Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments
In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single...
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| Autor*in: |
Aguilar, J.A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023transfer abstract |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells - 2012transfer abstract, Amsterdam [u.a.] |
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| Übergeordnetes Werk: |
volume:145 ; year:2023 ; pages:0 |
| Links: |
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| DOI / URN: |
10.1016/j.astropartphys.2022.102790 |
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| Katalog-ID: |
ELV059747692 |
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| 520 | |a In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. | ||
| 520 | |a In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. | ||
| 650 | 7 | |a Background rejection |2 Elsevier | |
| 650 | 7 | |a Ultra-high energy cosmic rays |2 Elsevier | |
| 650 | 7 | |a Triboelectric effect |2 Elsevier | |
| 650 | 7 | |a Neutrino |2 Elsevier | |
| 700 | 1 | |a Anker, A. |4 oth | |
| 700 | 1 | |a Allison, P. |4 oth | |
| 700 | 1 | |a Archambault, S. |4 oth | |
| 700 | 1 | |a Baldi, P. |4 oth | |
| 700 | 1 | |a Barwick, S.W. |4 oth | |
| 700 | 1 | |a Beatty, J.J. |4 oth | |
| 700 | 1 | |a Beise, J. |4 oth | |
| 700 | 1 | |a Besson, D. |4 oth | |
| 700 | 1 | |a Bishop, A. |4 oth | |
| 700 | 1 | |a Bondarev, E. |4 oth | |
| 700 | 1 | |a Botner, O. |4 oth | |
| 700 | 1 | |a Bouma, S. |4 oth | |
| 700 | 1 | |a Buitink, S. |4 oth | |
| 700 | 1 | |a Cataldo, M. |4 oth | |
| 700 | 1 | |a Chen, C.C. |4 oth | |
| 700 | 1 | |a Chen, C.H. |4 oth | |
| 700 | 1 | |a Chen, P. |4 oth | |
| 700 | 1 | |a Chen, Y.C. |4 oth | |
| 700 | 1 | |a Choi, T. |4 oth | |
| 700 | 1 | |a Clark, B.A. |4 oth | |
| 700 | 1 | |a Clay, W. |4 oth | |
| 700 | 1 | |a Curtis-Ginsberg, Z. |4 oth | |
| 700 | 1 | |a Connolly, A. |4 oth | |
| 700 | 1 | |a Cremonesi, L. |4 oth | |
| 700 | 1 | |a Dasgupta, P. |4 oth | |
| 700 | 1 | |a Davies, J. |4 oth | |
| 700 | 1 | |a de Kockere, S. |4 oth | |
| 700 | 1 | |a de Vries, K.D. |4 oth | |
| 700 | 1 | |a Deaconu, C. |4 oth | |
| 700 | 1 | |a DuVernois, M.A. |4 oth | |
| 700 | 1 | |a Flaherty, J. |4 oth | |
| 700 | 1 | |a Friedman, E. |4 oth | |
| 700 | 1 | |a Gaior, R. |4 oth | |
| 700 | 1 | |a Gaswint, G. |4 oth | |
| 700 | 1 | |a Glaser, C. |4 oth | |
| 700 | 1 | |a Hallgren, A. |4 oth | |
| 700 | 1 | |a Hallmann, S. |4 oth | |
| 700 | 1 | |a Ham, Y.-B. |4 oth | |
| 700 | 1 | |a Hanson, J.C. |4 oth | |
| 700 | 1 | |a Harty, N. |4 oth | |
| 700 | 1 | |a Hendricks, B. |4 oth | |
| 700 | 1 | |a Hoffman, K.D. |4 oth | |
| 700 | 1 | |a Hong, E. |4 oth | |
| 700 | 1 | |a Hornhuber, C. |4 oth | |
| 700 | 1 | |a Hsu, S.Y. |4 oth | |
| 700 | 1 | |a Hu, L. |4 oth | |
| 700 | 1 | |a Huang, J.J. |4 oth | |
| 700 | 1 | |a Huang, M.-H. |4 oth | |
| 700 | 1 | |a Hughes, K. |4 oth | |
| 700 | 1 | |a Ishihara, A. |4 oth | |
| 700 | 1 | |a Jee, G. |4 oth | |
| 700 | 1 | |a Jung, J. |4 oth | |
| 700 | 1 | |a Karle, A. |4 oth | |
| 700 | 1 | |a Kelley, J.L. |4 oth | |
| 700 | 1 | |a Klein, S.R. |4 oth | |
| 700 | 1 | |a Kleinfelder, S.A. |4 oth | |
| 700 | 1 | |a Kim, J. |4 oth | |
| 700 | 1 | |a Kim, K.-C. |4 oth | |
