The giant radio array for neutrino detection (GRAND): science and design
- Autores
- Álvarez Muñiz, Jaime; Alves Batista, Rafael; Balagopal V, Aswathi; Bolmont, Julien; Bustamante, Mauricio; Carvalho, Washington; Charrier, Didier; Cognard, Ismaël; Decoene, Valentin; Denton, Peter B.; De Jong, Sijbrand; De Vries, Krijn D.; Engel, Ralph; Fang, Ke; Finley, Chad; Gabici, Stefano; Gou, QuanBu; Gu, JunHua; Guépin, Claire; Hu, HongBo; Huang, Yan; Kotera, Kumiko; Le Coz, Sandra; Lenain, Jean-Philippe; Lü, GuoLiang; Martineau Huynh, Olivier; Mostafá, Miguel; Mottez, Fabrice; Murase, Kohta; Niess, Valentin; Oikonomou, Foteini; Pierog, Tanguy; Qian, XiangLi; Qin, Bo; Ran, Duan; Renault-Tinacci, Nicolas; Roth, Markus; Schröder, Frank Gerhard; Schüssler, Fabian; Tueros, Matias Jorge
- Año de publicación
- 2019
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km2. A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND.
Fil: Álvarez Muñiz, Jaime. Universidad de Santiago de Compostela; España
Fil: Alves Batista, Rafael. University of Oxford; Reino Unido. Universidade de Sao Paulo; Brasil
Fil: Balagopal V, Aswathi. Karlsruher Institut Für Technologie; Alemania
Fil: Bolmont, Julien. Université Pierre et Marie Curie; Francia
Fil: Bustamante, Mauricio. Niels Bohr Institutet; Dinamarca. Ohio State University; Estados Unidos
Fil: Carvalho, Washington. Universidad de Santiago de Compostela; España
Fil: Charrier, Didier. Universite de Nantes; Francia
Fil: Cognard, Ismaël. Centre National de la Recherche Scientifique; Francia. Laboratoire de Physique Et Chimie de L’environnement Et de L’espace Lpc2e Cnrs-université D’orléans; Francia
Fil: Decoene, Valentin. Université Pierre et Marie Curie; Francia
Fil: Denton, Peter B.. Niels Bohr Institutet; Dinamarca
Fil: De Jong, Sijbrand. Radboud Universiteit Nijmegen; Países Bajos. Nationaal Instituut voor Kernfysica en Hoge Energie Fysica; Países Bajos
Fil: De Vries, Krijn D.. Vrije Unviversiteit Brussel; Bélgica
Fil: Engel, Ralph. Karlsruher Institut Für Technologie; Alemania
Fil: Fang, Ke. University of Stanford; Estados Unidos. University of Maryland; Estados Unidos. Joint Space-science Institute; Estados Unidos
Fil: Finley, Chad. Stockholms Universitet; Suecia
Fil: Gabici, Stefano. Université Paris Diderot - Paris 7; Francia
Fil: Gou, QuanBu. Chinese Academy of Sciences; República de China
Fil: Gu, JunHua. Chinese Academy of Sciences; República de China
Fil: Guépin, Claire. Université Pierre et Marie Curie; Francia
Fil: Hu, HongBo. Chinese Academy of Sciences; República de China
Fil: Huang, Yan. Chinese Academy of Sciences; República de China
Fil: Kotera, Kumiko. Université Pierre et Marie Curie; Francia
Fil: Le Coz, Sandra. Chinese Academy of Sciences; República de China
Fil: Lenain, Jean-Philippe. Université Pierre et Marie Curie; Francia
Fil: Lü, GuoLiang. Xinjiang University; China
Fil: Martineau Huynh, Olivier. Université Pierre et Marie Curie; Francia. Chinese Academy of Sciences; República de China
Fil: Mostafá, Miguel. State University of Pennsylvania; Estados Unidos
Fil: Mottez, Fabrice. Centre National de la Recherche Scientifique. Observatoire de Paris. Laboratoire de L`univers Et Ses Theories; Francia
Fil: Murase, Kohta. State University of Pennsylvania; Estados Unidos
Fil: Niess, Valentin. Université Clermont Auvergne; Francia
Fil: Oikonomou, Foteini. State University of Pennsylvania; Estados Unidos. European Southern Observatory Chile; Chile
