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description Publicationkeyboard_double_arrow_right Article , Research , Preprint 2023Embargo end date: 01 Jan 2023 France, Australia, Slovenia, France, Chile, Netherlands, France, France, Australia, France, Slovenia, France, France, Spain, Germany, France, Croatia, France, France, Italy, France, United Kingdom, Poland, Slovenia, Germany, France, Croatia, Germany, France, SpainPublisher:Elsevier BV Funded by:EC | CTA-PP, EC | INFIERI, EC | MSCA4Ukraine +8 projectsEC| CTA-PP ,EC| INFIERI ,EC| MSCA4Ukraine ,AKA| Intrinsic Very High Energy Gamma-ray Emission of Blazars ,AKA| Intrinsic Very High Energy Gamma-ray Emission of Blazars ,EC| CTA-DEV ,EC| P-SPHERE ,UKRI| RootDetect: Remote Detection and Precision Management of Root Health ,EC| PREBIST ,NSERC ,EC| ESCAPEAcero, F.; Acharyya, A.; Adam, R.; Aguasca-Cabot, A.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, J.; Aloisio, R.; Crespo, N. Álvarez; Alves Batista, R.; Amati, L.; Amato, E.; Ambrosi, G.; Angüner, E. O.; Aramo, C.; Arcaro, C.; Armstrong, T.; Asano, K.; Ascasibar, Y.; Aschersleben, J.; Backes, M.; Baktash, A.; Balazs, C.; Balbo, M.; Ballet, J.; Larriva, A. Baquero; Barbosa Martins, V.; de Almeida, U. Barres; Barrio, J. A.; Bastieri, D.; Baxter, J. R.; Becker Tjus, J.; Benbow, W.; Bernardos-Martín, M. I.; Bernete, J.; Berti, A.; Bertucci, B.; Beshley, V.; Bhattacharjee, P.; Bhattacharyya, S.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Bordas, P.; Bottacini, E.; Bregeon, J.; Brose, R.; Bucciantini, N.; Bulgarelli, A.; Capasso, M.; Dolcetta, R. A. Capuzzo; Caraveo, P.; Cardillo, M.; Carosi, R.; Casanova, S.; Cascone, E.; Cassol, F.; Catalani, F.; Cerruti, M.; Chadwick, P.; Chaty, S.; Chen, A.; Chernyakova, M.; Chiavassa, A.; Chudoba, J.; Coimbra-Araujo, C.; Conforti, V.; Contreras, J. L.; Costa, A.; Costantini, H.; Cristofari, P.; Crocker, R.; D'Amico, G.; D'Ammando, F.; De Angelis, A.; De Caprio, V.; de Gouveia Dal Pino, E. M.; de Ona Wilhelmi, E.; de Souza, V.; Delgado, C.; della Volpe, D.; Depaoli, D.; Di Girolamo, T.; Di Pierro, F.; Di Tria, R.; Di Venere, L.; Diebold, S.; Djuvsland, J. I.; Donini, A.; Doro, M.; Anjos, R. d. C. Dos; Dwarkadas, V. V.; Einecke, S.; Elsässer, D.; Emery, G.; Evoli, C.; Falceta-Goncalves, D.; Fedorova, E.; Fegan, S.; Ferrand, G.; Fiandrini, E.; Filipovic, M.; Fioretti, V.; Fiori, M.; Foffano, L.; Fontaine, G.; Fukami, S.; Galanti, G.; Galaz, G.; Gammaldi, V.; Gasbarra, C.; Ghalumyan, A.; Ghirlanda, G.; Giarrusso, M.; Giavitto, G.; Giglietto, N.; Giordano, F.; Giroletti, M.; Giuliani, A.; Giunti, L.; Godinovic, N.; Coelho, J. Goulart; Gréaux, L.; Green, D.; Grondin, M.-H.; Gueta, O.; Gunji, S.; Hassan, T.; Heller, M.; Hernández-Cadena, S.; Hinton, J.; Hnatyk, B.; Hnatyk, R.; Hoffmann, D.; Hofmann, W.; Holder, J.; Horan, D.; Horvath, P.; Hrabovsky, M.; Hrupec, D.; Inada, T.; Incardona, F.; Inoue, S.; Ishio, K.; Jamrozy, M.; Janecek, P.; Martínez, I. Jiménez; Jin, W.; Jung-Richardt, I.; Jurysek, J.; Kaaret, P.; Karas, V.; Katz, U.; Kerszberg, D.; Khélifi, B.; Kieda, D. B.; Kissmann, R.; Kleiner, T.; Kluge, G.; Kluzniak, W.; Knödlseder, J.; Kobayashi, Y.; Kohri, K.; Komin, N.; Kornecki, P.; Kubo, H.; La Palombara, N.; Láinez, M.; Lamastra, A.; Lapington, J.; Lemoine-Goumard, M.; Lenain, J.-P.; Leone, F.; Leto, G.; Leuschner, F.; Lindfors, E.; Liodakis, I.; Lohse, T.; Lombardi, S.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Luque-Escamilla, P. L.; Macias, O.; Mackey, J.; Majumdar, P.; Mandat, D.; Manganaro, M.; Manicò, G.; Marconi, M.; Martí, J.; Martínez, G.; Martinez, M.; Martinez, O.; Mello, A. J. T. S.; Menchiari, S.; Meyer, D. M.-A.;handle: 11588/976647 , 11368/3047904 , 11245.1/26aa360c-6d24-4c9c-aef9-a636a93560c4 , 11370/74d54dea-9889-489b-af9b-675ecdf2eff6 , 10261/334192 , 10281/523759 , 11365/1273955 , 21.11116/0000-000D-A09B-F , 21.11116/0000-000D-A09D-D , 20.500.12556/RUNG-8136-953b8912-bf09-e99f-62b7-80e960af1492 , 11577/3478554 , 11589/254461 , 11391/1591774 , 11697/203019 , 20.500.11769/558462 , 2318/1931012 , 1959.7/uws:71480 , 2440/140227
handle: 11588/976647 , 11368/3047904 , 11245.1/26aa360c-6d24-4c9c-aef9-a636a93560c4 , 11370/74d54dea-9889-489b-af9b-675ecdf2eff6 , 10261/334192 , 10281/523759 , 11365/1273955 , 21.11116/0000-000D-A09B-F , 21.11116/0000-000D-A09D-D , 20.500.12556/RUNG-8136-953b8912-bf09-e99f-62b7-80e960af1492 , 11577/3478554 , 11589/254461 , 11391/1591774 , 11697/203019 , 20.500.11769/558462 , 2318/1931012 , 1959.7/uws:71480 , 2440/140227
The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy $γ$-ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte--Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a $γ$-ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 hours of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with $\mathcal{O}(100)$ hours of exposure per source. 34 pages, 16 figures, Accepted for publication in Astroparticle Physics