| 700 | 1 | |a Kim, M.-C. |4 oth | |
| 700 | 1 | |a Kravchenko, I. |4 oth | |
| 700 | 1 | |a Krebs, R. |4 oth | |
| 700 | 1 | |a Ku, Y. |4 oth | |
| 700 | 1 | |a Kuo, C.Y. |4 oth | |
| 700 | 1 | |a Kurusu, K. |4 oth | |
| 700 | 1 | |a Kwon, Hyuck-Jin |4 oth | |
| 700 | 1 | |a Lahmann, R. |4 oth | |
| 700 | 1 | |a Landsman, H. |4 oth | |
| 700 | 1 | |a Latif, U. |4 oth | |
| 700 | 1 | |a Lee, C. |4 oth | |
| 700 | 1 | |a Leung, C.-H. |4 oth | |
| 700 | 1 | |a Li, C.-J. |4 oth | |
| 700 | 1 | |a Liu, J. |4 oth | |
| 700 | 1 | |a Liu, T.-C. |4 oth | |
| 700 | 1 | |a Lu, M.-Y. |4 oth | |
| 700 | 1 | |a Madison, K. |4 oth | |
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| 700 | 1 | |a McAleer, S. |4 oth | |
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| 700 | 1 | |a Meyers, Z.S. |4 oth | |
| 700 | 1 | |a Michaels, K. |4 oth | |
| 700 | 1 | |a Mikhailova, M. |4 oth | |
| 700 | 1 | |a Mulrey, K. |4 oth | |
| 700 | 1 | |a Nam, J. |4 oth | |
| 700 | 1 | |a Nichol, R.J. |4 oth | |
| 700 | 1 | |a Nir, G. |4 oth | |
| 700 | 1 | |a Nelles, A. |4 oth | |
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| 700 | 1 | |a Nozdrina, A. |4 oth | |
| 700 | 1 | |a Oberla, E. |4 oth | |
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| 700 | 1 | |a Osborn, J. |4 oth | |
| 700 | 1 | |a Pan, Y. |4 oth | |
| 700 | 1 | |a Pandya, H. |4 oth | |
| 700 | 1 | |a Paul, M.P. |4 oth | |
| 700 | 1 | |a Persichilli, C. |4 oth | |
| 700 | 1 | |a Pfendner, C. |4 oth | |
| 700 | 1 | |a Plaisier, I. |4 oth | |
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| 700 | 1 | |a Shultz, A. |4 oth | |
| 700 | 1 | |a Smith, D. |4 oth | |
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| 700 | 1 | |a Tatar, J. |4 oth | |
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| 700 | 1 | |a Tosi, D. |4 oth | |
| 700 | 1 | |a Touart, J. |4 oth | |
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| 700 | 1 | |a Vieregg, A.G. |4 oth | |
| 700 | 1 | |a Wang, M.-Z. |4 oth | |
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10.1016/j.astropartphys.2022.102790 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001983.pica (DE-627)ELV059747692 (ELSEVIER)S0927-6505(22)00091-3 DE-627 ger DE-627 rakwb eng 620 VZ 690 VZ 50.92 bkl Aguilar, J.A. verfasserin aut Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments 2023transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. Background rejection Elsevier Ultra-high energy cosmic rays Elsevier Triboelectric effect Elsevier Neutrino Elsevier Anker, A. oth Allison, P. oth Archambault, S. oth Baldi, P. oth Barwick, S.W. oth Beatty, J.J. oth Beise, J. oth Besson, D. oth Bishop, A. oth Bondarev, E. oth Botner, O. oth Bouma, S. oth Buitink, S. oth Cataldo, M. oth Chen, C.C. oth Chen, C.H. oth Chen, P. oth Chen, Y.C. oth Choi, T. oth Clark, B.A. oth Clay, W. oth Curtis-Ginsberg, Z. oth Connolly, A. oth Cremonesi, L. oth Dasgupta, P. oth Davies, J. oth de Kockere, S. oth de Vries, K.D. oth Deaconu, C. oth DuVernois, M.A. oth Flaherty, J. oth Friedman, E. oth Gaior, R. oth Gaswint, G. oth Glaser, C. oth Hallgren, A. oth Hallmann, S. oth Ham, Y.-B. oth Hanson, J.C. oth Harty, N. oth Hendricks, B. oth Hoffman, K.D. oth Hong, E. oth Hornhuber, C. oth Hsu, S.Y. oth Hu, L. oth Huang, J.J. oth Huang, M.