Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II
Abstract The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-ν e survival probability P ee (E), and the chiral couplings of the neutrino and electron. Some theories of physics beyond the Standard Model postulate...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2020-02-01
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| Series: | Journal of High Energy Physics |
| Subjects: | |
| Online Access: | https://doi.org/10.1007/JHEP02(2020)038 |
| _version_ | 1818453765044305920 |
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| author | The Borexino collaboration S. K. Agarwalla M. Agostini K. Altenmüller S. Appel V. Atroshchenko Z. Bagdasarian D. Basilico G. Bellini J. Benziger D. Bick G. Bonfini D. Bravo B. Caccianiga F. Calaprice A. Caminata L. Cappelli P. Cavalcante F. Cavanna A. Chepurnov K. Choi D. D’Angelo S. Davini A. Derbin A. Di Giacinto V. Di Marcello X. F. Ding A. Di Ludovico L. Di Noto I. Drachnev K. Fomenko A. Formozov D. Franco F. Gabriele C. Galbiati M. Gschwender C. Ghiano M. Giammarchi A. Goretti M. Gromov D. Guffanti C. Hagner E. Hungerford Aldo Ianni Andrea Ianni A. Jany D. Jeschke S. Kumaran V. Kobychev G. Korga T. Lachenmaier M. Laubenstein E. Litvinovich P. Lombardi L. Ludhova G. Lukyanchenko L. Lukyanchenko I. Machulin G. Manuzio S. Marcocci J. Maricic J. Martyn E. Meroni M. Meyer L. Miramonti M. Misiaszek V. Muratova B. Neumair M. Nieslony L. Oberauer V. Orekhov F. Ortica M. Pallavicini L. Papp Ö. Penek L. Pietrofaccia N. Pilipenko A. Pocar G. Raikov G. Ranucci A. Razeto A. Re M. Redchuk A. Romani N. Rossi S. Rottenanger S. Schönert D. Semenov M. Skorokhvatov O. Smirnov A. Sotnikov C. Sun Y. Suvorov T. Takeuchi R. Tartaglia G. Testera J. Thurn E. Unzhakov A. Vishneva R. B. Vogelaar F. von Feilitzsch M. Wojcik M. Wurm O. Zaimidoroga S. Zavatarelli K. Zuber G. Zuzel |
| author_facet | The Borexino collaboration S. K. Agarwalla M. Agostini K. Altenmüller S. Appel V. Atroshchenko Z. Bagdasarian D. Basilico G. Bellini J. Benziger D. Bick G. Bonfini D. Bravo B. Caccianiga F. Calaprice A. Caminata L. Cappelli P. Cavalcante F. Cavanna A. Chepurnov K. Choi D. D’Angelo S. Davini A. Derbin A. Di Giacinto V. Di Marcello X. F. Ding A. Di Ludovico L. Di Noto I. Drachnev K. Fomenko A. Formozov D. Franco F. Gabriele C. Galbiati M. Gschwender C. Ghiano M. Giammarchi A. Goretti M. Gromov D. Guffanti C. Hagner E. Hungerford Aldo Ianni Andrea Ianni A. Jany D. Jeschke S. Kumaran V. Kobychev G. Korga T. Lachenmaier M. Laubenstein E. Litvinovich P. Lombardi L. Ludhova G. Lukyanchenko L. Lukyanchenko I. Machulin G. Manuzio S. Marcocci J. Maricic J. Martyn E. Meroni M. Meyer L. Miramonti M. Misiaszek V. Muratova B. Neumair M. Nieslony L. Oberauer V. Orekhov F. Ortica M. Pallavicini L. Papp Ö. Penek L. Pietrofaccia N. Pilipenko A. Pocar G. Raikov G. Ranucci A. Razeto A. Re M. Redchuk A. Romani N. Rossi S. Rottenanger S. Schönert D. Semenov M. Skorokhvatov O. Smirnov A. Sotnikov C. Sun Y. Suvorov T. Takeuchi R. Tartaglia G. Testera J. Thurn E. Unzhakov A. Vishneva R. B. Vogelaar F. von Feilitzsch M. Wojcik M. Wurm O. Zaimidoroga S. Zavatarelli K. Zuber G. Zuzel |
| author_sort | The Borexino collaboration |
| collection | DOAJ |
