Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino
Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Appel, S. [verfasserIn] Bagdasarian, Z. [verfasserIn] Basilico, D. [verfasserIn] Bellini, G. [verfasserIn] Benziger, J. [verfasserIn] Biondi, R. [verfasserIn] Caccianiga, B. [verfasserIn] Calaprice, F. [verfasserIn] Caminata, A. [verfasserIn] Chepurnov, A. [verfasserIn] D’Angelo, D. [verfasserIn] Derbin, A. [verfasserIn] Di Giacinto, A. [verfasserIn] Di Marcello, V. [verfasserIn] Ding, X.F. [verfasserIn] Di Ludovico, A. [verfasserIn] Di Noto, L. [verfasserIn] Drachnev, I. [verfasserIn] Franco, D. [verfasserIn] Galbiati, C. [verfasserIn] Ghiano, C. [verfasserIn] Giammarchi, M. [verfasserIn] Goretti, A. [verfasserIn] Göttel, A.S. [verfasserIn] Gromov, M. [verfasserIn] Guffanti, D. [verfasserIn] Ianni, Aldo [verfasserIn] Ianni, Andrea [verfasserIn] Jany, A. [verfasserIn] Kobychev, V. [verfasserIn] Korga, G. [verfasserIn] Kumaran, S. [verfasserIn] Laubenstein, M. [verfasserIn] Litvinovich, E. [verfasserIn] Lombardi, P. [verfasserIn] Lomskaya, I. [verfasserIn] Ludhova, L. [verfasserIn] Lukyanchenko, G. [verfasserIn] Machulin, I. [verfasserIn] Martyn, J. [verfasserIn] Meroni, E. [verfasserIn] Miramonti, L. [verfasserIn] Misiaszek, M. [verfasserIn] Muratova, V. [verfasserIn] Nugmanov, R. [verfasserIn] Oberauer, L. [verfasserIn] Orekhov, V. [verfasserIn] Ortica, F. [verfasserIn] Pallavicini, M. [verfasserIn] Pelicci, L. [verfasserIn] Penek, Ö. [verfasserIn] Pietrofaccia, L. [verfasserIn] Pilipenko, N. [verfasserIn] Pocar, A. [verfasserIn] Raikov, G. [verfasserIn] Ranalli, M.T. [verfasserIn] Ranucci, G. [verfasserIn] Razeto, A. [verfasserIn] Re, A. [verfasserIn] Redchuk, M. [verfasserIn] Rossi, N. [verfasserIn] Schönert, S. [verfasserIn] Semenov, D. [verfasserIn] Settanta, G. [verfasserIn] Skorokhvatov, M. [verfasserIn] Singhal, A. [verfasserIn] Smirnov, O. [verfasserIn] Sotnikov, A. [verfasserIn] Tartaglia, R. [verfasserIn] Testera, G. [verfasserIn] Unzhakov, E. [verfasserIn] Vishneva, A. [verfasserIn] Vogelaar, R.B. [verfasserIn] von Feilitzsch, F. [verfasserIn] Wojcik, M. [verfasserIn] Wurm, M. [verfasserIn] Zavatarelli, S. [verfasserIn] Zuber, K. [verfasserIn] Zuzel, G. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Astroparticle physics - Amsterdam [u.a.] : Elsevier Science, 1992, 145 |
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| Übergeordnetes Werk: |
volume:145 |
| DOI / URN: |
10.1016/j.astropartphys.2022.102778 |
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| Katalog-ID: |
ELV008903824 |
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| 100 | 1 | |a Appel, S. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino |
| 264 | 1 | |c 2022 | |
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| 520 | |a Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. | ||
| 650 | 4 | |a Solar neutrinos | |
| 650 | 4 | |a Solar standard model | |
| 650 | 4 | |a Annual modulation | |
| 650 | 4 | |a Earth’s orbit parameters | |
| 650 | 4 | |a Neutrino day–night effect | |
| 700 | 1 | |a Bagdasarian, Z. |e verfasserin |4 aut | |
| 700 | 1 | |a Basilico, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Bellini, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Benziger, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Biondi, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Caccianiga, B. |e verfasserin |4 aut | |
| 700 | 1 | |a Calaprice, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Caminata, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Chepurnov, A. |e verfasserin |4 aut | |
| 700 | 1 | |a D’Angelo, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Derbin, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Di Giacinto, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Di Marcello, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Ding, X.F. |e verfasserin |4 aut | |