-H. oth Hughes, K. oth Ishihara, A. oth Jee, G. oth Jung, J. oth Karle, A. oth Kelley, J.L. oth Klein, S.R. oth Kleinfelder, S.A. oth Kim, J. oth Kim, K.-C. oth Kim, M.-C. oth Kravchenko, I. oth Krebs, R. oth Ku, Y. oth Kuo, C.Y. oth Kurusu, K. oth Kwon, Hyuck-Jin oth Lahmann, R. oth Landsman, H. oth Latif, U. oth Lee, C. oth Leung, C.-H. oth Li, C.-J. oth Liu, J. oth Liu, T.-C. oth Lu, M.-Y. oth Madison, K. oth Mammo, J. oth Mase, K. oth McAleer, S. oth Meures, T. oth Meyers, Z.S. oth Michaels, K. oth Mikhailova, M. oth Mulrey, K. oth Nam, J. oth Nichol, R.J. oth Nir, G. oth Nelles, A. oth Novikov, A. oth Nozdrina, A. oth Oberla, E. oth Oeyen, B. oth Osborn, J. oth Pan, Y. oth Pandya, H. oth Paul, M.P. oth Persichilli, C. oth Pfendner, C. oth Plaisier, I. oth Punsuebsay, N. oth Pyras, L. oth Rice-Smith, R. oth Roth, J. oth Ryckbosch, D. oth Scholten, O. oth Seckel, D. oth Seikh, M.F.H. oth Shiao, Y.-S. oth Shin, B.-K. oth Shultz, A. oth Smith, D. oth Southall, D. oth Tatar, J. oth Torres, J. oth Toscano, S. oth Tosi, D. oth Touart, J. oth Van Den Broeck, D.J. oth van Eijndhoven, N. oth Varner, G.S. oth Vieregg, A.G. oth Wang, M.-Z. oth Wang, S.-H. oth Wang, Y.H. oth Welling, C. oth Williams, D.R. oth Wissel, S. oth Xie, C. oth Yoshida, S. oth Young, R. oth Zhao, L. oth Zink, A. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:145 year:2023 pages:0 https://doi.org/10.1016/j.astropartphys.2022.102790 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 145 2023 0 |
| spelling |
10.1016/j.astropartphys.2022.102790 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001983.pica (DE-627)ELV059747692 (ELSEVIER)S0927-6505(22)00091-3 DE-627 ger DE-627 rakwb eng 620 VZ 690 VZ 50.92 bkl Aguilar, J.A. verfasserin aut Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments 2023transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. Background rejection Elsevier Ultra-high energy cosmic rays Elsevier Triboelectric effect Elsevier Neutrino Elsevier Anker, A. oth Allison, P. oth Archambault, S. oth Baldi, P. oth Barwick, S.W. oth Beatty, J.J. oth Beise, J. oth Besson, D. oth Bishop, A. oth Bondarev, E. oth Botner, O. oth Bouma, S. oth Buitink, S. oth Cataldo, M. oth Chen, C.C. oth Chen, C.H. oth Chen, P. oth Chen, Y.C. oth Choi, T. oth Clark, B.A. oth Clay, W. oth Curtis-Ginsberg, Z. oth Connolly, A. oth Cremonesi, L. oth Dasgupta, P. oth Davies, J. oth de Kockere, S. oth de Vries, K.D. oth Deaconu, C. oth DuVernois, M.A. oth Flaherty, J. oth Friedman, E. oth Gaior, R. oth Gaswint, G. oth Glaser, C. oth Hallgren, A. oth Hallmann, S. oth Ham, Y.-B. oth Hanson, J.C. oth Harty, N. oth Hendricks, B. oth Hoffman, K.D. oth Hong, E. oth Hornhuber, C. oth Hsu, S.Y. oth Hu, L. oth Huang, J.J. oth Huang, M.-H. oth Hughes, K. oth Ishihara, A. oth Jee, G. oth Jung, J. oth Karle, A. oth Kelley, J.L. oth Klein, S.R. oth Kleinfelder, S.A. oth Kim, J. oth Kim, K.-C. oth Kim, M.-C. oth Kravchenko, I. oth Krebs, R. oth Ku, Y. oth Kuo, C.Y. oth Kurusu, K. oth Kwon, Hyuck-Jin oth Lahmann, R. oth Landsman, H. oth Latif, U. oth Lee, C. oth Leung, C.-H. oth Li, C.-J. oth Liu, J. oth Liu, T.-C. oth Lu, M.