Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment
Upper limits are presented on the diffuse flux of ultra-high energy $ν_e$, based on analysis of data taken by the RICE experiment during August, 2000. The RICE receiver array at South Pole monitors cold ice for radio-wavelength Cherenkov radiation resulting from neutrino-induced in-ice showers. For...
Main Author: | |
---|---|
Format: | Text |
Language: | unknown |
Published: |
arXiv
2002
|
Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0206371 https://arxiv.org/abs/astro-ph/0206371 |
id |
ftdatacite:10.48550/arxiv.astro-ph/0206371 |
---|---|
record_format |
openpolar |
spelling |
ftdatacite:10.48550/arxiv.astro-ph/0206371 2023-05-15T18:22:23+02:00 Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment Kravchenko, I. 2002 https://dx.doi.org/10.48550/arxiv.astro-ph/0206371 https://arxiv.org/abs/astro-ph/0206371 unknown arXiv https://dx.doi.org/10.1016/s0927-6505(03)00181-6 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph High Energy Physics - Experiment hep-ex FOS Physical sciences article-journal Article ScholarlyArticle Text 2002 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0206371 https://doi.org/10.1016/s0927-6505(03)00181-6 2022-04-01T16:40:22Z Upper limits are presented on the diffuse flux of ultra-high energy $ν_e$, based on analysis of data taken by the RICE experiment during August, 2000. The RICE receiver array at South Pole monitors cold ice for radio-wavelength Cherenkov radiation resulting from neutrino-induced in-ice showers. For energies above 1 EeV, RICE is an effective detector of over 15 km$^3$ sr. Potential signal events are separated from backgrounds using vertex location, event reconstruction, and signal shape. These are the first terrestrial limits exploiting the physics of radio Cherenkov emissions from charged-current $ν_e+N\to e+N'$ interactions. : 29 pages, 10 Figures (Latex2e), Revised version submitted to Astroparticle Physics. Revisions include: Extended discussion of systematic uncertainties. Extended discussion of event rates due to "hadronic channels". Revised limits due to changes in monte carlo simulation Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
Astrophysics astro-ph High Energy Physics - Experiment hep-ex FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph High Energy Physics - Experiment hep-ex FOS Physical sciences Kravchenko, I. Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment |
topic_facet |
Astrophysics astro-ph High Energy Physics - Experiment hep-ex FOS Physical sciences |
description |
Upper limits are presented on the diffuse flux of ultra-high energy $ν_e$, based on analysis of data taken by the RICE experiment during August, 2000. The RICE receiver array at South Pole monitors cold ice for radio-wavelength Cherenkov radiation resulting from neutrino-induced in-ice showers. For energies above 1 EeV, RICE is an effective detector of over 15 km$^3$ sr. Potential signal events are separated from backgrounds using vertex location, event reconstruction, and signal shape. These are the first terrestrial limits exploiting the physics of radio Cherenkov emissions from charged-current $ν_e+N\to e+N'$ interactions. : 29 pages, 10 Figures (Latex2e), Revised version submitted to Astroparticle Physics. Revisions include: Extended discussion of systematic uncertainties. Extended discussion of event rates due to "hadronic channels". Revised limits due to changes in monte carlo simulation |
format |
Text |
author |
Kravchenko, I. |
author_facet |
Kravchenko, I. |
author_sort |
Kravchenko, I. |
title |
Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment |
title_short |
Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment |
title_full |
Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment |
title_fullStr |
Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment |
title_full_unstemmed |
Limits on the Ultra-High Energy Electron Neutrino Flux from the RICE Experiment |
title_sort |
limits on the ultra-high energy electron neutrino flux from the rice experiment |
publisher |
arXiv |
publishDate |
2002 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0206371 https://arxiv.org/abs/astro-ph/0206371 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1016/s0927-6505(03)00181-6 |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0206371 https://doi.org/10.1016/s0927-6505(03)00181-6 |
_version_ |
1766201796374560768 |