tartaglia verfasserin aut G. Testera verfasserin aut E. Unzhakov verfasserin aut A. Vishneva verfasserin aut R. B. Vogelaar verfasserin aut F. von Feilitzsch verfasserin aut M. Wojcik verfasserin aut M. Wurm verfasserin aut S. Zavatarelli verfasserin aut I. Zhutikov verfasserin aut K. Zuber verfasserin aut G. Zuzel verfasserin aut Borexino Collaboration verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 82(2022), 3, Seite 13 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:82 year:2022 number:3 pages:13 https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/article/eeb0eeeff1474632a64d38603275bdf1 kostenfrei https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 3 13 |
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10.1140/epjc/s10052-022-10197-0 doi (DE-627)DOAJ057833176 (DE-599)DOAJeeb0eeeff1474632a64d38603275bdf1 DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 S. Appel verfasserin aut Search for low-energy signals from fast radio bursts with the Borexino detector 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 $$\pm \, 1000$$ ± 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. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity Z. Bagdasarian verfasserin aut D. Basilico verfasserin aut G. Bellini verfasserin aut J. Benziger verfasserin aut R. Biondi verfasserin aut B. Caccianiga verfasserin aut F. Calaprice verfasserin aut A. Caminata verfasserin aut A. Chepurnov verfasserin aut D. D’Angelo verfasserin aut A. Derbin verfasserin aut A. Di Giacinto verfasserin aut V. Di Marcello verfasserin aut X. F. Ding verfasserin aut A. Di Ludovico verfasserin aut L. Di Noto verfasserin aut I. Drachnev verfasserin aut D. Franco verfasserin aut C. Galbiati verfasserin aut C. Ghiano verfasserin aut M. Giammarchi verfasserin aut A. Goretti verfasserin aut A. S. Göttel verfasserin aut M. Gromov verfasserin aut D. Guffanti verfasserin aut Aldo Ianni verfasserin aut Andrea Ianni verfasserin aut A. Jany verfasserin aut V. Kobychev verfasserin aut G. Korga verfasserin aut S. Kumaran verfasserin aut M. Laubenstein verfasserin aut E. Litvinovich verfasserin aut P. Lombardi verfasserin aut I. Lomskaya verfasserin aut L. Ludhova verfasserin aut G. Lukyanchenko verfasserin aut I. Machulin verfasserin aut J. Martyn verfasserin aut E. Meroni verfasserin aut L. Miramonti verfasserin aut M. Misiaszek verfasserin aut V. Muratova verfasserin aut R. Nugmanov verfasserin aut L. Oberauer verfasserin aut V. Orekhov verfasserin aut F. Ortica verfasserin aut M. Pallavicini verfasserin aut L. Pelicci verfasserin aut Ö. Penek verfasserin aut L. Pietrofaccia verfasserin aut N. Pilipenko verfasserin aut A. Pocar verfasserin aut G. Raikov verfasserin aut M. T. Ranalli verfasserin aut G. Ranucci verfasserin aut A. Razeto verfasserin aut A. Re verfasserin aut M. Redchuk verfasserin aut N. Rossi verfasserin aut S. Schönert verfasserin aut D. Semenov verfasserin aut G. Settanta verfasserin aut M. Skorokhvatov verfasserin aut A. Singhal verfasserin aut O. Smirnov verfasserin aut A. Sotnikov verfasserin aut R. Tartaglia verfasserin aut G. Testera verfasserin aut E. Unzhakov verfasserin aut A. Vishneva verfasserin aut R. B. Vogelaar verfasserin aut F. von Feilitzsch verfasserin aut M. Wojcik verfasserin aut M. Wurm verfasserin aut S. Zavatarelli verfasserin aut I. Zhutikov verfasserin aut K. Zuber verfasserin aut G. Zuzel verfasserin aut Borexino Collaboration verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 82(2022), 3, Seite 13 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:82 year:2022 number:3 pages:13 https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/article/eeb0eeeff1474632a64d38603275bdf1 kostenfrei https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 3 13 |