-Y. oth Madison, K. oth Mammo, J. oth Mase, K. oth McAleer, S. oth Meures, T. oth Meyers, Z.S. oth Michaels, K. oth Mikhailova, M. oth Mulrey, K. oth Nam, J. oth Nichol, R.J. oth Nir, G. oth Nelles, A. oth Novikov, A. oth Nozdrina, A. oth Oberla, E. oth Oeyen, B. oth Osborn, J. oth Pan, Y. oth Pandya, H. oth Paul, M.P. oth Persichilli, C. oth Pfendner, C. oth Plaisier, I. oth Punsuebsay, N. oth Pyras, L. oth Rice-Smith, R. oth Roth, J. oth Ryckbosch, D. oth Scholten, O. oth Seckel, D. oth Seikh, M.F.H. oth Shiao, Y.-S. oth Shin, B.-K. oth Shultz, A. oth Smith, D. oth Southall, D. oth Tatar, J. oth Torres, J. oth Toscano, S. oth Tosi, D. oth Touart, J. oth Van Den Broeck, D.J. oth van Eijndhoven, N. oth Varner, G.S. oth Vieregg, A.G. oth Wang, M.-Z. oth Wang, S.-H. oth Wang, Y.H. oth Welling, C. oth Williams, D.R. oth Wissel, S. oth Xie, C. oth Yoshida, S. oth Young, R. oth Zhao, L. oth Zink, A. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:145 year:2023 pages:0 https://doi.org/10.1016/j.astropartphys.2022.102790 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 145 2023 0 |
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10.1016/j.astropartphys.2022.102790 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001983.pica (DE-627)ELV059747692 (ELSEVIER)S0927-6505(22)00091-3 DE-627 ger DE-627 rakwb eng 620 VZ 690 VZ 50.92 bkl Aguilar, J.A. verfasserin aut Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments 2023transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. Background rejection Elsevier Ultra-high energy cosmic rays Elsevier Triboelectric effect Elsevier Neutrino Elsevier Anker, A. oth Allison, P. oth Archambault, S. oth Baldi, P. oth Barwick, S.W. oth Beatty, J.J. oth Beise, J. oth Besson, D. oth Bishop, A. oth Bondarev, E. oth Botner, O. oth Bouma, S. oth Buitink, S. oth Cataldo, M. oth Chen, C.C. oth Chen, C.H. oth Chen, P. oth Chen, Y.C. oth Choi, T. oth Clark, B.A. oth Clay, W. oth Curtis-Ginsberg, Z. oth Connolly, A. oth Cremonesi, L. oth Dasgupta, P. oth Davies, J. oth de Kockere, S. oth de Vries, K.D. oth Deaconu, C. oth DuVernois, M.A. oth Flaherty, J. oth Friedman, E. oth Gaior, R. oth Gaswint, G. oth Glaser, C. oth Hallgren, A. oth Hallmann, S. oth Ham, Y.-B. oth Hanson, J.C. oth Harty, N. oth Hendricks, B. oth Hoffman, K.D. oth Hong, E. oth Hornhuber, C. oth Hsu, S.Y. oth Hu, L. oth Huang, J.J. oth Huang, M.-H. oth Hughes, K. oth Ishihara, A. oth Jee, G. oth Jung, J. oth Karle, A. oth Kelley, J.L. oth Klein, S.R. oth Kleinfelder, S.A. oth Kim, J. oth Kim, K.-C. oth Kim, M.-C. oth Kravchenko, I. oth Krebs, R. oth Ku, Y. oth Kuo, C.Y. oth Kurusu, K. oth Kwon, Hyuck-Jin oth Lahmann, R. oth Landsman, H. oth Latif, U. oth Lee, C. oth Leung, C.-H. oth Li, C.-J. oth Liu, J. oth Liu, T.-C. oth Lu, M.-Y. oth Madison, K. oth Mammo, J. oth Mase, K. oth McAleer, S. oth Meures, T. oth Meyers, Z.S. oth Michaels, K. oth Mikhailova, M. oth Mulrey, K. oth Nam, J. oth Nichol, R.J. oth Nir, G. oth Nelles, A. oth Novikov, A. oth Nozdrina, A. oth Oberla, E. oth Oeyen, B. oth Osborn, J. oth Pan, Y. oth Pandya, H. oth Paul, M.P. oth Persichilli, C. oth Pfendner, C. oth Plaisier, I. oth Punsuebsay, N. oth Pyras, L. oth Rice-Smith, R. oth Roth, J. oth Ryckbosch, D. oth Scholten, O. oth Seckel, D. oth Seikh, M.F.H. oth Shiao, Y.-S. oth Shin, B.-K. oth Shultz, A. oth Smith, D. oth Southall, D. oth Tatar, J. oth Torres, J. oth Toscano, S. oth Tosi, D. oth Touart, J. oth Van Den Broeck, D.J. oth van Eijndhoven, N. oth Varner, G.S. oth Vieregg, A.G. oth Wang, M.-Z. oth Wang, S.-H. oth Wang, Y.H. oth Welling, C. oth Williams, D.R. oth Wissel, S. oth Xie, C. oth Yoshida, S. oth Young, R. oth Zhao, L. oth Zink, A. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:145 year:2023 pages:0 https://doi.org/10.1016/j.astropartphys.2022.102790 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 145 2023 0 |