| description | Abstract The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-ν e survival probability P ee (E), and the chiral couplings of the neutrino and electron. Some theories of physics beyond the Standard Model postulate the existence of Non-Standard Interactions (NSI’s) which modify the chiral couplings and P ee (E). In this paper, we search for such NSI’s, in particular, flavor-diagonal neutral current interactions that modify the ν e e and ν τ e couplings using Borexino Phase II data. Standard Solar Model predictions of the solar neutrino fluxes for both high- and low-metallicity assumptions are considered. No indication of new physics is found at the level of sensitivity of the detector and constraints on the parameters of the NSI’s are placed. In addition, with the same dataset the value of sin2 θ W is obtained with a precision comparable to that achieved in reactor antineutrino experiments . |
| first_indexed | 2024-12-14T21:44:11Z |
| format | Article |
| id | doaj.art-2e5e2fc0459e42b195d5d5a23dedaa48 |
| institution | Directory Open Access Journal |
| issn | 1029-8479 |
| language | English |
| last_indexed | 2024-12-14T21:44:11Z |
| publishDate | 2020-02-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | Journal of High Energy Physics |
| spelling | doaj.art-2e5e2fc0459e42b195d5d5a23dedaa482022-12-21T22:46:23ZengSpringerOpenJournal of High Energy Physics1029-84792020-02-012020212910.1007/JHEP02(2020)038Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-IIThe Borexino collaborationS. K. Agarwalla0M. Agostini1K. Altenmüller2S. Appel3V. Atroshchenko4Z. Bagdasarian5D. Basilico6G. Bellini7J. Benziger8D. Bick9G. Bonfini10D. Bravo11B. Caccianiga12F. Calaprice13A. Caminata14L. Cappelli15P. Cavalcante16F. Cavanna17A. Chepurnov18K. Choi19D. D’Angelo20S. Davini21A. Derbin22A. Di Giacinto23V. Di Marcello24X. F. Ding25A. Di Ludovico26L. Di Noto27I. Drachnev28K. Fomenko29A. Formozov30D. Franco31F. Gabriele32C. Galbiati33M. Gschwender34C. Ghiano35M. Giammarchi36A. Goretti37M. Gromov38D. Guffanti39C. Hagner40E. Hungerford41Aldo Ianni42Andrea Ianni43A. Jany44D. Jeschke45S. Kumaran46V. Kobychev47G. Korga48T. Lachenmaier49M. Laubenstein50E. Litvinovich51P. Lombardi52L. Ludhova53G. Lukyanchenko54L. Lukyanchenko55I. Machulin56G. Manuzio57S. Marcocci58J. Maricic59J. Martyn60E. Meroni61M. Meyer62L. Miramonti63M. Misiaszek64V. Muratova65B. Neumair66M. Nieslony67L. Oberauer68V. Orekhov69F. Ortica70M. Pallavicini71L. Papp72Ö. Penek73L. Pietrofaccia74N. Pilipenko75A. Pocar76G. Raikov77G. Ranucci78A. Razeto79A. Re80M. Redchuk81A. Romani82N. Rossi83S. Rottenanger84S. Schönert85D. Semenov86M. Skorokhvatov87O. Smirnov88A. Sotnikov89C. Sun90Y. Suvorov91T. Takeuchi92R. Tartaglia93G. Testera94J. Thurn95E. Unzhakov96A. Vishneva97R. B. Vogelaar98F. von Feilitzsch99M. Wojcik100M. Wurm101O. Zaimidoroga102S. Zavatarelli103K. Zuber104G. Zuzel105Institute of Physics, Sachivalaya Marg, Sainik School PostPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenNational Research Centre Kurchatov InstituteInstitut für Kernphysik, Forschungszentrum JülichDipartimento di Fisica, Università degli Studi e INFNDipartimento di Fisica, Università degli Studi e INFNChemical Engineering Department, Princeton UniversityInstitut für Experimentalphysik, Universität HamburgINFN Laboratori Nazionali del Gran SassoDipartimento di Fisica, Università degli Studi e INFNDipartimento di Fisica, Università degli Studi e INFNPhysics Department, Princeton UniversityDipartimento di Fisica, Università degli Studi e INFNINFN Laboratori Nazionali del Gran SassoINFN Laboratori Nazionali del Gran SassoDipartimento di Fisica, Università degli Studi e INFNLomonosov Moscow State University Skobeltsyn Institute of Nuclear PhysicsDepartment of Physics and Astronomy, University of HawaiiDipartimento di Fisica, Università degli Studi e INFNDipartimento di Fisica, Università degli Studi e INFNSt. Petersburg Nuclear Physics Institute NRC Kurchatov InstituteINFN Laboratori Nazionali del Gran SassoINFN Laboratori Nazionali del Gran SassoINFN Laboratori Nazionali del Gran SassoPhysics Department, Princeton