Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ
The description of the methodology and results of searching for air showers generated by neutral particles such as high energy gamma quanta and astroneutrinos are presented. For this purpose, we conducted a comprehensive analysis of the data: the electron, the muon and the EAS Cerenkov light, and th...
| Glavni autori: | , , |
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| Format: | Članak |
| Jezik: | English |
| Izdano: |
EDP Sciences
2017-01-01
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| Serija: | EPJ Web of Conferences |
| Online pristup: | https://doi.org/10.1051/epjconf/201714507005 |
| _version_ | 1828930113563000832 |
|---|---|
| author | Knurenko Stanislav Petrov Igor Sabourov Artem |
| author_facet | Knurenko Stanislav Petrov Igor Sabourov Artem |
| author_sort | Knurenko Stanislav |
| collection | DOAJ |
| description | The description of the methodology and results of searching for air showers generated by neutral particles such as high energy gamma quanta and astroneutrinos are presented. For this purpose, we conducted a comprehensive analysis of the data: the electron, the muon and the EAS Cerenkov light, and their response time in scintillation and Cherenkov detectors. Air showers with energy more than 5·1018 eV and zenith angle θ ≥ 55∘ are selected and analyzed. Search results indicate a lack of air shower events formed by gamma-rays or high-energy neutrinos, but it does not mean that such air showers do not exist in nature; for example, experiments that recorded showers having a marked low muon content, i.e., “Muonless”, are likely to be candidates for showers produced by neutral primary particles. |
| first_indexed | 2024-12-14T00:27:56Z |
| format | Article |
| id | doaj.art-a3fdee947fb84d7899b4eef6f36c5ea8 |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-14T00:27:56Z |
| publishDate | 2017-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-a3fdee947fb84d7899b4eef6f36c5ea82022-12-21T23:24:59ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011450700510.1051/epjconf/201714507005epjconf-isvhecri2016_07005Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θKnurenko StanislavPetrov IgorSabourov ArtemThe description of the methodology and results of searching for air showers generated by neutral particles such as high energy gamma quanta and astroneutrinos are presented. For this purpose, we conducted a comprehensive analysis of the data: the electron, the muon and the EAS Cerenkov light, and their response time in scintillation and Cherenkov detectors. Air showers with energy more than 5·1018 eV and zenith angle θ ≥ 55∘ are selected and analyzed. Search results indicate a lack of air shower events formed by gamma-rays or high-energy neutrinos, but it does not mean that such air showers do not exist in nature; for example, experiments that recorded showers having a marked low muon content, i.e., “Muonless”, are likely to be candidates for showers produced by neutral primary particles.https://doi.org/10.1051/epjconf/201714507005 |
| spellingShingle | Knurenko Stanislav Petrov Igor Sabourov Artem Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ EPJ Web of Conferences |
| title | Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ |
| title_full | Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ |
| title_fullStr | Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ |
| title_full_unstemmed | Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ |
| title_short | Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ |
| title_sort | search for neutrino generated air shower candidates with energy ≥ 1019 ev and zenith angle θ |
| url | https://doi.org/10.1051/epjconf/201714507005 |
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