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10.1016/j.astropartphys.2022.102790 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001983.pica (DE-627)ELV059747692 (ELSEVIER)S0927-6505(22)00091-3 DE-627 ger DE-627 rakwb eng 620 VZ 690 VZ 50.92 bkl Aguilar, J.A. verfasserin aut Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments 2023transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. Background rejection Elsevier Ultra-high energy cosmic rays Elsevier Triboelectric effect Elsevier Neutrino Elsevier Anker, A. oth Allison, P. oth Archambault, S. oth Baldi, P. oth Barwick, S.W. oth Beatty, J.J. oth Beise, J. oth Besson, D. oth Bishop, A. oth Bondarev, E. oth Botner, O. oth Bouma, S. oth Buitink, S. oth Cataldo, M. oth Chen, C.C. oth Chen, C.H. oth Chen, P. oth Chen, Y.C. oth Choi, T. oth Clark, B.A. oth Clay, W. oth Curtis-Ginsberg, Z. oth Connolly, A. oth Cremonesi, L. oth Dasgupta, P. oth Davies, J. oth de Kockere, S. oth de Vries, K.D. oth Deaconu, C. oth DuVernois, M.A. oth Flaherty, J. oth Friedman, E. oth Gaior, R. oth Gaswint, G. oth Glaser, C. oth Hallgren, A. oth Hallmann, S. oth Ham, Y.-B. oth Hanson, J.C. oth Harty, N. oth Hendricks, B. oth Hoffman, K.D. oth Hong, E. oth Hornhuber, C. oth Hsu, S.Y. oth Hu, L. oth Huang, J.J. oth Huang, M.-H. oth Hughes, K. oth Ishihara, A. oth Jee, G. oth Jung, J. oth Karle, A. oth Kelley, J.L. oth Klein, S.R. oth Kleinfelder, S.A. oth Kim, J. oth Kim, K.-C. oth Kim, M.-C. oth Kravchenko, I. oth Krebs, R. oth Ku, Y. oth Kuo, C.Y. oth Kurusu, K. oth Kwon, Hyuck-Jin oth Lahmann, R. oth Landsman, H. oth Latif, U. oth Lee, C. oth Leung, C.-H. oth Li, C.-J. oth Liu, J. oth Liu, T.-C. oth Lu, M.-Y. oth Madison, K. oth Mammo, J. oth Mase, K. oth McAleer, S. oth Meures, T. oth Meyers, Z.S. oth Michaels, K. oth Mikhailova, M. oth Mulrey, K. oth Nam, J. oth Nichol, R.J. oth Nir, G. oth Nelles, A. oth Novikov, A. oth Nozdrina, A. oth Oberla, E. oth Oeyen, B. oth Osborn, J. oth Pan, Y. oth Pandya, H. oth Paul, M.P. oth Persichilli, C. oth Pfendner, C. oth Plaisier, I. oth Punsuebsay, N. oth Pyras, L. oth Rice-Smith, R. oth Roth, J. oth Ryckbosch, D. oth Scholten, O. oth Seckel, D. oth Seikh, M.F.H. oth Shiao, Y.-S. oth Shin, B.-K. oth Shultz, A. oth Smith, D. oth Southall, D. oth Tatar, J. oth Torres, J. oth Toscano, S. oth Tosi, D. oth Touart, J. oth Van Den Broeck, D.J. oth van Eijndhoven, N. oth Varner, G.S. oth Vieregg, A.G. oth Wang, M.-Z. oth Wang, S.-H. oth Wang, Y.H. oth Welling, C. oth Williams, D.R. oth Wissel, S. oth Xie, C. oth Yoshida, S. oth Young, R. oth Zhao, L. oth Zink, A. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:145 year:2023 pages:0 https://doi.org/10.1016/j.astropartphys.2022.102790 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 145 2023 0 |