UniversityDipartimento di Fisica, Università degli Studi e INFNSt. Petersburg Nuclear Physics Institute NRC Kurchatov InstituteJoint Institute for Nuclear ResearchDipartimento di Fisica, Università degli Studi e INFNAstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Sorbonne Paris CitéINFN Laboratori Nazionali del Gran SassoPhysics Department, Princeton UniversityKepler Center for Astro and Particle Physics, Universität TübingenINFN Laboratori Nazionali del Gran SassoDipartimento di Fisica, Università degli Studi e INFNPhysics Department, Princeton UniversityLomonosov Moscow State University Skobeltsyn Institute of Nuclear PhysicsInstitute of Physics and Excellence Cluster PRISMA+, Johannes Gutenberg-Universität MainzInstitut für Experimentalphysik, Universität HamburgDepartment of Physics, University of HoustonINFN Laboratori Nazionali del Gran SassoPhysics Department, Princeton UniversityM. Smoluchowski Institute of Physics, Jagiellonian UniversityPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenInstitut für Kernphysik, Forschungszentrum JülichInstitute for Nuclear Research of NAS UkraineDepartment of Physics, University of HoustonKepler Center for Astro and Particle Physics, Universität TübingenINFN Laboratori Nazionali del Gran SassoNational Research Centre Kurchatov InstituteDipartimento di Fisica, Università degli Studi e INFNInstitut für Kernphysik, Forschungszentrum JülichNational Research Centre Kurchatov InstituteNational Research Centre Kurchatov InstituteNational Research Centre Kurchatov InstituteDipartimento di Fisica, Università degli Studi e INFNGran Sasso Science InstituteDepartment of Physics and Astronomy, University of HawaiiInstitute of Physics and Excellence Cluster PRISMA+, Johannes Gutenberg-Universität MainzDipartimento di Fisica, Università degli Studi e INFNDepartment of Physics, Technische Universität DresdenDipartimento di Fisica, Università degli Studi e INFNM. Smoluchowski Institute of Physics, Jagiellonian UniversitySt. Petersburg Nuclear Physics Institute NRC Kurchatov InstitutePhysik-Department and Excellence Cluster Universe, Technische Universität MünchenInstitute of Physics and Excellence Cluster PRISMA+, Johannes Gutenberg-Universität MainzPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenNational Research Centre Kurchatov InstituteDipartimento di Chimica, Biologia e Biotecnologie, Università degli Studi e INFNDipartimento di Fisica, Università degli Studi e INFNPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenInstitut für Kernphysik, Forschungszentrum JülichPhysics Department, Princeton UniversitySt. Petersburg Nuclear Physics Institute NRC Kurchatov InstituteAmherst Center for Fundamental Interactions and Physics Department, University of MassachusettsNational Research Centre Kurchatov InstituteDipartimento di Fisica, Università degli Studi e INFNINFN Laboratori Nazionali del Gran SassoDipartimento di Fisica, Università degli Studi e INFNInstitut für Kernphysik, Forschungszentrum JülichDipartimento di Chimica, Biologia e Biotecnologie, Università degli Studi e INFNINFN Laboratori Nazionali del Gran SassoKepler Center for Astro and Particle Physics, Universität TübingenPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenSt. Petersburg Nuclear Physics Institute NRC Kurchatov InstituteNational Research Centre Kurchatov InstituteJoint Institute for Nuclear ResearchJoint Institute for Nuclear ResearchCAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of SciencesNational Research Centre Kurchatov InstitutePhysics Department, Virginia Polytechnic Institute and State UniversityINFN Laboratori Nazionali del Gran SassoDipartimento di Fisica, Università degli Studi e