Usiena air - Univers... arrow_drop_down HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi di Siena: USiena airArticle . 2023Full-Text: https://hdl.handle.net/11365/1273955Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2023Data sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2023License: taverneData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2023License: taverneData sources: University of Groningen Research PortalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2023Data sources: OA@INAF - Istituto Nazionale di AstrofisicaDiposit Digital de la Universitat de BarcelonaArticle . 2023License: CC BY NC NDData sources: Diposit Digital de la Universitat de BarcelonaCroatian Scientific Bibliography - CROSBIArticle . 2023Data sources: Croatian Scientific Bibliography - CROSBIRepository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023IRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttp://dx.doi.org/10.48550/arX...Article . 2023 . Peer-reviewedData sources: European Union Open Data PortalPontificia Universidad Católica de Chile: Repositorio UCArticle . 2025Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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more_vert Usiena air - Univers... arrow_drop_down HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi di Siena: USiena airArticle . 2023Full-Text: https://hdl.handle.net/11365/1273955Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2023Data sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2023License: taverneData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2023License: taverneData sources: University of Groningen Research PortalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2023Data sources: OA@INAF - Istituto Nazionale di AstrofisicaDiposit Digital de la Universitat de BarcelonaArticle . 2023License: CC BY NC NDData sources: Diposit Digital de la Universitat de BarcelonaCroatian Scientific Bibliography - CROSBIArticle . 2023Data sources: Croatian Scientific Bibliography - CROSBIRepository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023IRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttp://dx.doi.org/10.48550/arX...Article . 2023 . Peer-reviewedData sources: European Union Open Data PortalPontificia Universidad Católica de Chile: Repositorio UCArticle . 2025Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.astropartphys.2023.102850&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Research , Preprint , Journal 2021Embargo end date: 01 Jan 2021 Netherlands, Italy, Slovenia, Netherlands, Spain, Czech Republic, Italy, Italy, Italy, Argentina, Netherlands, Netherlands, France, Italy, Germany, Czech Republic, Belgium, Italy, Argentina, Italy, Germany, NetherlandsPublisher:Springer Science and Business Media LLC Funded by:NSF | Pierre Auger Project, ANR | SUPERNSF| Pierre Auger Project ,ANR| SUPERG. Medina-Tanco; J. Stasielak; G. Farrar; Trent D. Grubb; Sullivan Marafico; F. C. T. Barbato; Rodrigo Guedes Lang; P. Abreu; Kai Daumiller; Adriana Vásquez-Ramírez; E.E. Pereira Martins; E.E. Pereira Martins; S. Querchfeld; Andres Travaini; Juan Manuel González; V. Scherini; François Montanet; Jonathan Blazek; Eleonora Guido; Marcel Köpke; J. de Oliveira; D. Lo Presti; A. M. Botti; Juan Miguel Carceller; O. Martínez Bravo; Jacco Vink; L. Perrone; M. Risse; A. Parra; A. Saftoiu; A. Machado Payeras; H. Wilczyński; Gualberto Avila; J. R. T. de Mello Neto; A.L. Garcia Vegas; I. Allekotte; B. Tome; Marc Weber; Kathrin Bismark; Kathrin Bismark; A. Di Matteo; Lorenzo Cazon; C. Pérez Bertolli; C. Pérez Bertolli; Alina Nasr-Esfahani; Paolo Privitera; Miguel Mostafa; M. E. Bertaina; W. M. Namasaka; Fabio Convenga; C. J.W.P. Timmermans; Fabian Gobbi; Fernando Contreras; L. Valore; A. Streich; A. Streich; Giovanni Consolati; Karen S. Caballero-Mora; Q. Luce; Raul Sarmento; M. Schimassek; M. Schimassek; Esteban Roulet; A. Haungs; J. Pȩkala; Martin Vacula; Virginia Binet; Vladimir Lenok; Niklas Langner; Carlos Escobar; Antonella Castellina; M. R. Hampel; Nataliia Borodai; A. A. Nucita; N. Kunka; Marco Aglietta; M. Zavrtanik; A.C. Cobos Cerutti; J. Rautenberg; R. López; Clara Keiko Oliveira Watanabe; R. Squartini; Josina Schulte; J. Vicha; M. del Río; Florian Lukas Briechle; Maximilian Stadelmaier; Maximilian Stadelmaier; G. De Mauro; J. Kleinfeller; M. Platino; John Matthews; M. Wirtz; S. Petrera; Giovanni Mancarella; Jon Paul Lundquist; Humberto Ibarguen Salazar; Octavian Sima; L. Nožka; Rossella Caruso; G. C. Hill; Carla Taricco; Kevin-Druis Merenda; Juan Pablo Gongora; Antonio Condorelli; Pierre Billoir; Philipp Papenbreer; Lino Miramonti; G. Golup; Carlo Ventura; G. Parente; Denis Stanca; Felix Schlüter; Felix Schlüter; Peter Buchholz; B. Andrada; R. Alves Batista; Toshihiro Fujii; Toshihiro Fujii; H. Martinez; A. Insolia; G. Cataldi; Alan Coleman; Corinne Berat; Cristina Galea; Alina Mihaela Badescu; G. P. Guedes; L. Lu; Orazio Zapparrata; B. Wundheiler; A. Filipčič; Peter L. Biermann; A. Weindl; Maria-Teresa Dova; Marcus Niechciol; E. De Vito; Jan Ebr; Jonathan Biteau; Isabel Goos; Isabel Goos; Jonas Glombitza; Fridtjof Feldbusch; D. D. dos Santos; Jeffrey Brack; V. de Souza; Radomir Smida; H.O. Klages; Jörg R. Hörandel; Ladislav Chytka; A. C. Fauth; M. I. Micheletti; Ioana Caracas; Julien Manshanden; L. Zehrer; W. Rodrigues de Carvalho; Vincenzo Rizi; Martina Bohacova; Zoé Torrès; Thomas Hebbeker; Frank G. Schröder; Frank G. Schröder; Petr Hamal; Alena Bakalova; Günter Sigl; Lukáš Vaclavek; J. Ridky; F. Riehn; Tomáš Fodran; K. Mulrey; Miroslav Pech; Juan Carlos D'Olivo; D. Ravignani; E. Varela; Markus Roth; M. A. Leigui de Oliveira; Claudio Galelli; Antonio Bueno; Marco Giammarchi; M. Palatka; R. Sato; Roberto Mussa; Olivier Deligny; C. Hojvat; Fabrizia Canfora; Sara Martinelli; Sara Martinelli; L. M. Domingues Mendes; David Wittkowski; P.R. Araújo Ferreira; Max Büsken; Max Büsken; Thomas Bretz; S. J. De Jong; M. Unger; Carla Aramo; M. Kleifges; Daniela Mockler; Daniela Mockler; Marcos Cerda; Serguei Vorobiov;doi: 10.1140/epjc/s10052-021-09700-w , 10.48550/arxiv.2109.13400 , 10.18154/rwth-2021-12100 , 10.18154/rwth-2022-00047