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10.1016/j.astropartphys.2022.102790 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001983.pica (DE-627)ELV059747692 (ELSEVIER)S0927-6505(22)00091-3 DE-627 ger DE-627 rakwb eng 620 VZ 690 VZ 50.92 bkl Aguilar, J.A. verfasserin aut Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments 2023transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. Background rejection Elsevier Ultra-high energy cosmic rays Elsevier Triboelectric effect Elsevier Neutrino Elsevier Anker, A. oth Allison, P. oth Archambault, S. oth Baldi, P. oth Barwick, S.W. oth Beatty, J.J. oth Beise, J. oth Besson, D. oth Bishop, A. oth Bondarev, E. oth Botner, O. oth Bouma, S. oth Buitink, S. oth Cataldo, M. oth Chen, C.C. oth Chen, C.H. oth Chen, P. oth Chen, Y.C. oth Choi, T. oth Clark, B.A. oth Clay, W. oth Curtis-Ginsberg, Z. oth Connolly, A. oth Cremonesi, L. oth Dasgupta, P. oth Davies, J. oth de Kockere, S. oth de Vries, K.D. oth Deaconu, C. oth DuVernois, M.A. oth Flaherty, J. oth Friedman, E. oth Gaior, R. oth Gaswint, G. oth Glaser, C. oth Hallgren, A. oth Hallmann, S. oth Ham, Y.-B. oth Hanson, J.C. oth Harty, N. oth Hendricks, B. oth Hoffman, K.D. oth Hong, E. oth Hornhuber, C. oth Hsu, S.Y. oth Hu, L. oth Huang, J.J. oth Huang, M.-H. oth Hughes, K. oth Ishihara, A. oth Jee, G. oth Jung, J. oth Karle, A. oth Kelley, J.L. oth Klein, S.R. oth Kleinfelder, S.A. oth Kim, J. oth Kim, K.-C. oth Kim, M.-C. oth Kravchenko, I. oth Krebs, R. oth Ku, Y. oth Kuo, C.Y. oth Kurusu, K. oth Kwon, Hyuck-Jin oth Lahmann, R. oth Landsman, H. oth Latif, U. oth Lee, C. oth Leung, C.-H. oth Li, C.-J. oth Liu, J. oth Liu, T.-C. oth Lu, M.-Y. oth Madison, K. oth Mammo, J. oth Mase, K. oth McAleer, S. oth Meures, T. oth Meyers, Z.S. oth Michaels, K. oth Mikhailova, M. oth Mulrey, K. oth Nam, J. oth Nichol, R.J. oth Nir, G. oth Nelles, A. oth Novikov, A. oth Nozdrina, A. oth Oberla, E. oth Oeyen, B. oth Osborn, J. oth Pan, Y. oth Pandya, H. oth Paul, M.P. oth Persichilli, C. oth Pfendner, C. oth Plaisier, I. oth Punsuebsay, N. oth Pyras, L. oth Rice-Smith, R. oth Roth, J. oth Ryckbosch, D. oth Scholten, O. oth Seckel, D. oth Seikh, M.F.H. oth Shiao, Y.-S. oth Shin, B.-K. oth Shultz, A. oth Smith, D. oth Southall, D. oth Tatar, J. oth Torres, J. oth Toscano, S. oth Tosi, D. oth Touart, J. oth Van Den Broeck, D.J. oth van Eijndhoven, N. oth Varner, G.S. oth Vieregg, A.G. oth Wang, M.-Z. oth Wang, S.-H. oth Wang, Y.H. oth Welling, C. oth Williams, D.R. oth Wissel, S. oth Xie, C. oth Yoshida, S. oth Young, R. oth Zhao, L. oth Zink, A. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:145 year:2023 pages:0 https://doi.org/10.1016/j.astropartphys.2022.102790 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 145 2023 0 |
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Aguilar, J.A. @@aut@@ Anker, A. @@oth@@ Allison, P. @@oth@@ Archambault, S. @@oth@@ Baldi, P. @@oth@@ Barwick, S.W. @@oth@@ Beatty, J.J. @@oth@@ Beise, J. @@oth@@ Besson, D. @@oth@@ Bishop, A. @@oth@@ Bondarev, E. @@oth@@ Botner, O. @@oth@@ Bouma, S. @@oth@@ Buitink, S. @@oth@@ Cataldo, M. @@oth@@ Chen, C.C. @@oth@@ Chen, C.H. @@oth@@ Chen, P. @@oth@@ Chen, Y.C. @@oth@@ Choi, T. @@oth@@ Clark, B.A. @@oth@@ Clay, W. @@oth@@ Curtis-Ginsberg, Z. @@oth@@ Connolly, A. @@oth@@ Cremonesi, L. @@oth@@ Dasgupta, P. @@oth@@ Davies, J. @@oth@@ de Kockere, S. @@oth@@ de Vries, K.D. @@oth@@ Deaconu, C. @@oth@@ DuVernois, M.A. @@oth@@ Flaherty, J. @@oth@@ Friedman, E. @@oth@@ Gaior, R. @@oth@@ Gaswint, G. @@oth@@ Glaser, C. @@oth@@ Hallgren, A. @@oth@@ Hallmann, S. @@oth@@ Ham, Y.