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10.1140/epjc/s10052-022-10197-0 doi (DE-627)DOAJ057833176 (DE-599)DOAJeeb0eeeff1474632a64d38603275bdf1 DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 S. Appel verfasserin aut Search for low-energy signals from fast radio bursts with the Borexino detector 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 $$\pm \, 1000$$ ± 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. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity Z. Bagdasarian verfasserin aut D. Basilico verfasserin aut G. Bellini verfasserin aut J. Benziger verfasserin aut R. Biondi verfasserin aut B. Caccianiga verfasserin aut F. Calaprice verfasserin aut A. Caminata verfasserin aut A. Chepurnov verfasserin aut D. D’Angelo verfasserin aut A. Derbin verfasserin aut A. Di Giacinto verfasserin aut V. Di Marcello verfasserin aut X. F. Ding verfasserin aut A. Di Ludovico verfasserin aut L. Di Noto verfasserin aut I. Drachnev verfasserin aut D. Franco verfasserin aut C. Galbiati verfasserin aut C. Ghiano verfasserin aut M. Giammarchi verfasserin aut A. Goretti verfasserin aut A. S. Göttel verfasserin aut M. Gromov verfasserin aut D. Guffanti verfasserin aut Aldo Ianni verfasserin aut Andrea Ianni verfasserin aut A. Jany verfasserin aut V. Kobychev verfasserin aut G. Korga verfasserin aut S. Kumaran verfasserin aut M. Laubenstein verfasserin aut E. Litvinovich verfasserin aut P. Lombardi verfasserin aut I. Lomskaya verfasserin aut L. Ludhova verfasserin aut G. Lukyanchenko verfasserin aut I. Machulin verfasserin aut J. Martyn verfasserin aut E. Meroni verfasserin aut L. Miramonti verfasserin aut M. Misiaszek verfasserin aut V. Muratova verfasserin aut R. Nugmanov verfasserin aut L. Oberauer verfasserin aut V. Orekhov verfasserin aut F. Ortica verfasserin aut M. Pallavicini verfasserin aut L. Pelicci verfasserin aut Ö. Penek verfasserin aut L. Pietrofaccia verfasserin aut N. Pilipenko verfasserin aut A. Pocar verfasserin aut G. Raikov verfasserin aut M. T. Ranalli verfasserin aut G. Ranucci verfasserin aut A. Razeto verfasserin aut A. Re verfasserin aut M. Redchuk verfasserin aut N. Rossi verfasserin aut S. Schönert verfasserin aut D. Semenov verfasserin aut G. Settanta verfasserin aut M. Skorokhvatov verfasserin aut A. Singhal verfasserin aut O. Smirnov verfasserin aut A. Sotnikov verfasserin aut R. Tartaglia verfasserin aut G. Testera verfasserin aut E. Unzhakov verfasserin aut A. Vishneva verfasserin aut R. B. Vogelaar verfasserin aut F. von Feilitzsch verfasserin aut M. Wojcik verfasserin aut M. Wurm verfasserin aut S. Zavatarelli verfasserin aut I. Zhutikov verfasserin aut K. Zuber verfasserin aut G. Zuzel verfasserin aut Borexino Collaboration verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 82(2022), 3, Seite 13 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:82 year:2022 number:3 pages:13 https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/article/eeb0eeeff1474632a64d38603275bdf1 kostenfrei https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 3 13 |