handle: https://repository.ubn.ru.nl/handle/2066/239867 , 11588/890384 , 11245.1/e277820a-6074-4fdc-9cd2-9d87842d0efe , 2066/239867 , 2434/1033134 , 10481/71942 , 20.500.12556/RUNG-6965 , 11311/1189557 , 20.500.14017/fb76dc10-e5e8-4ff6-88c2-75af44762dfb , 11697/176134 , 11587/458363 , 20.500.11769/526705 , 2318/1841975 , 2133/23683
doi: 10.1140/epjc/s10052-021-09700-w , 10.48550/arxiv.2109.13400 , 10.18154/rwth-2021-12100 , 10.18154/rwth-2022-00047
handle: https://repository.ubn.ru.nl/handle/2066/239867 , 11588/890384 , 11245.1/e277820a-6074-4fdc-9cd2-9d87842d0efe , 2066/239867 , 2434/1033134 , 10481/71942 , 20.500.12556/RUNG-6965 , 11311/1189557 , 20.500.14017/fb76dc10-e5e8-4ff6-88c2-75af44762dfb , 11697/176134 , 11587/458363 , 20.500.11769/526705 , 2318/1841975 , 2133/23683
AbstractWe present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface detector of the Pierre Auger Observatory that has a spacing of 750 m. An inflection of the spectrum is observed, confirming the presence of the so-called second-knee feature. The spectrum is then combined with that of the 1500 m array to produce a single measurement of the flux, linking this spectral feature with the three additional breaks at the highest energies. The combined spectrum, with an energy scale set calorimetrically via fluorescence telescopes and using a single detector type, results in the most statistically and systematically precise measurement of spectral breaks yet obtained. These measurements are critical for furthering our understanding of the highest energy cosmic rays.
Archivio Istituziona... arrow_drop_down RepHipUNR - Repositorio Hipermedial de la Universidad Nacional de RosarioArticle . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)European Physical Journal C: Particles and FieldsArticle . 2021 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2021License: CC BYData sources: Universiteit van Amsterdam Digital Academic RepositoryRepository of the Czech Academy of SciencesArticle . 2021Data sources: Repository of the Czech Academy of SciencesVrije Universiteit Brussel Research PortalArticle . 2021Data sources: Vrije Universiteit Brussel Research PortalMémoires en Sciences de l'Information et de la CommunicationPreprint . 2021Publikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityPublikationsserver der RWTH Aachen UniversityArticle . 2021Data sources: Publikationsserver der RWTH Aachen UniversityUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2021Data sources: Repository of University of Nova GoricaRepositorio Institucional Universidad de GranadaArticle . 2021License: CC BYData sources: Repositorio Institucional Universidad de GranadaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di Cataniaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1140/epjc/s10052-021-09700-w&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 73 citations 73 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down RepHipUNR - Repositorio Hipermedial de la Universidad Nacional de RosarioArticle . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)European Physical Journal C: Particles and FieldsArticle . 2021 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2021License: CC BYData sources: Universiteit van Amsterdam Digital Academic RepositoryRepository of the Czech Academy of SciencesArticle . 2021Data sources: Repository of the Czech Academy of SciencesVrije Universiteit Brussel Research PortalArticle . 2021Data sources: Vrije Universiteit Brussel Research PortalMémoires en Sciences de l'Information et de la CommunicationPreprint . 2021Publikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityPublikationsserver der RWTH Aachen UniversityArticle . 2021Data sources: Publikationsserver der RWTH Aachen UniversityUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2021Data sources: Repository of University of Nova GoricaRepositorio Institucional Universidad de GranadaArticle . 2021License: CC BYData sources: Repositorio Institucional Universidad de GranadaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di Cataniaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1140/epjc/s10052-021-09700-w&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2024Embargo end date: 01 Jan 2024 FrancePublisher:American Astronomical Society Funded by:ANR | MICRO, ANR | P2IO, ANR | IPSANR| MICRO ,ANR| P2IO ,ANR| IPSSullivan Marafico; Jonathan Biteau; Antonio Condorelli; Olivier Deligny; Johan Bregeon;Abstract The arrival directions of ultrahigh-energy cosmic rays (UHECRs) observed above 4 × 1019 eV provide evidence of localized excesses that are key to identifying their sources. We leverage the 3D matter distribution from optical and infrared surveys as a density model of UHECR sources, which are considered to be transient. Agreement of the sky model with UHECR data imposes constraints on both the emission rate per unit matter and the time spread induced by encountered turbulent magnetic fields. Based on radio measurements of cosmic magnetism, we identify the Local Sheet as the magnetized structure responsible for the kiloyear duration of UHECR bursts for an observer on Earth and find that the turbulence amplitude must be within 0.5–20 nG for a coherence length of 10 kpc. At the same time, the burst-rate density must be above 50 Gpc−3 yr−1 for Local Sheet galaxies to reproduce the UHECR excesses and below 5000 Gpc−3 yr−1 (30,000 Gpc−3 yr−1) for the Milky Way (Local Group galaxies) not to outshine other galaxies. For the transient emissions of protons and nuclei to match the energy spectra of UHECRs, the kinetic energy of the outflows responsible for UHECR acceleration must be below 4 × 1054 erg and above 5 × 1050 erg (2 × 1049 erg) if we consider the Milky Way (or not). The only stellar-sized transients that satisfy both Hillas’ and our criteria are long-duration gamma-ray bursts.