Fil: Pierog, Tanguy. Karlsruher Institut Für Technologie; Alemania
Fil: Qian, XiangLi. Shandong Management University; China
Fil: Qin, Bo. Chinese Academy of Sciences; República de China
Fil: Ran, Duan. Chinese Academy of Sciences; República de China
Fil: Renault-Tinacci, Nicolas. Université Pierre et Marie Curie; Francia
Fil: Roth, Markus. Karlsruher Institut Für Technologie; Alemania
Fil: Schröder, Frank Gerhard. Karlsruher Institut Für Technologie; Alemania. The Bartol Research Institute; Alemania
Fil: Schüssler, Fabian. Universite Paris-Saclay;
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
-
COSMIC RAYS IN ASTRONOMICAL OBSERVATIONS
COSMIC RAYS: GALACTIC AND EXTRAGALACTIC
GALACTIC AND EXTRAGALACTIC
NEUTRINOS IN ASTRONOMICAL OBSERVATIONS
RADIO TELESCOPES
RADIOWAVE RADIATION: SOURCES - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/183829
Ver los metadatos del registro completo
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The giant radio array for neutrino detection (GRAND): science and designÁlvarez Muñiz, JaimeAlves Batista, RafaelBalagopal V, AswathiBolmont, JulienBustamante, MauricioCarvalho, WashingtonCharrier, DidierCognard, IsmaëlDecoene, ValentinDenton, Peter B.De Jong, SijbrandDe Vries, Krijn D.Engel, RalphFang, KeFinley, ChadGabici, StefanoGou, QuanBuGu, JunHuaGuépin, ClaireHu, HongBoHuang, YanKotera, KumikoLe Coz, SandraLenain, Jean-PhilippeLü, GuoLiangMartineau Huynh, OlivierMostafá, MiguelMottez, FabriceMurase, KohtaNiess, ValentinOikonomou, FoteiniPierog, TanguyQian, XiangLiQin, BoRan, DuanRenault-Tinacci, NicolasRoth, MarkusSchröder, Frank GerhardSchüssler, FabianTueros, Matias JorgeCOSMIC RAYS IN ASTRONOMICAL OBSERVATIONSCOSMIC RAYS: GALACTIC AND EXTRAGALACTICGALACTIC AND EXTRAGALACTICNEUTRINOS IN ASTRONOMICAL OBSERVATIONSRADIO TELESCOPESRADIOWAVE RADIATION: SOURCEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km2. A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND.Fil: Álvarez Muñiz, Jaime. Universidad de Santiago de Compostela; EspañaFil: Alves Batista, Rafael. University of Oxford; Reino Unido. Universidade de Sao Paulo; BrasilFil: Balagopal V, Aswathi. Karlsruher Institut Für Technologie; AlemaniaFil: Bolmont, Julien. Université Pierre et Marie Curie; FranciaFil: Bustamante, Mauricio. Niels Bohr Institutet; Dinamarca. Ohio State University; Estados UnidosFil: Carvalho, Washington. Universidad de Santiago de Compostela; EspañaFil: Charrier, Didier. Universite de Nantes; FranciaFil: Cognard, Ismaël. Centre National de la Recherche Scientifique; Francia. Laboratoire de Physique Et Chimie de L’environnement Et de L’espace Lpc2e Cnrs-université D’orléans; FranciaFil: Decoene, Valentin. Université Pierre et Marie Curie; FranciaFil: Denton, Peter B.. Niels Bohr Institutet; DinamarcaFil: De Jong, Sijbrand. Radboud Universiteit Nijmegen; Países Bajos. Nationaal Instituut voor Kernfysica en Hoge Energie Fysica; Países BajosFil: De Vries, Krijn D.. Vrije Unviversiteit Brussel; BélgicaFil: Engel, Ralph. Karlsruher Institut Für Technologie; AlemaniaFil: Fang, Ke. University of Stanford; Estados Unidos. University of Maryland; Estados Unidos. Joint Space-science Institute; Estados UnidosFil: Finley, Chad. Stockholms Universitet; SueciaFil: Gabici, Stefano. Université Paris Diderot - Paris 7; FranciaFil: Gou, QuanBu. Chinese Academy of Sciences; República de ChinaFil: Gu, JunHua. Chinese Academy of Sciences; República de ChinaFil: Guépin, Claire. Université Pierre et Marie