-B. @@oth@@ Hanson, J.C. @@oth@@ Harty, N. @@oth@@ Hendricks, B. @@oth@@ Hoffman, K.D. @@oth@@ Hong, E. @@oth@@ Hornhuber, C. @@oth@@ Hsu, S.Y. @@oth@@ Hu, L. @@oth@@ Huang, J.J. @@oth@@ Huang, M.-H. @@oth@@ Hughes, K. @@oth@@ Ishihara, A. @@oth@@ Jee, G. @@oth@@ Jung, J. @@oth@@ Karle, A. @@oth@@ Kelley, J.L. @@oth@@ Klein, S.R. @@oth@@ Kleinfelder, S.A. @@oth@@ Kim, J. @@oth@@ Kim, K.-C. @@oth@@ Kim, M.-C. @@oth@@ Kravchenko, I. @@oth@@ Krebs, R. @@oth@@ Ku, Y. @@oth@@ Kuo, C.Y. @@oth@@ Kurusu, K. @@oth@@ Kwon, Hyuck-Jin @@oth@@ Lahmann, R. @@oth@@ Landsman, H. @@oth@@ Latif, U. @@oth@@ Lee, C. @@oth@@ Leung, C.-H. @@oth@@ Li, C.-J. @@oth@@ Liu, J. @@oth@@ Liu, T.-C. @@oth@@ Lu, M.-Y. @@oth@@ Madison, K. @@oth@@ Mammo, J. @@oth@@ Mase, K. @@oth@@ McAleer, S. @@oth@@ Meures, T. @@oth@@ Meyers, Z.S. @@oth@@ Michaels, K. @@oth@@ Mikhailova, M. @@oth@@ Mulrey, K. @@oth@@ Nam, J. @@oth@@ Nichol, R.J. @@oth@@ Nir, G. @@oth@@ Nelles, A. @@oth@@ Novikov, A. @@oth@@ Nozdrina, A. @@oth@@ Oberla, E. @@oth@@ Oeyen, B. @@oth@@ Osborn, J. @@oth@@ Pan, Y. @@oth@@ Pandya, H. @@oth@@ Paul, M.P. @@oth@@ Persichilli, C. @@oth@@ Pfendner, C. @@oth@@ Plaisier, I. @@oth@@ Punsuebsay, N. @@oth@@ Pyras, L. @@oth@@ Rice-Smith, R. @@oth@@ Roth, J. @@oth@@ Ryckbosch, D. @@oth@@ Scholten, O. @@oth@@ Seckel, D. @@oth@@ Seikh, M.F.H. @@oth@@ Shiao, Y.-S. @@oth@@ Shin, B.-K. @@oth@@ Shultz, A. @@oth@@ Smith, D. @@oth@@ Southall, D. @@oth@@ Tatar, J. @@oth@@ Torres, J. @@oth@@ Toscano, S. @@oth@@ Tosi, D. @@oth@@ Touart, J. @@oth@@ Van Den Broeck, D.J. @@oth@@ van Eijndhoven, N. @@oth@@ Varner, G.S. @@oth@@ Vieregg, A.G. @@oth@@ Wang, M.-Z. @@oth@@ Wang, S.-H. @@oth@@ Wang, Y.H. @@oth@@ Welling, C. @@oth@@ Williams, D.R. @@oth@@ Wissel, S. @@oth@@ Xie, C. @@oth@@ Yoshida, S. @@oth@@ Young, R. @@oth@@ Zhao, L. @@oth@@ Zink, A. @@oth@@ |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV059747692</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230626053837.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">221219s2023 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.astropartphys.2022.102790</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">/cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001983.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV059747692</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0927-6505(22)00091-3</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">690</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">50.92</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Aguilar, J.A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2023transfer abstract</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Background rejection</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Ultra-high energy cosmic rays</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Triboelectric effect</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Neutrino</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anker, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Allison, P.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" 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| author |