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10.1140/epjc/s10052-022-10197-0 doi (DE-627)DOAJ057833176 (DE-599)DOAJeeb0eeeff1474632a64d38603275bdf1 DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 S. Appel verfasserin aut Search for low-energy signals from fast radio bursts with the Borexino detector 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 $$\pm \, 1000$$ ± 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. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity Z. Bagdasarian verfasserin aut D. Basilico verfasserin aut G. Bellini verfasserin aut J. Benziger verfasserin aut R. Biondi verfasserin aut B. Caccianiga verfasserin aut F. Calaprice verfasserin aut A. Caminata verfasserin aut A. Chepurnov verfasserin aut D. D’Angelo verfasserin aut A. Derbin verfasserin aut A. Di Giacinto verfasserin aut V. Di Marcello verfasserin aut X. F. Ding verfasserin aut A. Di Ludovico verfasserin aut L. Di Noto verfasserin aut I. Drachnev verfasserin aut D. Franco verfasserin aut C. Galbiati verfasserin aut C. Ghiano verfasserin aut M. Giammarchi verfasserin aut A. Goretti verfasserin aut A. S. Göttel verfasserin aut M. Gromov verfasserin aut D. Guffanti verfasserin aut Aldo Ianni verfasserin aut Andrea Ianni verfasserin aut A. Jany verfasserin aut V. Kobychev verfasserin aut G. Korga verfasserin aut S. Kumaran verfasserin aut M. Laubenstein verfasserin aut E. Litvinovich verfasserin aut P. Lombardi verfasserin aut I. Lomskaya verfasserin aut L. Ludhova verfasserin aut G. Lukyanchenko verfasserin aut I. Machulin verfasserin aut J. Martyn verfasserin aut E. Meroni verfasserin aut L. Miramonti verfasserin aut M. Misiaszek verfasserin aut V. Muratova verfasserin aut R. Nugmanov verfasserin aut L. Oberauer verfasserin aut V. Orekhov verfasserin aut F. Ortica verfasserin aut M. Pallavicini verfasserin aut L. Pelicci verfasserin aut Ö. Penek verfasserin aut L. Pietrofaccia verfasserin aut N. Pilipenko verfasserin aut A. Pocar verfasserin aut G. Raikov verfasserin aut M. T. Ranalli verfasserin aut G. Ranucci verfasserin aut A. Razeto verfasserin aut A. Re verfasserin aut M. Redchuk verfasserin aut N. Rossi verfasserin aut S. Schönert verfasserin aut D. Semenov verfasserin aut G. Settanta verfasserin aut M. Skorokhvatov verfasserin aut A. Singhal verfasserin aut O. Smirnov verfasserin aut A. Sotnikov verfasserin aut R. Tartaglia verfasserin aut G. Testera verfasserin aut E. Unzhakov verfasserin aut A. Vishneva verfasserin aut R. B. Vogelaar verfasserin aut F. von Feilitzsch verfasserin aut M. Wojcik verfasserin aut M. Wurm verfasserin aut S. Zavatarelli verfasserin aut I. Zhutikov verfasserin aut K. Zuber verfasserin aut G. Zuzel verfasserin aut Borexino Collaboration verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 82(2022), 3, Seite 13 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:82 year:2022 number:3 pages:13 https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/article/eeb0eeeff1474632a64d38603275bdf1 kostenfrei https://doi.org/10.1140/epjc/s10052-022-10197-0 kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 3 13 |
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European Physical Journal C: Particles and Fields |
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S. Appel @@aut@@ Z. Bagdasarian @@aut@@ D. Basilico @@aut@@ G. Bellini @@aut@@ J. Benziger @@aut@@ R. Biondi @@aut@@ B. Caccianiga @@aut@@ F. Calaprice @@aut@@ A. Caminata @@aut@@ A. Chepurnov @@aut@@ D. D’Angelo @@aut@@ A. Derbin @@aut@@ A. Di Giacinto @@aut@@ V. Di Marcello @@aut@@ X. F. Ding @@aut@@ A. Di Ludovico @@aut@@ L. Di Noto @@aut@@ I. Drachnev @@aut@@ D. Franco @@aut@@ C. Galbiati @@aut@@ C. Ghiano @@aut@@ M. Giammarchi @@aut@@ A. Goretti @@aut@@ A. S. Göttel @@aut@@ M. Gromov @@aut@@ D. Guffanti @@aut@@ Aldo Ianni @@aut@@ Andrea Ianni @@aut@@ A. Jany @@aut@@ V. Kobychev @@aut@@ G. Korga @@aut@@ S. Kumaran @@aut@@ M. Laubenstein @@aut@@ E. Litvinovich @@aut@@ P. Lombardi @@aut@@ I. Lomskaya @@aut@@ L. Ludhova @@aut@@ G. Lukyanchenko @@aut@@ I. Machulin @@aut@@ J. Martyn @@aut@@ E. Meroni @@aut@@ L. Miramonti @@aut@@ M. Misiaszek @@aut@@ V. Muratova @@aut@@ R. Nugmanov @@aut@@ L. Oberauer @@aut@@ V. Orekhov @@aut@@ F. Ortica @@aut@@ M. Pallavicini @@aut@@ L. Pelicci @@aut@@ Ö. Penek @@aut@@ L. Pietrofaccia @@aut@@ N. Pilipenko @@aut@@ A. Pocar @@aut@@ G. Raikov @@aut@@ M. T. Ranalli @@aut@@ G. Ranucci @@aut@@ A. Razeto @@aut@@ A. Re @@aut@@ M. Redchuk @@aut@@ N. Rossi @@aut@@ S. Schönert @@aut@@ D. Semenov @@aut@@ G. Settanta @@aut@@ M. Skorokhvatov @@aut@@ A. Singhal @@aut@@ O. Smirnov @@aut@@ A. Sotnikov @@aut@@ R. Tartaglia @@aut@@ G. Testera @@aut@@ E. Unzhakov @@aut@@ A. Vishneva @@aut@@ R. B. Vogelaar @@aut@@ F. von Feilitzsch @@aut@@ M. Wojcik @@aut@@ M. Wurm @@aut@@ S. Zavatarelli @@aut@@ I. Zhutikov @@aut@@ K. Zuber @@aut@@ G. Zuzel @@aut@@ Borexino Collaboration @@aut@@ |
| publishDateDaySort_date |
2022-01-01T00:00:00Z |
| hierarchy_top_id |
253722934 |
| id |
DOAJ057833176 |
| language_de |
englisch |
| fullrecord |
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Appel</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Search for low-energy signals from fast radio bursts with the Borexino detector</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2022</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">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 $$\pm \, 1000$$ ± 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.</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Astrophysics</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Nuclear and particle physics. 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S. Appel Z. Bagdasarian D. Basilico G. Bellini J. Benziger R. Biondi B. Caccianiga F. Calaprice A. Caminata A. Chepurnov D. D’Angelo A. Derbin A. Di Giacinto V. Di Marcello X. F. Ding A. Di Ludovico L. Di Noto I. Drachnev D. Franco C. Galbiati C. Ghiano M. Giammarchi A. Goretti A. S. Göttel M. Gromov D. Guffanti Aldo Ianni Andrea Ianni A. Jany V. Kobychev G. Korga S. Kumaran M. Laubenstein E. Litvinovich P. Lombardi I. Lomskaya L. Ludhova G. Lukyanchenko I. Machulin J. Martyn E. Meroni L. Miramonti M. Misiaszek V. Muratova R. Nugmanov L. Oberauer V. Orekhov F. Ortica M. Pallavicini L. Pelicci Ö. Penek L. Pietrofaccia N. Pilipenko A. Pocar G. Raikov M. T. Ranalli G. Ranucci A. Razeto A. Re M. Redchuk N. Rossi S. Schönert D. Semenov G. Settanta M. Skorokhvatov A. Singhal O. Smirnov A. Sotnikov R. Tartaglia G. Testera E. Unzhakov A. Vishneva R. B. Vogelaar F. von Feilitzsch M. Wojcik M. Wurm S. Zavatarelli I. Zhutikov K. Zuber G. Zuzel Borexino Collaboration |
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search for low-energy signals from fast radio bursts with the borexino detector |
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Search for low-energy signals from fast radio bursts with the Borexino detector |
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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 $$\pm \, 1000$$ ± 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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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 $$\pm \, 1000$$ ± 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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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 $$\pm \, 1000$$ ± 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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| score |
7.399805 |