Curie; FranciaFil: Hu, HongBo. Chinese Academy of Sciences; República de ChinaFil: Huang, Yan. Chinese Academy of Sciences; República de ChinaFil: Kotera, Kumiko. Université Pierre et Marie Curie; FranciaFil: Le Coz, Sandra. Chinese Academy of Sciences; República de ChinaFil: Lenain, Jean-Philippe. Université Pierre et Marie Curie; FranciaFil: Lü, GuoLiang. Xinjiang University; ChinaFil: Martineau Huynh, Olivier. Université Pierre et Marie Curie; Francia. Chinese Academy of Sciences; República de ChinaFil: Mostafá, Miguel. State University of Pennsylvania; Estados UnidosFil: Mottez, Fabrice. Centre National de la Recherche Scientifique. Observatoire de Paris. Laboratoire de L`univers Et Ses Theories; FranciaFil: Murase, Kohta. State University of Pennsylvania; Estados UnidosFil: Niess, Valentin. Université Clermont Auvergne; FranciaFil: Oikonomou, Foteini. State University of Pennsylvania; Estados Unidos. European Southern Observatory Chile; ChileFil: Pierog, Tanguy. Karlsruher Institut Für Technologie; AlemaniaFil: Qian, XiangLi. Shandong Management University; ChinaFil: Qin, Bo. Chinese Academy of Sciences; República de ChinaFil: Ran, Duan. Chinese Academy of Sciences; República de ChinaFil: Renault-Tinacci, Nicolas. Université Pierre et Marie Curie; FranciaFil: Roth, Markus. Karlsruher Institut Für Technologie; AlemaniaFil: Schröder, Frank Gerhard. Karlsruher Institut Für Technologie; Alemania. The Bartol Research Institute; AlemaniaFil: Schüssler, Fabian. Universite Paris-Saclay;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; ArgentinaSpringer2019-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/183829Álvarez Muñiz, Jaime; Alves Batista, Rafael; Balagopal V, Aswathi; Bolmont, Julien; Bustamante, Mauricio; et al.; The giant radio array for neutrino detection (GRAND): science and design; Springer; Science China: Physics, Mechanics and Astronomy; 63; 1; 8-2019; 1-451674-73481869-1927CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://link.springer.com/10.1007/s11433-018-9385-7info:eu-repo/semantics/altIdentifier/doi/10.1007/s11433-018-9385-7info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1810.09994info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:27:12Zoai:ri.conicet.gov.ar:11336/183829instacron: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 10:27:12.733CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The giant radio array for neutrino detection (GRAND): science and design |
| title |
The giant radio array for neutrino detection (GRAND): science and design |
| spellingShingle |
The giant radio array for neutrino detection (GRAND): science and design Álvarez Muñiz, Jaime COSMIC RAYS IN ASTRONOMICAL OBSERVATIONS COSMIC RAYS: GALACTIC AND EXTRAGALACTIC GALACTIC AND EXTRAGALACTIC NEUTRINOS IN ASTRONOMICAL OBSERVATIONS RADIO TELESCOPES RADIOWAVE RADIATION: SOURCES |
| title_short |
The giant radio array for neutrino detection (GRAND): science and design |
| title_full |
The giant radio array for neutrino detection (GRAND): science and design |
| title_fullStr |
The giant radio array for neutrino detection (GRAND): science and design |
| title_full_unstemmed |
The giant radio array for neutrino detection (GRAND): science and design |
| title_sort |
The giant radio array for neutrino detection (GRAND): science and design |
| dc.creator.none.fl_str_mv |
