Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays

Autores
Decoene, Valentin; Martineau Huynh, Olivier; Tueros, Matias Jorge
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Radio-detection is becoming an established technique for the detection of air showers induced by cosmic particles. This is in particular true at the highest energies, where very large detection areas are required. A proper description of the shape of the radio wavefront emitted by air showers may allow to reconstruct the properties of its parent particle. In this article, we show that for showers with zenith angles larger than 60° – those targeted by giant radio arrays detecting extensive air showers induced by cosmic particles –, a point-source-like description of the radio wavefront allows to constraint the lateral position of the shower axis within a few meters. Following, we show that the reconstructed longitudinal position of this point source is correlated with the nature of the cosmic rays initiating the shower. Further systematic studies are pending to determine the robustness of this parameter and its validity as a proxy for cosmic ray composition studies.
Fil: Decoene, Valentin. The Pennsylvania State University; Estados Unidos
Fil: Martineau Huynh, Olivier. Université Pierre et Marie Curie; Francia
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Materia
EXTENSIVE-AIR-SHOWERS PHYSICS
RADIO
RADIO-DETECTION
RADIO-EMISSION
ULTRA-HIGH-ENERGY COSMIC RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/248604

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network_name_str CONICET Digital (CONICET)
spelling Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arraysDecoene, ValentinMartineau Huynh, OlivierTueros, Matias JorgeEXTENSIVE-AIR-SHOWERS PHYSICSRADIORADIO-DETECTIONRADIO-EMISSIONULTRA-HIGH-ENERGY COSMIC RAYSULTRA-HIGH-ENERGY NEUTRINOShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Radio-detection is becoming an established technique for the detection of air showers induced by cosmic particles. This is in particular true at the highest energies, where very large detection areas are required. A proper description of the shape of the radio wavefront emitted by air showers may allow to reconstruct the properties of its parent particle. In this article, we show that for showers with zenith angles larger than 60° – those targeted by giant radio arrays detecting extensive air showers induced by cosmic particles –, a point-source-like description of the radio wavefront allows to constraint the lateral position of the shower axis within a few meters. Following, we show that the reconstructed longitudinal position of this point source is correlated with the nature of the cosmic rays initiating the shower. Further systematic studies are pending to determine the robustness of this parameter and its validity as a proxy for cosmic ray composition studies.Fil: Decoene, Valentin. The Pennsylvania State University; Estados UnidosFil: Martineau Huynh, Olivier. Université Pierre et Marie Curie; FranciaFil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaElsevier Science2023-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/248604Decoene, Valentin; Martineau Huynh, Olivier; Tueros, Matias Jorge; Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays; Elsevier Science; Astroparticle Physics; 145; 3-2023; 102779-1028030927-6505CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2022.102779info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0927650522000809info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:40:49Zoai:ri.conicet.gov.ar:11336/248604instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:40:49.67CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
title Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
spellingShingle Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
Decoene, Valentin
EXTENSIVE-AIR-SHOWERS PHYSICS
RADIO
RADIO-DETECTION
RADIO-EMISSION
ULTRA-HIGH-ENERGY COSMIC RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
title_short Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
title_full Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
title_fullStr Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
title_full_unstemmed Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
title_sort Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
dc.creator.none.fl_str_mv Decoene, Valentin
Martineau Huynh, Olivier
Tueros, Matias Jorge
author Decoene, Valentin
author_facet Decoene, Valentin
Martineau Huynh, Olivier
Tueros, Matias Jorge
author_role author
author2 Martineau Huynh, Olivier
Tueros, Matias Jorge
author2_role author
author
dc.subject.none.fl_str_mv EXTENSIVE-AIR-SHOWERS PHYSICS
RADIO
RADIO-DETECTION
RADIO-EMISSION
ULTRA-HIGH-ENERGY COSMIC RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
topic EXTENSIVE-AIR-SHOWERS PHYSICS
RADIO
RADIO-DETECTION
RADIO-EMISSION
ULTRA-HIGH-ENERGY COSMIC RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Radio-detection is becoming an established technique for the detection of air showers induced by cosmic particles. This is in particular true at the highest energies, where very large detection areas are required. A proper description of the shape of the radio wavefront emitted by air showers may allow to reconstruct the properties of its parent particle. In this article, we show that for showers with zenith angles larger than 60° – those targeted by giant radio arrays detecting extensive air showers induced by cosmic particles –, a point-source-like description of the radio wavefront allows to constraint the lateral position of the shower axis within a few meters. Following, we show that the reconstructed longitudinal position of this point source is correlated with the nature of the cosmic rays initiating the shower. Further systematic studies are pending to determine the robustness of this parameter and its validity as a proxy for cosmic ray composition studies.
Fil: Decoene, Valentin. The Pennsylvania State University; Estados Unidos
Fil: Martineau Huynh, Olivier. Université Pierre et Marie Curie; Francia
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
description Radio-detection is becoming an established technique for the detection of air showers induced by cosmic particles. This is in particular true at the highest energies, where very large detection areas are required. A proper description of the shape of the radio wavefront emitted by air showers may allow to reconstruct the properties of its parent particle. In this article, we show that for showers with zenith angles larger than 60° – those targeted by giant radio arrays detecting extensive air showers induced by cosmic particles –, a point-source-like description of the radio wavefront allows to constraint the lateral position of the shower axis within a few meters. Following, we show that the reconstructed longitudinal position of this point source is correlated with the nature of the cosmic rays initiating the shower. Further systematic studies are pending to determine the robustness of this parameter and its validity as a proxy for cosmic ray composition studies.
publishDate 2023
dc.date.none.fl_str_mv 2023-03
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/248604
Decoene, Valentin; Martineau Huynh, Olivier; Tueros, Matias Jorge; Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays; Elsevier Science; Astroparticle Physics; 145; 3-2023; 102779-102803
0927-6505
CONICET Digital
CONICET
url http://hdl.handle.net/11336/248604
identifier_str_mv Decoene, Valentin; Martineau Huynh, Olivier; Tueros, Matias Jorge; Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays; Elsevier Science; Astroparticle Physics; 145; 3-2023; 102779-102803
0927-6505
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2022.102779
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0927650522000809
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Elsevier Science
publisher.none.fl_str_mv Elsevier Science
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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