| 700 | 1 | |a Di Ludovico, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Di Noto, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Drachnev, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Franco, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Galbiati, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Ghiano, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Giammarchi, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Goretti, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Göttel, A.S. |e verfasserin |4 aut | |
| 700 | 1 | |a Gromov, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Guffanti, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Ianni, Aldo |e verfasserin |4 aut | |
| 700 | 1 | |a Ianni, Andrea |e verfasserin |4 aut | |
| 700 | 1 | |a Jany, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Kobychev, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Korga, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Kumaran, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Laubenstein, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Litvinovich, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Lombardi, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Lomskaya, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Ludhova, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Lukyanchenko, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Machulin, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Martyn, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Meroni, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Miramonti, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Misiaszek, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Muratova, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Nugmanov, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Oberauer, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Orekhov, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Ortica, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Pallavicini, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Pelicci, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Penek, Ö. |e verfasserin |4 aut | |
| 700 | 1 | |a Pietrofaccia, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Pilipenko, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Pocar, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Raikov, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Ranalli, M.T. |e verfasserin |4 aut | |
| 700 | 1 | |a Ranucci, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Razeto, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Re, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Redchuk, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Rossi, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Schönert, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Semenov, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Settanta, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Skorokhvatov, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Singhal, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Smirnov, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Sotnikov, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Tartaglia, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Testera, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Unzhakov, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Vishneva, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vogelaar, R.B. |e verfasserin |4 aut | |
| 700 | 1 | |a von Feilitzsch, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Wojcik, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Wurm, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Zavatarelli, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Zuber, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Zuzel, G. |e verfasserin |4 aut | |