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ad5a11&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu2 citations 2 popularity Average influence Average impulse Average Powered by BIP!more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ad5a11&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Journal 2016Embargo end date: 01 Jan 2016 Spain, Netherlands, Italy, Netherlands, Italy, Germany, Italy, Netherlands, Netherlands, Italy, France, Italy, Australia, Germany, Italy, Italy, Australia, Italy, GermanyPublisher:American Physical Society (APS) Funded by:DFG, EC | EPLANET, NSF | Pierre Auger Project +5 projectsDFG ,EC| EPLANET ,NSF| Pierre Auger Project ,MIUR ,EC| AUGER2FUTURE ,ANR| SUPER ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| The Highest Energy Astroparticle PhysicsG. Cataldi; A. Yushkov; Karl-Heinz Kampert; Zbigniew Szadkowski; R. Piegaia; A. Shadkam; S. G. Blaess; F. Suarez; Antonio Bueno; Igor Katkov; R. Sato; Olivier Deligny; M. L. Díaz Castro; Stefano D'Amico; Rossella Caruso; J. A.J. Matthews; Julien Aublin; Julien Aublin; J. Biteau; H.O. Klages; Jörg R. Hörandel; E. J. Quel; Jan Ebr; Jeffrey A. Johnsen; M. Pimenta; A. López Casado; C. Aramo; Francesca Zuccarello; Danielle LaHurd; M. Unger; Rúben Conceição; Stijn Buitink; B. Tome; Brian Fick; Marco Torri; Martin Erdmann; H. Gemmeke; J. Phuntsok; Silvia Mollerach; M. R. Hampel; Esteban Roulet; S. Quinn; J. R. Vázquez; L. A. S. Pereira; D. Nosek; G. Medina-Tanco; N. Krohm; F. Salamida; A. E. Herve; J. R. T. de Mello Neto; G. A. Anastasi; B. Sarkar; Carlos Escobar; J. Debatin; Antonella Castellina; V. M. Theodoro; Nataliia Borodai; Jaime Alvarez-Muñiz; David Walz; Dieter Heck; B. Revenu; A. Dorofeev; A. C. Rovero; M. Kleifges; Markus Lauscher; O. Martínez Bravo; R. A. Vázquez; Marc Weber; A. Di Matteo; J. Stasielak; G. Farrar; L. Ochilo; R.J. Barreira Luz; R.J. Barreira Luz; Xavier Bertou; A. Blanco; A. Blanco; Martina Bohacova; M. J. Cooper; A. Śmiałkowski; Katrin Link; M. Ambrosio; Samo Stanič; I. Naranjo; G. van Aar; Max Malacari; C. Porowski; J. Alvarez Castillo; Norberto Fazzini; Tim Huege; S. J. De Jong; B. Vargas Cárdenas; Carla Bonifazi; I.M. Brancus; B. Wundheiler; A. Filipčič; M. Schauer; J. Neuser; André Schulz; L. Perrone; Pavel Horvath; Andrej Dundovic; Trent D. Grubb; Peter Buchholz; J. W. Cronin; Marcus Niechciol; S. J. Sciutto; Marco Aglietta; Marco Aglietta; N. Kunka; R.C. dos Anjos; D. Martello; J. Hulsman; S. Messina; Tim Niggemann; S. Jansen; Benedikt Zimmermann; A. Fuster; P. Sanchez-Lucas; V. Novotny; Lorenzo Caccianiga; Christine Peters; Thomas Harrison; M. Trini; Ingomar Allekotte; L. Niemietz; M. Zavrtanik; R. López; F. Sánchez; E. Santos; G. Torralba Elipe; Nicolás González; M. Risse; Francesco Strafella; H. Wilczyński; Gualberto Avila; Harald Schieler; L. Molina-Bueno; Heino Falcke; John N. Matthews; Alan Watson; Kai Daumiller; Octavian Fratu; Gaia Silli; Alberto Daniel Supanitsky; P. Ristori; I. A. Minaya; M. Erfani; Johannes Schulz; F. Montanet; A. Lucero; R. Squartini; J. Vicha; F. Canfora; Paula Gina Isar; S. Mathys; Lili Yang; A. Kuotb Awad; Martin Urban; Alexandru Balaceanu; J. J. Masías Meza; P. Abreu; P. Abreu; F. Diogo; J. Ridky; Charles Timmermans; Carlos Hojvat; H. Nožka; C. J. Todero Peixoto; A. G. Mariazzi; R. Gaior; L. Nellen; Philipp Papenbreer; Foteini Oikonomou; R. Legumina; A. G. Chavez; Luis A. Nunez; Peter Mazur; M. Prouza; L. Valore; Darko Veberič; Mihai Niculescu-Oglinzanu; M. Plum; David Wittkowski; E.M. Holt; Corbin Covault; Florian Lukas Briechle; L. Lopes; S. Querchfeld; Paul M. Mantsch; Hernán Asorey; Hernán Asorey; Lukas Middendorf; A. Parra; Denise Boncioli; P. Pieroni; E. Kemp; Enrique Zas; R. Ramos-Pollan; R. Sarmento;We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles range from $10^{-19}$ (cm$^{2}$ sr s)$^{-1}$ for a Lorentz factor $��=10^9$ to $2.5 \times10^{-21}$ (cm$^{2}$ sr s)$^{-1}$ for $��=10^{12}$. These results - the first obtained with a UHECR detector - improve previously published limits by up to an order of magnitude. Published version. Corrected title. Added journal reference and DOI. Added Report Number