INFNDepartment of Physics, Technische Universität DresdenSt. Petersburg Nuclear Physics Institute NRC Kurchatov InstituteJoint Institute for Nuclear ResearchPhysics Department, Virginia Polytechnic Institute and State UniversityPhysik-Department and Excellence Cluster Universe, Technische Universität MünchenM. Smoluchowski Institute of Physics, Jagiellonian UniversityInstitute of Physics and Excellence Cluster PRISMA+, Johannes Gutenberg-Universität MainzJoint Institute for Nuclear ResearchDipartimento di Fisica, Università degli Studi e INFNDepartment of Physics, Technische Universität DresdenM. Smoluchowski Institute of Physics, Jagiellonian UniversityAbstract The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-ν e survival probability P ee (E), and the chiral couplings of the neutrino and electron. Some theories of physics beyond the Standard Model postulate the existence of Non-Standard Interactions (NSI’s) which modify the chiral couplings and P ee (E). In this paper, we search for such NSI’s, in particular, flavor-diagonal neutral current interactions that modify the ν e e and ν τ e couplings using Borexino Phase II data. Standard Solar Model predictions of the solar neutrino fluxes for both high- and low-metallicity assumptions are considered. No indication of new physics is found at the level of sensitivity of the detector and constraints on the parameters of the NSI’s are placed. In addition, with the same dataset the value of sin2 θ W is obtained with a precision comparable to that achieved in reactor antineutrino experiments .https://doi.org/10.1007/JHEP02(2020)038Neutrino PhysicsBeyond Standard Model |
| spellingShingle | The Borexino collaboration S. K. Agarwalla M. Agostini K. Altenmüller S. Appel V. Atroshchenko Z. Bagdasarian D. Basilico G. Bellini J. Benziger D. Bick G. Bonfini D. Bravo B. Caccianiga F. Calaprice A. Caminata L. Cappelli P. Cavalcante F. Cavanna A. Chepurnov K. Choi D. D’Angelo S. Davini A. Derbin A. Di Giacinto V. Di Marcello X. F. Ding A. Di Ludovico L. Di Noto I. Drachnev K. Fomenko A. Formozov D. Franco F. Gabriele C. Galbiati M. Gschwender C. Ghiano M. Giammarchi A. Goretti M. Gromov D. Guffanti C. Hagner E. Hungerford Aldo Ianni Andrea Ianni A. Jany D. Jeschke S. Kumaran V. Kobychev G. Korga T. Lachenmaier M. Laubenstein E. Litvinovich P. Lombardi L. Ludhova G. Lukyanchenko L. Lukyanchenko I. Machulin G. Manuzio S. Marcocci J. Maricic J. Martyn E. Meroni M. Meyer L. Miramonti M. Misiaszek V. Muratova B. Neumair M. Nieslony L. Oberauer V. Orekhov F. Ortica M. Pallavicini L. Papp Ö. Penek L. Pietrofaccia N. Pilipenko A. Pocar G. Raikov G. Ranucci A. Razeto A. Re M. Redchuk A. Romani N. Rossi S. Rottenanger S. Schönert D. Semenov M. Skorokhvatov O. Smirnov A. Sotnikov C. Sun Y. Suvorov T. Takeuchi R. Tartaglia G. Testera J. Thurn E. Unzhakov A. Vishneva R. B. Vogelaar F. von Feilitzsch M. Wojcik M. Wurm O. Zaimidoroga S. Zavatarelli K. Zuber G. Zuzel Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II Journal of High Energy Physics Neutrino Physics Beyond Standard Model |
| title | Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II |
| title_full | Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II |
| title_fullStr | Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II |
| title_full_unstemmed | Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II |
| title_short | Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II |
| title_sort | constraints on flavor diagonal non standard neutrino interactions from borexino phase ii |
| topic | Neutrino Physics Beyond Standard Model |
| url | https://doi.org/10.1007/JHEP02(2020)038 |
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