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10.1016/j.astropartphys.2022.102778 doi (DE-627)ELV008903824 (ELSEVIER)S0927-6505(22)00079-2 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Appel, S. verfasserin aut Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. Solar neutrinos Solar standard model Annual modulation Earth’s orbit parameters Neutrino day–night effect Bagdasarian, Z. verfasserin aut Basilico, D. verfasserin aut Bellini, G. verfasserin aut Benziger, J. verfasserin aut Biondi, R. verfasserin aut Caccianiga, B. verfasserin aut Calaprice, F. verfasserin aut Caminata, A. verfasserin aut Chepurnov, A. verfasserin aut D’Angelo, D. verfasserin aut Derbin, A. verfasserin aut Di Giacinto, A. verfasserin aut Di Marcello, V. verfasserin aut Ding, X.F. verfasserin aut Di Ludovico, A. verfasserin aut Di Noto, L. verfasserin aut Drachnev, I. verfasserin aut Franco, D. verfasserin aut Galbiati, C. verfasserin aut Ghiano, C. verfasserin aut Giammarchi, M. verfasserin aut Goretti, A. verfasserin aut Göttel, A.S. verfasserin aut Gromov, M. verfasserin aut Guffanti, D. verfasserin aut Ianni, Aldo verfasserin aut Ianni, Andrea verfasserin aut Jany, A. verfasserin aut Kobychev, V. verfasserin aut Korga, G. verfasserin aut Kumaran, S. verfasserin aut Laubenstein, M. verfasserin aut Litvinovich, E. verfasserin aut Lombardi, P. verfasserin aut Lomskaya, I. verfasserin aut Ludhova, L. verfasserin aut Lukyanchenko, G. verfasserin aut Machulin, I. verfasserin aut Martyn, J. verfasserin aut Meroni, E. verfasserin aut Miramonti, L. verfasserin aut Misiaszek, M. verfasserin aut Muratova, V. verfasserin aut Nugmanov, R. verfasserin aut Oberauer, L. verfasserin aut Orekhov, V. verfasserin aut Ortica, F. verfasserin aut Pallavicini, M. verfasserin aut Pelicci, L. verfasserin aut Penek, Ö. verfasserin aut Pietrofaccia, L. verfasserin aut Pilipenko, N. verfasserin aut Pocar, A. verfasserin aut Raikov, G. verfasserin aut Ranalli, M.T. verfasserin aut Ranucci, G. verfasserin aut Razeto, A. verfasserin aut Re, A. verfasserin aut Redchuk, M. verfasserin aut Rossi, N. verfasserin aut Schönert, S. verfasserin aut Semenov, D. verfasserin aut Settanta, G. verfasserin aut Skorokhvatov, M. verfasserin aut Singhal, A. verfasserin aut Smirnov, O. verfasserin aut Sotnikov, A. verfasserin aut Tartaglia, R. verfasserin aut Testera, G. verfasserin aut Unzhakov, E. verfasserin aut Vishneva, A. verfasserin aut Vogelaar, R.B. verfasserin aut von Feilitzsch, F. verfasserin aut Wojcik, M. verfasserin aut Wurm, M. verfasserin aut Zavatarelli, S. verfasserin aut Zuber, K. verfasserin aut Zuzel, G. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 145 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:145 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.22 Astrophysik AR 145 |
| spelling |
10.1016/j.astropartphys.2022.102778 doi (DE-627)ELV008903824 (ELSEVIER)S0927-6505(22)00079-2 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Appel, S. verfasserin aut Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. Solar neutrinos Solar standard model Annual modulation Earth’s orbit parameters Neutrino day–night effect Bagdasarian, Z. verfasserin aut Basilico, D. verfasserin aut Bellini, G. verfasserin aut Benziger, J. verfasserin aut Biondi, R. verfasserin aut Caccianiga, B. verfasserin aut Calaprice, F. verfasserin aut Caminata, A. verfasserin aut Chepurnov, A. verfasserin aut D’Angelo, D. verfasserin aut Derbin, A. verfasserin aut Di Giacinto, A. verfasserin aut Di Marcello, V. verfasserin aut Ding, X.F. verfasserin aut Di Ludovico, A. verfasserin aut Di Noto, L. verfasserin aut Drachnev, I. verfasserin aut Franco, D. verfasserin aut Galbiati, C. verfasserin aut Ghiano, C. verfasserin aut Giammarchi, M. verfasserin aut Goretti, A. verfasserin aut Göttel, A.S. verfasserin aut Gromov, M. verfasserin aut Guffanti, D. verfasserin aut Ianni, Aldo verfasserin aut Ianni, Andrea verfasserin aut Jany, A. verfasserin aut Kobychev, V. verfasserin aut Korga, G. verfasserin aut Kumaran, S. verfasserin aut Laubenstein, M. verfasserin aut Litvinovich, E. verfasserin aut Lombardi, P. verfasserin aut Lomskaya, I. verfasserin aut Ludhova, L. verfasserin aut Lukyanchenko, G. verfasserin aut Machulin, I. verfasserin aut Martyn, J. verfasserin aut