Archivio Istituziona... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2016Data sources: Bielefeld Academic Search Engine (BASE)https://link.aps.org/accepted/...ArticleLicense: publisher-specific, author manuscriptData sources: UnpayWallRecolector de Ciencia Abierta, RECOLECTAArticle . 2016Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2016 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2016Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2016Data sources: INRIA a CCSD electronic archive serverhttps://doi.org/10.1103/physre...Article . 2016 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://hdl.handle.net/11370/e...Article . 2016Data sources: DANS (Data Archiving and Networked Services)https://dx.doi.org/10.48550/ar...Article . 2016License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.94.082002&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 15 citations 15 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2016Data sources: Bielefeld Academic Search Engine (BASE)https://link.aps.org/accepted/...ArticleLicense: publisher-specific, author manuscriptData sources: UnpayWallRecolector de Ciencia Abierta, RECOLECTAArticle . 2016Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2016 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2016Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2016Data sources: INRIA a CCSD electronic archive serverhttps://doi.org/10.1103/physre...Article . 2016 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://hdl.handle.net/11370/e...Article . 2016Data sources: DANS (Data Archiving and Networked Services)https://dx.doi.org/10.48550/ar...Article . 2016License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.94.082002&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Preprint , Book 2022Embargo end date: 01 Jan 2022 Germany, FrancePublisher:American Astronomical Society Funded by:ANR | MICRO, ANR | P2IO, ANR | IPSANR| MICRO ,ANR| P2IO ,ANR| IPSQuentin Luce; Sullivan Marafico; Jonathan Biteau; Antonio Condorelli; Olivier Deligny;Abstract Interactions of ultra-high energy cosmic rays (UHECRs) accelerated in specific astrophysical environments have been shown to shape the energy production rate of nuclei differently from that of the secondary neutrons escaping from the confinement zone. Here, we aim at testing a generic scenario of in-source interactions through phenomenological modeling of the flux and composition of UHECRs. We fit a model in which nucleons and nuclei follow different particle energy distributions to the all-particle energy spectrum and proton spectrum below the ankle energy and distributions of maximum shower depths above this energy, as inferred at the Pierre Auger Observatory. We obtain that the data can be reproduced using a spatial distribution of sources that follows the density of extragalactic matter on both local and large scales, providing hence a realistic set of constraints for the emission mechanisms in cosmic accelerators, for their energetics, and for the abundances of elements at escape from their environments. While the quasi monoelemental increase of the cosmic-ray mass number observed on Earth from ≃2 EeV up to the highest energies calls for nuclei accelerated with a hard spectral index, the inferred flux of protons down to ≃0.6 EeV is shown to require for this population a spectral index significantly softer than that generally obtained up to now. We demonstrate that modeling UHECR data across the ankle substantiates the conjecture of in-source interactions in a robust statistical framework, although pushing the mechanism to the extreme.
KITopen (Karlsruhe I... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Book . 2024License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2022License: CC BYData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ac81cc&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 11 citations 11 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert KITopen (Karlsruhe I... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Book . 2024License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2022License: CC BYData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ac81cc&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu
description Publicationkeyboard_double_arrow_right Article , Research , Preprint 2023Embargo end date: 01 Jan 2023 France, Australia, Slovenia, France, Chile, Netherlands, France, France, Australia, France, Slovenia, France, France, Spain, Germany, France, Croatia, France, France, Italy, France, United Kingdom, Poland, Slovenia, Germany, France, Croatia, Germany, France, SpainPublisher:Elsevier BV Funded by:EC | CTA-PP, EC | INFIERI, EC | MSCA4Ukraine +8 projectsEC| CTA-PP ,EC| INFIERI ,EC| MSCA4Ukraine ,AKA| Intrinsic Very High Energy Gamma-ray Emission of Blazars ,AKA| Intrinsic Very High Energy Gamma-ray Emission of Blazars ,EC| CTA-DEV ,EC| P-SPHERE ,UKRI| RootDetect: Remote Detection and Precision Management of Root Health ,EC| PREBIST ,NSERC ,EC| ESCAPEAcero, F.; Acharyya, A.; Adam, R.; Aguasca-Cabot, A.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, J.; Aloisio, R.; Crespo, N. Álvarez; Alves Batista, R.; Amati, L.; Amato, E.; Ambrosi, G.; Angüner, E. O.; Aramo, C.; Arcaro, C.; Armstrong, T.; Asano, K.; Ascasibar, Y.; Aschersleben, J.; Backes, M.; Baktash, A.; Balazs, C.; Balbo, M.; Ballet, J.; Larriva, A. Baquero; Barbosa Martins, V.; de Almeida, U. Barres; Barrio, J. A.; Bastieri, D.; Baxter, J. R.; Becker Tjus, J.; Benbow, W.; Bernardos-Martín, M. I.; Bernete, J.; Berti, A.; Bertucci, B.; Beshley, V.; Bhattacharjee, P.; Bhattacharyya, S.