Álvarez Muñiz, Jaime Alves Batista, Rafael Balagopal V, Aswathi Bolmont, Julien Bustamante, Mauricio Carvalho, Washington Charrier, Didier Cognard, Ismaël Decoene, Valentin Denton, Peter B. De Jong, Sijbrand De Vries, Krijn D. Engel, Ralph Fang, Ke Finley, Chad Gabici, Stefano Gou, QuanBu Gu, JunHua Guépin, Claire Hu, HongBo Huang, Yan Kotera, Kumiko Le Coz, Sandra Lenain, Jean-Philippe Lü, GuoLiang Martineau Huynh, Olivier Mostafá, Miguel Mottez, Fabrice Murase, Kohta Niess, Valentin Oikonomou, Foteini Pierog, Tanguy Qian, XiangLi Qin, Bo Ran, Duan Renault-Tinacci, Nicolas Roth, Markus Schröder, Frank Gerhard Schüssler, Fabian Tueros, Matias Jorge |
| author |
Álvarez Muñiz, Jaime |
| author_facet |
Álvarez Muñiz, Jaime Alves Batista, Rafael Balagopal V, Aswathi Bolmont, Julien Bustamante, Mauricio Carvalho, Washington Charrier, Didier Cognard, Ismaël Decoene, Valentin Denton, Peter B. De Jong, Sijbrand De Vries, Krijn D. Engel, Ralph Fang, Ke Finley, Chad Gabici, Stefano Gou, QuanBu Gu, JunHua Guépin, Claire Hu, HongBo Huang, Yan Kotera, Kumiko Le Coz, Sandra Lenain, Jean-Philippe Lü, GuoLiang Martineau Huynh, Olivier Mostafá, Miguel Mottez, Fabrice Murase, Kohta Niess, Valentin Oikonomou, Foteini Pierog, Tanguy Qian, XiangLi Qin, Bo Ran, Duan Renault-Tinacci, Nicolas Roth, Markus Schröder, Frank Gerhard Schüssler, Fabian Tueros, Matias Jorge |
| author_role |
author |
| author2 |
Alves Batista, Rafael Balagopal V, Aswathi Bolmont, Julien Bustamante, Mauricio Carvalho, Washington Charrier, Didier Cognard, Ismaël Decoene, Valentin Denton, Peter B. De Jong, Sijbrand De Vries, Krijn D. Engel, Ralph Fang, Ke Finley, Chad Gabici, Stefano Gou, QuanBu Gu, JunHua Guépin, Claire Hu, HongBo Huang, Yan Kotera, Kumiko Le Coz, Sandra Lenain, Jean-Philippe Lü, GuoLiang Martineau Huynh, Olivier Mostafá, Miguel Mottez, Fabrice Murase, Kohta Niess, Valentin Oikonomou, Foteini Pierog, Tanguy Qian, XiangLi Qin, Bo Ran, Duan Renault-Tinacci, Nicolas Roth, Markus Schröder, Frank Gerhard Schüssler, Fabian Tueros, Matias Jorge |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
COSMIC RAYS IN ASTRONOMICAL OBSERVATIONS COSMIC RAYS: GALACTIC AND EXTRAGALACTIC GALACTIC AND EXTRAGALACTIC NEUTRINOS IN ASTRONOMICAL OBSERVATIONS RADIO TELESCOPES RADIOWAVE RADIATION: SOURCES |
| topic |
COSMIC RAYS IN ASTRONOMICAL OBSERVATIONS COSMIC RAYS: GALACTIC AND EXTRAGALACTIC GALACTIC AND EXTRAGALACTIC NEUTRINOS IN ASTRONOMICAL OBSERVATIONS RADIO TELESCOPES RADIOWAVE RADIATION: SOURCES |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km2. A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND. Fil: Álvarez Muñiz, Jaime. Universidad de Santiago de Compostela; España Fil: Alves Batista, Rafael. University of Oxford; Reino Unido. Universidade de Sao Paulo; Brasil Fil: Balagopal V, Aswathi. Karlsruher Institut Für Technologie; Alemania Fil: Bolmont, Julien. Université Pierre et Marie Curie; Francia Fil: Bustamante, Mauricio. Niels Bohr Institutet; Dinamarca. Ohio State University; Estados Unidos Fil: Carvalho, Washington. Universidad de Santiago de Compostela; España Fil: Charrier, Didier. Universite de Nantes; Francia Fil: Cognard, Ismaël. Centre National de la Recherche Scientifique; Francia. Laboratoire de Physique Et Chimie de L’environnement Et de L’espace Lpc2e Cnrs-université D’orléans; Francia Fil: Decoene, Valentin. Université Pierre et Marie Curie; Francia Fil: Denton, Peter B.. Niels Bohr Institutet; Dinamarca Fil: De Jong, Sijbrand. Radboud Universiteit Nijmegen; Países Bajos. Nationaal Instituut voor Kernfysica en Hoge