Meroni, E. verfasserin aut Miramonti, L. verfasserin aut Misiaszek, M. verfasserin aut Muratova, V. verfasserin aut Nugmanov, R. verfasserin aut Oberauer, L. verfasserin aut Orekhov, V. verfasserin aut Ortica, F. verfasserin aut Pallavicini, M. verfasserin aut Pelicci, L. verfasserin aut Penek, Ö. verfasserin aut Pietrofaccia, L. verfasserin aut Pilipenko, N. verfasserin aut Pocar, A. verfasserin aut Raikov, G. verfasserin aut Ranalli, M.T. verfasserin aut Ranucci, G. verfasserin aut Razeto, A. verfasserin aut Re, A. verfasserin aut Redchuk, M. verfasserin aut Rossi, N. verfasserin aut Schönert, S. verfasserin aut Semenov, D. verfasserin aut Settanta, G. verfasserin aut Skorokhvatov, M. verfasserin aut Singhal, A. verfasserin aut Smirnov, O. verfasserin aut Sotnikov, A. verfasserin aut Tartaglia, R. verfasserin aut Testera, G. verfasserin aut Unzhakov, E. verfasserin aut Vishneva, A. verfasserin aut Vogelaar, R.B. verfasserin aut von Feilitzsch, F. verfasserin aut Wojcik, M. verfasserin aut Wurm, M. verfasserin aut Zavatarelli, S. verfasserin aut Zuber, K. verfasserin aut Zuzel, G. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 145 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:145 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.22 Astrophysik AR 145 |
| allfields_unstemmed |
10.1016/j.astropartphys.2022.102778 doi (DE-627)ELV008903824 (ELSEVIER)S0927-6505(22)00079-2 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Appel, S. verfasserin aut Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. Solar neutrinos Solar standard model Annual modulation Earth’s orbit parameters Neutrino day–night effect Bagdasarian, Z. verfasserin aut Basilico, D. verfasserin aut Bellini, G. verfasserin aut Benziger, J. verfasserin aut Biondi, R. verfasserin aut Caccianiga, B. verfasserin aut Calaprice, F. verfasserin aut Caminata, A. verfasserin aut Chepurnov, A. verfasserin aut D’Angelo, D. verfasserin aut Derbin, A. verfasserin aut Di Giacinto, A. verfasserin aut Di Marcello, V. verfasserin aut Ding, X.F. verfasserin aut Di Ludovico, A. verfasserin aut Di Noto, L. verfasserin aut Drachnev, I. verfasserin aut Franco, D. verfasserin aut Galbiati, C. verfasserin aut Ghiano, C. verfasserin aut Giammarchi, M. verfasserin aut Goretti, A. verfasserin aut Göttel, A.S. verfasserin aut Gromov, M. verfasserin aut Guffanti, D. verfasserin aut Ianni, Aldo verfasserin aut Ianni, Andrea verfasserin aut Jany, A. verfasserin aut Kobychev, V. verfasserin aut Korga, G. verfasserin aut Kumaran, S. verfasserin aut Laubenstein, M. verfasserin aut Litvinovich, E. verfasserin aut Lombardi, P. verfasserin aut Lomskaya, I. verfasserin aut Ludhova, L. verfasserin aut Lukyanchenko, G. verfasserin aut Machulin, I. verfasserin aut Martyn, J. verfasserin aut Meroni, E. verfasserin aut Miramonti, L. verfasserin aut Misiaszek, M. verfasserin aut Muratova, V. verfasserin aut Nugmanov, R. verfasserin aut Oberauer, L. verfasserin aut Orekhov, V. verfasserin aut Ortica, F. verfasserin aut Pallavicini, M. verfasserin aut Pelicci, L. verfasserin aut Penek, Ö. verfasserin aut Pietrofaccia, L. verfasserin aut Pilipenko, N. verfasserin aut Pocar, A. verfasserin aut Raikov, G. verfasserin aut Ranalli, M.T. verfasserin aut Ranucci, G. verfasserin aut Razeto, A. verfasserin aut Re, A. verfasserin aut Redchuk, M. verfasserin aut Rossi, N. verfasserin aut Schönert, S. verfasserin aut Semenov, D. verfasserin aut Settanta, G. verfasserin aut Skorokhvatov, M. verfasserin aut Singhal, A. verfasserin aut Smirnov, O. verfasserin aut Sotnikov, A. verfasserin aut Tartaglia, R. verfasserin aut Testera, G. verfasserin aut Unzhakov, E. verfasserin aut Vishneva, A. verfasserin aut Vogelaar, R.B. verfasserin aut von Feilitzsch, F. verfasserin aut Wojcik, M. verfasserin aut Wurm, M. verfasserin aut Zavatarelli, S. verfasserin aut Zuber, K. verfasserin aut Zuzel, G. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 145 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:145 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.22 Astrophysik AR 145 |