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Bordas, P.; Bottacini, E.; Bregeon, J.; Brose, R.; Bucciantini, N.; Bulgarelli, A.; Capasso, M.; Dolcetta, R. A. Capuzzo; Caraveo, P.; Cardillo, M.; Carosi, R.; Casanova, S.; Cascone, E.; Cassol, F.; Catalani, F.; Cerruti, M.; Chadwick, P.; Chaty, S.; Chen, A.; Chernyakova, M.; Chiavassa, A.; Chudoba, J.; Coimbra-Araujo, C.; Conforti, V.; Contreras, J. L.; Costa, A.; Costantini, H.; Cristofari, P.; Crocker, R.; D'Amico, G.; D'Ammando, F.; De Angelis, A.; De Caprio, V.; de Gouveia Dal Pino, E. M.; de Ona Wilhelmi, E.; de Souza, V.; Delgado, C.; della Volpe, D.; Depaoli, D.; Di Girolamo, T.; Di Pierro, F.; Di Tria, R.; Di Venere, L.; Diebold, S.; Djuvsland, J. I.; Donini, A.; Doro, M.; Anjos, R. d. C. Dos; Dwarkadas, V. V.; Einecke, S.; Elsässer, D.; Emery, G.; Evoli, C.; Falceta-Goncalves, D.; Fedorova, E.; Fegan, S.; Ferrand, G.; Fiandrini, E.; Filipovic, M.; Fioretti, V.; Fiori, M.; Foffano, L.; Fontaine, G.; Fukami, S.; Galanti, G.; Galaz, G.; Gammaldi, V.; Gasbarra, C.; Ghalumyan, A.; Ghirlanda, G.; Giarrusso, M.; Giavitto, G.; Giglietto, N.; Giordano, F.; Giroletti, M.; Giuliani, A.; Giunti, L.; Godinovic, N.; Coelho, J. Goulart; Gréaux, L.; Green, D.; Grondin, M.-H.; Gueta, O.; Gunji, S.; Hassan, T.; Heller, M.; Hernández-Cadena, S.; Hinton, J.; Hnatyk, B.; Hnatyk, R.; Hoffmann, D.; Hofmann, W.; Holder, J.; Horan, D.; Horvath, P.; Hrabovsky, M.; Hrupec, D.; Inada, T.; Incardona, F.; Inoue, S.; Ishio, K.; Jamrozy, M.; Janecek, P.; Martínez, I. Jiménez; Jin, W.; Jung-Richardt, I.; Jurysek, J.; Kaaret, P.; Karas, V.; Katz, U.; Kerszberg, D.; Khélifi, B.; Kieda, D. B.; Kissmann, R.; Kleiner, T.; Kluge, G.; Kluzniak, W.; Knödlseder, J.; Kobayashi, Y.; Kohri, K.; Komin, N.; Kornecki, P.; Kubo, H.; La Palombara, N.; Láinez, M.; Lamastra, A.; Lapington, J.; Lemoine-Goumard, M.; Lenain, J.-P.; Leone, F.; Leto, G.; Leuschner, F.; Lindfors, E.; Liodakis, I.; Lohse, T.; Lombardi, S.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Luque-Escamilla, P. L.; Macias, O.; Mackey, J.; Majumdar, P.; Mandat, D.; Manganaro, M.; Manicò, G.; Marconi, M.; Martí, J.; Martínez, G.; Martinez, M.; Martinez, O.; Mello, A. J. T. S.; Menchiari, S.; Meyer, D. M.-A.;handle: 11588/976647 , 11368/3047904 , 11245.1/26aa360c-6d24-4c9c-aef9-a636a93560c4 , 11370/74d54dea-9889-489b-af9b-675ecdf2eff6 , 10261/334192 , 10281/523759 , 11365/1273955 , 21.11116/0000-000D-A09B-F , 21.11116/0000-000D-A09D-D , 20.500.12556/RUNG-8136-953b8912-bf09-e99f-62b7-80e960af1492 , 11577/3478554 , 11589/254461 , 11391/1591774 , 11697/203019 , 20.500.11769/558462 , 2318/1931012 , 1959.7/uws:71480 , 2440/140227
handle: 11588/976647 , 11368/3047904 , 11245.1/26aa360c-6d24-4c9c-aef9-a636a93560c4 , 11370/74d54dea-9889-489b-af9b-675ecdf2eff6 , 10261/334192 , 10281/523759 , 11365/1273955 , 21.11116/0000-000D-A09B-F , 21.11116/0000-000D-A09D-D , 20.500.12556/RUNG-8136-953b8912-bf09-e99f-62b7-80e960af1492 , 11577/3478554 , 11589/254461 , 11391/1591774 , 11697/203019 , 20.500.11769/558462 , 2318/1931012 , 1959.7/uws:71480 , 2440/140227
The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy $γ$-ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte--Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a $γ$-ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 hours of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with $\mathcal{O}(100)$ hours of exposure per source. 34 pages, 16 figures, Accepted for publication in Astroparticle Physics
Usiena air - Univers... arrow_drop_down HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi di Siena: USiena airArticle . 2023Full-Text: https://hdl.handle.net/11365/1273955Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2023Data sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2023License: taverneData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2023License: taverneData sources: University of Groningen Research PortalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2023Data sources: OA@INAF - Istituto Nazionale di AstrofisicaDiposit Digital de la Universitat de BarcelonaArticle . 2023License: CC BY NC NDData sources: Diposit Digital de la Universitat de BarcelonaCroatian Scientific Bibliography - CROSBIArticle . 2023Data sources: Croatian Scientific Bibliography - CROSBIRepository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023IRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttp://dx.doi.org/10.48550/arX...Article . 2023 . Peer-reviewedData sources: European Union Open Data PortalPontificia Universidad Católica de Chile: Repositorio UCArticle . 2025Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.astropartphys.2023.102850&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 80visibility views 80 download downloads 28 Powered bymore_vert Usiena air - Univers... arrow_drop_down HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi di Siena: USiena airArticle . 2023Full-Text: https://hdl.handle.net/11365/1273955Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Full-Text: https://hal.science/hal-04300157Data sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2023Data sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2023License: taverneData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2023License: taverneData sources: University of Groningen Research PortalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2023Data sources: OA@INAF - Istituto Nazionale di AstrofisicaDiposit Digital de la Universitat de BarcelonaArticle . 2023License: CC BY NC NDData sources: Diposit Digital de la Universitat de BarcelonaCroatian Scientific Bibliography - CROSBIArticle . 2023Data sources: Croatian Scientific Bibliography - CROSBIRepository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023IRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttp://dx.doi.org/10.48550/arX...Article . 2023 . Peer-reviewedData sources: European Union Open Data PortalPontificia Universidad Católica de Chile: Repositorio UCArticle . 