Energie Fysica; Países Bajos Fil: De Vries, Krijn D.. Vrije Unviversiteit Brussel; Bélgica Fil: Engel, Ralph. Karlsruher Institut Für Technologie; Alemania Fil: Fang, Ke. University of Stanford; Estados Unidos. University of Maryland; Estados Unidos. Joint Space-science Institute; Estados Unidos Fil: Finley, Chad. Stockholms Universitet; Suecia Fil: Gabici, Stefano. Université Paris Diderot - Paris 7; Francia Fil: Gou, QuanBu. Chinese Academy of Sciences; República de China Fil: Gu, JunHua. Chinese Academy of Sciences; República de China Fil: Guépin, Claire. Université Pierre et Marie Curie; Francia Fil: Hu, HongBo. Chinese Academy of Sciences; República de China Fil: Huang, Yan. Chinese Academy of Sciences; República de China Fil: Kotera, Kumiko. Université Pierre et Marie Curie; Francia Fil: Le Coz, Sandra. Chinese Academy of Sciences; República de China Fil: Lenain, Jean-Philippe. Université Pierre et Marie Curie; Francia Fil: Lü, GuoLiang. Xinjiang University; China Fil: Martineau Huynh, Olivier. Université Pierre et Marie Curie; Francia. Chinese Academy of Sciences; República de China Fil: Mostafá, Miguel. State University of Pennsylvania; Estados Unidos Fil: Mottez, Fabrice. Centre National de la Recherche Scientifique. Observatoire de Paris. Laboratoire de L`univers Et Ses Theories; Francia Fil: Murase, Kohta. State University of Pennsylvania; Estados Unidos Fil: Niess, Valentin. Université Clermont Auvergne; Francia Fil: Oikonomou, Foteini. State University of Pennsylvania; Estados Unidos. European Southern Observatory Chile; Chile Fil: Pierog, Tanguy. Karlsruher Institut Für Technologie; Alemania Fil: Qian, XiangLi. Shandong Management University; China Fil: Qin, Bo. Chinese Academy of Sciences; República de China Fil: Ran, Duan. Chinese Academy of Sciences; República de China Fil: Renault-Tinacci, Nicolas. Université Pierre et Marie Curie; Francia Fil: Roth, Markus. Karlsruher Institut Für Technologie; Alemania Fil: Schröder, Frank Gerhard. Karlsruher Institut Für Technologie; Alemania. The Bartol Research Institute; Alemania Fil: Schüssler, Fabian. Universite Paris-Saclay; 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 |
The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km2. A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND. |
| publishDate |
2019 |
| dc.date.none.fl_str_mv |
2019-08 |
| 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/11336/183829 Álvarez Muñiz, Jaime; Alves Batista, Rafael; Balagopal V, Aswathi; Bolmont, Julien; Bustamante, Mauricio; et al.; The giant radio array for neutrino detection (GRAND): science and design; Springer; Science China: Physics, Mechanics and Astronomy; 63; 1; 8-2019; 1-45 1674-7348 1869-1927 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/183829 |
| identifier_str_mv |
Álvarez Muñiz, Jaime; Alves Batista, Rafael; Balagopal V, Aswathi; Bolmont, Julien; Bustamante, Mauricio; et al.; The giant radio array for neutrino detection (GRAND): science and design; Springer; Science China: Physics, Mechanics and Astronomy; 63; 1; 8-2019; 1-45 1674-7348 1869-1927 CONICET Digital CONICET |
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eng |
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eng |
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Springer |
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Springer |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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