| allfieldsGer |
10.1016/j.astropartphys.2022.102778 doi (DE-627)ELV008903824 (ELSEVIER)S0927-6505(22)00079-2 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Appel, S. verfasserin aut Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. Solar neutrinos Solar standard model Annual modulation Earth’s orbit parameters Neutrino day–night effect Bagdasarian, Z. verfasserin aut Basilico, D. verfasserin aut Bellini, G. verfasserin aut Benziger, J. verfasserin aut Biondi, R. verfasserin aut Caccianiga, B. verfasserin aut Calaprice, F. verfasserin aut Caminata, A. verfasserin aut Chepurnov, A. verfasserin aut D’Angelo, D. verfasserin aut Derbin, A. verfasserin aut Di Giacinto, A. verfasserin aut Di Marcello, V. verfasserin aut Ding, X.F. verfasserin aut Di Ludovico, A. verfasserin aut Di Noto, L. verfasserin aut Drachnev, I. verfasserin aut Franco, D. verfasserin aut Galbiati, C. verfasserin aut Ghiano, C. verfasserin aut Giammarchi, M. verfasserin aut Goretti, A. verfasserin aut Göttel, A.S. verfasserin aut Gromov, M. verfasserin aut Guffanti, D. verfasserin aut Ianni, Aldo verfasserin aut Ianni, Andrea verfasserin aut Jany, A. verfasserin aut Kobychev, V. verfasserin aut Korga, G. verfasserin aut Kumaran, S. verfasserin aut Laubenstein, M. verfasserin aut Litvinovich, E. verfasserin aut Lombardi, P. verfasserin aut Lomskaya, I. verfasserin aut Ludhova, L. verfasserin aut Lukyanchenko, G. verfasserin aut Machulin, I. verfasserin aut Martyn, J. verfasserin aut Meroni, E. verfasserin aut Miramonti, L. verfasserin aut Misiaszek, M. verfasserin aut Muratova, V. verfasserin aut Nugmanov, R. verfasserin aut Oberauer, L. verfasserin aut Orekhov, V. verfasserin aut Ortica, F. verfasserin aut Pallavicini, M. verfasserin aut Pelicci, L. verfasserin aut Penek, Ö. verfasserin aut Pietrofaccia, L. verfasserin aut Pilipenko, N. verfasserin aut Pocar, A. verfasserin aut Raikov, G. verfasserin aut Ranalli, M.T. verfasserin aut Ranucci, G. verfasserin aut Razeto, A. verfasserin aut Re, A. verfasserin aut Redchuk, M. verfasserin aut Rossi, N. verfasserin aut Schönert, S. verfasserin aut Semenov, D. verfasserin aut Settanta, G. verfasserin aut Skorokhvatov, M. verfasserin aut Singhal, A. verfasserin aut Smirnov, O. verfasserin aut Sotnikov, A. verfasserin aut Tartaglia, R. verfasserin aut Testera, G. verfasserin aut Unzhakov, E. verfasserin aut Vishneva, A. verfasserin aut Vogelaar, R.B. verfasserin aut von Feilitzsch, F. verfasserin aut Wojcik, M. verfasserin aut Wurm, M. verfasserin aut Zavatarelli, S. verfasserin aut Zuber, K. verfasserin aut Zuzel, G. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 145 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:145 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.22 Astrophysik AR 145 |
| allfieldsSound |
10.1016/j.astropartphys.2022.102778 doi (DE-627)ELV008903824 (ELSEVIER)S0927-6505(22)00079-2 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Appel, S. verfasserin aut Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. Solar neutrinos Solar standard model Annual modulation Earth’s orbit parameters Neutrino day–night effect Bagdasarian, Z. verfasserin aut Basilico, D. verfasserin aut Bellini, G. verfasserin aut Benziger, J. verfasserin aut Biondi, R. verfasserin aut Caccianiga, B. verfasserin aut Calaprice, F. verfasserin aut Caminata, A. verfasserin aut Chepurnov, A. verfasserin aut D’Angelo, D. verfasserin aut Derbin, A. verfasserin aut Di Giacinto, A. verfasserin aut Di Marcello, V. verfasserin aut Ding, X.F. verfasserin aut Di Ludovico, A. verfasserin aut Di Noto, L. verfasserin aut Drachnev, I. verfasserin aut Franco, D. verfasserin aut Galbiati, C. verfasserin aut Ghiano, C. verfasserin aut Giammarchi, M. verfasserin aut Goretti, A. verfasserin aut Göttel, A.S. verfasserin aut Gromov, M. verfasserin aut Guffanti, D. verfasserin aut Ianni, Aldo verfasserin aut Ianni, Andrea verfasserin aut Jany, A. verfasserin aut Kobychev, V. verfasserin aut Korga, G. verfasserin aut