2025Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.astropartphys.2023.102850&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Research , Preprint , Journal 2021Embargo end date: 01 Jan 2021 Netherlands, Italy, Slovenia, Netherlands, Spain, Czech Republic, Italy, Italy, Italy, Argentina, Netherlands, Netherlands, France, Italy, Germany, Czech Republic, Belgium, Italy, Argentina, Italy, Germany, NetherlandsPublisher:Springer Science and Business Media LLC Funded by:NSF | Pierre Auger Project, ANR | SUPERNSF| Pierre Auger Project ,ANR| SUPERG. Medina-Tanco; J. Stasielak; G. Farrar; Trent D. Grubb; Sullivan Marafico; F. C. T. Barbato; Rodrigo Guedes Lang; P. Abreu; Kai Daumiller; Adriana Vásquez-Ramírez; E.E. Pereira Martins; E.E. Pereira Martins; S. Querchfeld; Andres Travaini; Juan Manuel González; V. Scherini; François Montanet; Jonathan Blazek; Eleonora Guido; Marcel Köpke; J. de Oliveira; D. Lo Presti; A. M. Botti; Juan Miguel Carceller; O. Martínez Bravo; Jacco Vink; L. Perrone; M. Risse; A. Parra; A. Saftoiu; A. Machado Payeras; H. Wilczyński; Gualberto Avila; J. R. T. de Mello Neto; A.L. Garcia Vegas; I. Allekotte; B. Tome; Marc Weber; Kathrin Bismark; Kathrin Bismark; A. Di Matteo; Lorenzo Cazon; C. Pérez Bertolli; C. Pérez Bertolli; Alina Nasr-Esfahani; Paolo Privitera; Miguel Mostafa; M. E. Bertaina; W. M. Namasaka; Fabio Convenga; C. J.W.P. Timmermans; Fabian Gobbi; Fernando Contreras; L. Valore; A. Streich; A. Streich; Giovanni Consolati; Karen S. Caballero-Mora; Q. Luce; Raul Sarmento; M. Schimassek; M. Schimassek; Esteban Roulet; A. Haungs; J. Pȩkala; Martin Vacula; Virginia Binet; Vladimir Lenok; Niklas Langner; Carlos Escobar; Antonella Castellina; M. R. Hampel; Nataliia Borodai; A. A. Nucita; N. Kunka; Marco Aglietta; M. Zavrtanik; A.C. Cobos Cerutti; J. Rautenberg; R. López; Clara Keiko Oliveira Watanabe; R. Squartini; Josina Schulte; J. Vicha; M. del Río; Florian Lukas Briechle; Maximilian Stadelmaier; Maximilian Stadelmaier; G. De Mauro; J. Kleinfeller; M. Platino; John Matthews; M. Wirtz; S. Petrera; Giovanni Mancarella; Jon Paul Lundquist; Humberto Ibarguen Salazar; Octavian Sima; L. Nožka; Rossella Caruso; G. C. Hill; Carla Taricco; Kevin-Druis Merenda; Juan Pablo Gongora; Antonio Condorelli; Pierre Billoir; Philipp Papenbreer; Lino Miramonti; G. Golup; Carlo Ventura; G. Parente; Denis Stanca; Felix Schlüter; Felix Schlüter; Peter Buchholz; B. Andrada; R. Alves Batista; Toshihiro Fujii; Toshihiro Fujii; H. Martinez; A. Insolia; G. Cataldi; Alan Coleman; Corinne Berat; Cristina Galea; Alina Mihaela Badescu; G. P. Guedes; L. Lu; Orazio Zapparrata; B. Wundheiler; A. Filipčič; Peter L. Biermann; A. Weindl; Maria-Teresa Dova; Marcus Niechciol; E. De Vito; Jan Ebr; Jonathan Biteau; Isabel Goos; Isabel Goos; Jonas Glombitza; Fridtjof Feldbusch; D. D. dos Santos; Jeffrey Brack; V. de Souza; Radomir Smida; H.O. Klages; Jörg R. Hörandel; Ladislav Chytka; A. C. Fauth; M. I. Micheletti; Ioana Caracas; Julien Manshanden; L. Zehrer; W. Rodrigues de Carvalho; Vincenzo Rizi; Martina Bohacova; Zoé Torrès; Thomas Hebbeker; Frank G. Schröder; Frank G. Schröder; Petr Hamal; Alena Bakalova; Günter Sigl; Lukáš Vaclavek; J. Ridky; F. Riehn; Tomáš Fodran; K. Mulrey; Miroslav Pech; Juan Carlos D'Olivo; D. Ravignani; E. Varela; Markus Roth; M. A. Leigui de Oliveira; Claudio Galelli; Antonio Bueno; Marco Giammarchi; M. Palatka; R. Sato; Roberto Mussa; Olivier Deligny; C. Hojvat; Fabrizia Canfora; Sara Martinelli; Sara Martinelli; L. M. Domingues Mendes; David Wittkowski; P.R. Araújo Ferreira; Max Büsken; Max Büsken; Thomas Bretz; S. J. De Jong; M. Unger; Carla Aramo; M. Kleifges; Daniela Mockler; Daniela Mockler; Marcos Cerda; Serguei Vorobiov;doi: 10.1140/epjc/s10052-021-09700-w , 10.48550/arxiv.2109.13400 , 10.18154/rwth-2021-12100 , 10.18154/rwth-2022-00047
handle: https://repository.ubn.ru.nl/handle/2066/239867 , 11588/890384 , 11245.1/e277820a-6074-4fdc-9cd2-9d87842d0efe , 2066/239867 , 2434/1033134 , 10481/71942 , 20.500.12556/RUNG-6965 , 11311/1189557 , 20.500.14017/fb76dc10-e5e8-4ff6-88c2-75af44762dfb , 11697/176134 , 11587/458363 , 20.500.11769/526705 , 2318/1841975 , 2133/23683
doi: 10.1140/epjc/s10052-021-09700-w , 10.48550/arxiv.2109.13400 , 10.18154/rwth-2021-12100 , 10.18154/rwth-2022-00047
handle: https://repository.ubn.ru.nl/handle/2066/239867 , 11588/890384 , 11245.1/e277820a-6074-4fdc-9cd2-9d87842d0efe , 2066/239867 , 2434/1033134 , 10481/71942 , 20.500.12556/RUNG-6965 , 11311/1189557 , 20.500.14017/fb76dc10-e5e8-4ff6-88c2-75af44762dfb , 11697/176134 , 11587/458363 , 20.500.11769/526705 , 2318/1841975 , 2133/23683
AbstractWe present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface detector of the Pierre Auger Observatory that has a spacing of 750 m. An inflection of the spectrum is observed, confirming the presence of the so-called second-knee feature. The spectrum is then combined with that of the 1500 m array to produce a single measurement of the flux, linking this spectral feature with the three additional breaks at the highest energies. The combined spectrum, with an energy scale set calorimetrically via fluorescence telescopes and using a single detector type, results in the most statistically and systematically precise measurement of spectral breaks yet obtained. These measurements are critical for furthering our understanding of the highest energy cosmic rays.