Aguilar, J.A. |
| spellingShingle |
Aguilar, J.A. ddc 620 ddc 690 bkl 50.92 Elsevier Background rejection Elsevier Ultra-high energy cosmic rays Elsevier Triboelectric effect Elsevier Neutrino Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments |
| authorStr |
Aguilar, J.A. |
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Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
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Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
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Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
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10.1016/j.astropartphys.2022.102790 |
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triboelectric backgrounds to radio-based polar ultra-high energy neutrino (uhen) experiments |
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Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments |
| abstract |
In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. |
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In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. |
| abstract_unstemmed |
In the hopes of observing the highest-energy neutrinos (E > 1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference Δ V. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. |
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Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments |
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Anker, A. Allison, P. Archambault, S. Baldi, P. Barwick, S.W. Beatty, J.J. Beise, J. Besson, D. Bishop, A. Bondarev, E. Botner, O. Bouma, S. Buitink, S. Cataldo, M. Chen, C.C. Chen, C.H. Chen, P. Chen, Y.C. Choi, T. Clark, B.A. Clay, W. Curtis-Ginsberg, Z. Connolly, A. Cremonesi, L. Dasgupta, P. Davies, J. de Kockere, S. de Vries, K.D. Deaconu, C. DuVernois, M.A. Flaherty, J. Friedman, E. Gaior, R. Gaswint, G. Glaser, C. Hallgren, A. Hallmann, S. Ham, Y.-B. Hanson, J.C. Harty, N. Hendricks, B. Hoffman, K.D. Hong, E. Hornhuber, C. Hsu, S.Y. Hu, L. Huang, J.J. Huang, M.-H. Hughes, K. Ishihara, A. Jee, G. Jung, J. Karle, A. Kelley, J.L. Klein, S.R. Kleinfelder, S.A. Kim, J. Kim, K.-C. Kim, M.-C. Kravchenko, I. Krebs, R. Ku, Y. Kuo, C.Y. Kurusu, K. Kwon, Hyuck-Jin Lahmann, R. Landsman, H. Latif, U. Lee, C. Leung, C.-H. Li, C.-J. Liu, J. Liu, T.-C. Lu, M.-Y. Madison, K. Mammo, J. Mase, K. McAleer, S. Meures, T. Meyers, Z.S. Michaels, K. Mikhailova, M. Mulrey, K. Nam, J. Nichol, R.J. Nir, G. Nelles, A. Novikov, A. Nozdrina, A. Oberla, E. Oeyen, B. Osborn, J. Pan, Y. Pandya, H. Paul, M.P. Persichilli, C. Pfendner, C. Plaisier, I. Punsuebsay, N. Pyras, L. Rice-Smith, R. Roth, J. Ryckbosch, D. Scholten, O. Seckel, D. Seikh, M.F.H. Shiao, Y.-S. Shin, B.-K. Shultz, A. Smith, D. Southall, D. Tatar, J. Torres, J. Toscano, S. Tosi, D. Touart, J. Van Den Broeck, D.J. van Eijndhoven, N. Varner, G.S. Vieregg, A.G. Wang, M.-Z. Wang, S.-H. Wang, Y.H. Welling, C. Williams, D.R. Wissel, S. Xie, C. Yoshida, S. Young, R. Zhao, L. Zink, A. |
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