Kumaran, S. verfasserin aut Laubenstein, M. verfasserin aut Litvinovich, E. verfasserin aut Lombardi, P. verfasserin aut Lomskaya, I. verfasserin aut Ludhova, L. verfasserin aut Lukyanchenko, G. verfasserin aut Machulin, I. verfasserin aut Martyn, J. verfasserin aut Meroni, E. verfasserin aut Miramonti, L. verfasserin aut Misiaszek, M. verfasserin aut Muratova, V. verfasserin aut Nugmanov, R. verfasserin aut Oberauer, L. verfasserin aut Orekhov, V. verfasserin aut Ortica, F. verfasserin aut Pallavicini, M. verfasserin aut Pelicci, L. verfasserin aut Penek, Ö. verfasserin aut Pietrofaccia, L. verfasserin aut Pilipenko, N. verfasserin aut Pocar, A. verfasserin aut Raikov, G. verfasserin aut Ranalli, M.T. verfasserin aut Ranucci, G. verfasserin aut Razeto, A. verfasserin aut Re, A. verfasserin aut Redchuk, M. verfasserin aut Rossi, N. verfasserin aut Schönert, S. verfasserin aut Semenov, D. verfasserin aut Settanta, G. verfasserin aut Skorokhvatov, M. verfasserin aut Singhal, A. verfasserin aut Smirnov, O. verfasserin aut Sotnikov, A. verfasserin aut Tartaglia, R. verfasserin aut Testera, G. verfasserin aut Unzhakov, E. verfasserin aut Vishneva, A. verfasserin aut Vogelaar, R.B. verfasserin aut von Feilitzsch, F. verfasserin aut Wojcik, M. verfasserin aut Wurm, M. verfasserin aut Zavatarelli, S. verfasserin aut Zuber, K. verfasserin aut Zuzel, G. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 145 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:145 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.22 Astrophysik AR 145 |
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Appel, S. @@aut@@ Bagdasarian, Z. @@aut@@ Basilico, D. @@aut@@ Bellini, G. @@aut@@ Benziger, J. @@aut@@ Biondi, R. @@aut@@ Caccianiga, B. @@aut@@ Calaprice, F. @@aut@@ Caminata, A. @@aut@@ Chepurnov, A. @@aut@@ D’Angelo, D. @@aut@@ Derbin, A. @@aut@@ Di Giacinto, A. @@aut@@ Di Marcello, V. @@aut@@ Ding, X.F. @@aut@@ Di Ludovico, A. @@aut@@ Di Noto, L. @@aut@@ Drachnev, I. @@aut@@ Franco, D. @@aut@@ Galbiati, C. @@aut@@ Ghiano, C. @@aut@@ Giammarchi, M. @@aut@@ Goretti, A. @@aut@@ Göttel, A.S. @@aut@@ Gromov, M. @@aut@@ Guffanti, D. @@aut@@ Ianni, Aldo @@aut@@ Ianni, Andrea @@aut@@ Jany, A. @@aut@@ Kobychev, V. @@aut@@ Korga, G. @@aut@@ Kumaran, S. @@aut@@ Laubenstein, M. @@aut@@ Litvinovich, E. @@aut@@ Lombardi, P. @@aut@@ Lomskaya, I. @@aut@@ Ludhova, L. @@aut@@ Lukyanchenko, G. @@aut@@ Machulin, I. @@aut@@ Martyn, J. @@aut@@ Meroni, E. @@aut@@ Miramonti, L. @@aut@@ Misiaszek, M. @@aut@@ Muratova, V. @@aut@@ Nugmanov, R. @@aut@@ Oberauer, L. @@aut@@ Orekhov, V. @@aut@@ Ortica, F. @@aut@@ Pallavicini, M. @@aut@@ Pelicci, L. @@aut@@ Penek, Ö. @@aut@@ Pietrofaccia, L. @@aut@@ Pilipenko, N. @@aut@@ Pocar, A. @@aut@@ Raikov, G. @@aut@@ Ranalli, M.T. @@aut@@ Ranucci, G. @@aut@@ Razeto, A. @@aut@@ Re, A. @@aut@@ Redchuk, M. @@aut@@ Rossi, N. @@aut@@ Schönert, S. @@aut@@ Semenov, D. @@aut@@ Settanta, G. @@aut@@ Skorokhvatov, M. @@aut@@ Singhal, A. @@aut@@ Smirnov, O. @@aut@@ Sotnikov, A. @@aut@@ Tartaglia, R. @@aut@@ Testera, G. @@aut@@ Unzhakov, E. @@aut@@ Vishneva, A. @@aut@@ Vogelaar, R.B. @@aut@@ von Feilitzsch, F. @@aut@@ Wojcik, M. @@aut@@ Wurm, M. @@aut@@ Zavatarelli, S. @@aut@@ Zuber, K. @@aut@@ Zuzel, G. @@aut@@ |
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Appel, S. |
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540 DE-600 39.22 bkl Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino Solar neutrinos Solar standard model Annual modulation Earth’s orbit parameters Neutrino day–night effect |
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Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino |
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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. Di Giacinto, A. Di Marcello, V. Ding, X.F. Di Ludovico, A. Di Noto, L. Drachnev, I. Franco, D. Galbiati, C. Ghiano, C. Giammarchi, M. Goretti, A. Göttel, A.S. Gromov, M. Guffanti, D. Ianni, Aldo Ianni, Andrea Jany, A. Kobychev, V. Korga, G. Kumaran, S. Laubenstein, M. Litvinovich, E. Lombardi, P. Lomskaya, I. Ludhova, L. 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. Penek, Ö. Pietrofaccia, L. Pilipenko, N. Pocar, A. Raikov, G. Ranalli, M.T. Ranucci, G. Razeto, A. Re, A. Redchuk, M. Rossi, N. Schönert, S. Semenov, D. Settanta, G. Skorokhvatov, M. Singhal, A. Smirnov, O. Sotnikov, A. Tartaglia, R. Testera, G. Unzhakov, E. Vishneva, A. Vogelaar, R.B. von Feilitzsch, F. Wojcik, M. Wurm, M. Zavatarelli, S. Zuber, K. Zuzel, G. |
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Appel, S. |
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| title_sort |
independent determination of the earth’s orbital parameters with solar neutrinos in borexino |
| title_auth |
Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino |
| abstract |
Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. |
| abstractGer |
Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. |
| abstract_unstemmed |
Since the beginning of 2012, the Borexino collaboration has been reporting precision measurements of the solar neutrino fluxes, emitted in the proton–proton chain and in the Carbon–Nitrogen–Oxygen cycle. The experimental sensitivity achieved in Phase-II and Phase-III of the Borexino data taking made it possible to detect the annual modulation of the solar neutrino interaction rate due to the eccentricity of Earth’s orbit, with a statistical significance greater than 5 σ . This is the first precise measurement of the Earth’s orbital parameters based solely on solar neutrinos and an additional signature of the solar origin of the Borexino signal. The complete periodogram of the time series of the Borexino solar neutrino detection rate is also reported, exploring frequencies between one cycle/year and one cycle/day. No other significant modulation frequencies are found. The present results were uniquely made possible by Borexino’s decade-long high-precision solar neutrino detection. |
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| title_short |
Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino |
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Bagdasarian, Z. Basilico, D. Bellini, G. Benziger, J. Biondi, R. Caccianiga, B. Calaprice, F. Caminata, A. Chepurnov, A. D’Angelo, D. Derbin, A. Di Giacinto, A. Di Marcello, V. Ding, X.F. Di Ludovico, A. Di Noto, L. Drachnev, I. Franco, D. Galbiati, C. Ghiano, C. Giammarchi, M. Goretti, A. Göttel, A.S. Gromov, M. Guffanti, D. Ianni, Aldo Ianni, Andrea Jany, A. Kobychev, V. Korga, G. Kumaran, S. Laubenstein, M. Litvinovich, E. Lombardi, P. Lomskaya, I. Ludhova, L. 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. Penek, Ö. Pietrofaccia, L. Pilipenko, N. Pocar, A. Raikov, G. Ranalli, M.T. Ranucci, G. Razeto, A. Re, A. Redchuk, M. Rossi, N. Schönert, S. Semenov, D. Settanta, G. Skorokhvatov, M. Singhal, A. Smirnov, O. Sotnikov, A. Tartaglia, R. Testera, G. Unzhakov, E. Vishneva, A. Vogelaar, R.B. von Feilitzsch, F. Wojcik, M. Wurm, M. Zavatarelli, S. Zuber, K. Zuzel, G. |
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Bagdasarian, Z. Basilico, D. Bellini, G. Benziger, J. Biondi, R. Caccianiga, B. Calaprice, F. Caminata, A. Chepurnov, A. D’Angelo, D. Derbin, A. Di Giacinto, A. Di Marcello, V. Ding, X.F. Di Ludovico, A. Di Noto, L. Drachnev, I. Franco, D. Galbiati, C. Ghiano, C. Giammarchi, M. Goretti, A. Göttel, A.S. Gromov, M. Guffanti, D. Ianni, Aldo Ianni, Andrea Jany, A. Kobychev, V. Korga, G. Kumaran, S. Laubenstein, M. Litvinovich, E. Lombardi, P. Lomskaya, I. Ludhova, L. 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. Penek, Ö. Pietrofaccia, L. Pilipenko, N. Pocar, A. Raikov, G. Ranalli, M.T. Ranucci, G. Razeto, A. Re, A. Redchuk, M. Rossi, N. Schönert, S. Semenov, D. Settanta, G. Skorokhvatov, M. Singhal, A. Smirnov, O. Sotnikov, A. Tartaglia, R. Testera, G. Unzhakov, E. Vishneva, A. Vogelaar, R.B. von Feilitzsch, F. Wojcik, M. Wurm, M. Zavatarelli, S. Zuber, K. Zuzel, G. |
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7.400549 |