Radio signatures of cosmic-ray showers with deep in-ice antennas
To detect ultra-high-energy neutrinos, experiments such as ARA and RNO-G target the radio emission these particles induce when cascading in the ice, using deep antennas in South Pole or in Greenland. One of the main backgrounds for such signals is the radio emission generated by cosmic-ray showers,...
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| creator | Chiche, Simon Moller, Nicolas Bishop, Abby de Kockere, Simon de Vries, Krijn D Latif, Uzair Toscano, Simona |
| description | To detect ultra-high-energy neutrinos, experiments such as ARA and RNO-G
target the radio emission these particles induce when cascading in the ice,
using deep antennas in South Pole or in Greenland. One of the main backgrounds
for such signals is the radio emission generated by cosmic-ray showers, either
directly in the ice, or in the air and transmitted to the ice, which can both
reach the deep antennas. The first detection of cosmic rays with deep antennas
would thus validate this detection principle and allow us to calibrate the
detectors. FAERIE, the Framework for the simulation of Air shower Emission of
Radio for in-Ice Experiments, is a numerical tool that couples both CoREAS and
GEANT4 Monte-Carlo codes to simulate the radio emission from cosmic-ray showers
deep in the ice. Using this code, we will investigate cosmic-ray radio
signatures and the possible implications on the design of a cosmic-ray veto. |
| doi_str_mv | 10.48550/arxiv.2409.02185 |
| format | Article |
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target the radio emission these particles induce when cascading in the ice,
using deep antennas in South Pole or in Greenland. One of the main backgrounds
for such signals is the radio emission generated by cosmic-ray showers, either
directly in the ice, or in the air and transmitted to the ice, which can both
reach the deep antennas. The first detection of cosmic rays with deep antennas
would thus validate this detection principle and allow us to calibrate the
detectors. FAERIE, the Framework for the simulation of Air shower Emission of
Radio for in-Ice Experiments, is a numerical tool that couples both CoREAS and
GEANT4 Monte-Carlo codes to simulate the radio emission from cosmic-ray showers
deep in the ice. Using this code, we will investigate cosmic-ray radio
signatures and the possible implications on the design of a cosmic-ray veto.</description><identifier>DOI: 10.48550/arxiv.2409.02185</identifier><language>eng</language><subject>Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics</subject><creationdate>2024-09</creationdate><rights>http://creativecommons.org/licenses/by-nc-nd/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2409.02185$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2409.02185$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Chiche, Simon</creatorcontrib><creatorcontrib>Moller, Nicolas</creatorcontrib><creatorcontrib>Bishop, Abby</creatorcontrib><creatorcontrib>de Kockere, Simon</creatorcontrib><creatorcontrib>de Vries, Krijn D</creatorcontrib><creatorcontrib>Latif, Uzair</creatorcontrib><creatorcontrib>Toscano, Simona</creatorcontrib><title>Radio signatures of cosmic-ray showers with deep in-ice antennas</title><description>To detect ultra-high-energy neutrinos, experiments such as ARA and RNO-G
target the radio emission these particles induce when cascading in the ice,
using deep antennas in South Pole or in Greenland. One of the main backgrounds
for such signals is the radio emission generated by cosmic-ray showers, either
directly in the ice, or in the air and transmitted to the ice, which can both
reach the deep antennas. The first detection of cosmic rays with deep antennas
would thus validate this detection principle and allow us to calibrate the
detectors. FAERIE, the Framework for the simulation of Air shower Emission of
Radio for in-Ice Experiments, is a numerical tool that couples both CoREAS and
GEANT4 Monte-Carlo codes to simulate the radio emission from cosmic-ray showers
deep in the ice. Using this code, we will investigate cosmic-ray radio
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target the radio emission these particles induce when cascading in the ice,
using deep antennas in South Pole or in Greenland. One of the main backgrounds
for such signals is the radio emission generated by cosmic-ray showers, either
directly in the ice, or in the air and transmitted to the ice, which can both
reach the deep antennas. The first detection of cosmic rays with deep antennas
would thus validate this detection principle and allow us to calibrate the
detectors. FAERIE, the Framework for the simulation of Air shower Emission of
Radio for in-Ice Experiments, is a numerical tool that couples both CoREAS and
GEANT4 Monte-Carlo codes to simulate the radio emission from cosmic-ray showers
deep in the ice. Using this code, we will investigate cosmic-ray radio
signatures and the possible implications on the design of a cosmic-ray veto.</abstract><doi>10.48550/arxiv.2409.02185</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics |
| title | Radio signatures of cosmic-ray showers with deep in-ice antennas |
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