Archivio Istituziona... arrow_drop_down RepHipUNR - Repositorio Hipermedial de la Universidad Nacional de RosarioArticle . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)European Physical Journal C: Particles and FieldsArticle . 2021 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2021License: CC BYData sources: Universiteit van Amsterdam Digital Academic RepositoryRepository of the Czech Academy of SciencesArticle . 2021Data sources: Repository of the Czech Academy of SciencesVrije Universiteit Brussel Research PortalArticle . 2021Data sources: Vrije Universiteit Brussel Research PortalMémoires en Sciences de l'Information et de la CommunicationPreprint . 2021Publikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityPublikationsserver der RWTH Aachen UniversityArticle . 2021Data sources: Publikationsserver der RWTH Aachen UniversityUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2021Data sources: Repository of University of Nova GoricaRepositorio Institucional Universidad de GranadaArticle . 2021License: CC BYData sources: Repositorio Institucional Universidad de GranadaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di Cataniaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1140/epjc/s10052-021-09700-w&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 73 citations 73 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down RepHipUNR - Repositorio Hipermedial de la Universidad Nacional de RosarioArticle . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2021License: CC BYData sources: Bielefeld Academic Search Engine (BASE)European Physical Journal C: Particles and FieldsArticle . 2021 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2021License: CC BYData sources: Universiteit van Amsterdam Digital Academic RepositoryRepository of the Czech Academy of SciencesArticle . 2021Data sources: Repository of the Czech Academy of SciencesVrije Universiteit Brussel Research PortalArticle . 2021Data sources: Vrije Universiteit Brussel Research PortalMémoires en Sciences de l'Information et de la CommunicationPreprint . 2021Publikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityPublikationsserver der RWTH Aachen UniversityArticle . 2021Data sources: Publikationsserver der RWTH Aachen UniversityUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2021Data sources: Repository of University of Nova GoricaRepositorio Institucional Universidad de GranadaArticle . 2021License: CC BYData sources: Repositorio Institucional Universidad de GranadaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di Cataniaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1140/epjc/s10052-021-09700-w&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2024Embargo end date: 01 Jan 2024 FrancePublisher:American Astronomical Society Funded by:ANR | MICRO, ANR | P2IO, ANR | IPSANR| MICRO ,ANR| P2IO ,ANR| IPSSullivan Marafico; Jonathan Biteau; Antonio Condorelli; Olivier Deligny; Johan Bregeon;Abstract The arrival directions of ultrahigh-energy cosmic rays (UHECRs) observed above 4 × 1019 eV provide evidence of localized excesses that are key to identifying their sources. We leverage the 3D matter distribution from optical and infrared surveys as a density model of UHECR sources, which are considered to be transient. Agreement of the sky model with UHECR data imposes constraints on both the emission rate per unit matter and the time spread induced by encountered turbulent magnetic fields. Based on radio measurements of cosmic magnetism, we identify the Local Sheet as the magnetized structure responsible for the kiloyear duration of UHECR bursts for an observer on Earth and find that the turbulence amplitude must be within 0.5–20 nG for a coherence length of 10 kpc. At the same time, the burst-rate density must be above 50 Gpc−3 yr−1 for Local Sheet galaxies to reproduce the UHECR excesses and below 5000 Gpc−3 yr−1 (30,000 Gpc−3 yr−1) for the Milky Way (Local Group galaxies) not to outshine other galaxies. For the transient emissions of protons and nuclei to match the energy spectra of UHECRs, the kinetic energy of the outflows responsible for UHECR acceleration must be below 4 × 1054 erg and above 5 × 1050 erg (2 × 1049 erg) if we consider the Milky Way (or not). The only stellar-sized transients that satisfy both Hillas’ and our criteria are long-duration gamma-ray bursts.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ad5a11&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu2 citations 2 popularity Average influence Average impulse Average Powered by BIP!more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ad5a11&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Journal 2016Embargo end date: 01 Jan 2016 Spain, Netherlands, Italy, Netherlands, Italy, Germany, Italy, Netherlands, Netherlands, Italy, France, Italy, Australia, Germany, Italy, Italy, Australia, Italy, GermanyPublisher:American Physical Society (APS) Funded by:DFG, EC | EPLANET, NSF | Pierre Auger Project +5 projectsDFG ,EC| EPLANET ,NSF| Pierre Auger Project ,MIUR ,EC| AUGER2FUTURE ,ANR| SUPER ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| The Highest Energy Astroparticle PhysicsG. Cataldi; A. Yushkov; Karl-Heinz Kampert; Zbigniew Szadkowski; R. Piegaia; A. Shadkam; S. G. Blaess; F. Suarez; Antonio Bueno; Igor Katkov; R. Sato; Olivier Deligny; M. L. Díaz Castro; Stefano D'Amico; Rossella Caruso; J. A.J. Matthews; Julien Aublin; Julien Aublin; J. Biteau; H.O. Klages; Jörg R. Hörandel; E. J. Quel; Jan Ebr; Jeffrey A. Johnsen; M. Pimenta; A. López Casado; C. Aramo; Francesca Zuccarello; Danielle LaHurd; M. Unger; Rúben Conceição; Stijn Buitink; B. Tome; Brian Fick; Marco Torri; Martin Erdmann; H. Gemmeke; J. Phuntsok; Silvia Mollerach; M. R. Hampel; Esteban Roulet; S. Quinn; J. R. Vázquez; L. A. S. Pereira; D. Nosek; G. Medina-Tanco; N. Krohm; F. Salamida; A. E. Herve; J. R. T. de Mello Neto; G. A. Anastasi; B. Sarkar; Carlos Escobar; J. Debatin; Antonella Castellina; V. M. Theodoro; Nataliia Borodai; Jaime Alvarez-Muñiz; David Walz; Dieter Heck; B. Revenu; A. Dorofeev; A. C. Rovero; M. Kleifges; Markus Lauscher; O. Martínez Bravo; R. A. Vázquez; Marc Weber; A. Di Matteo; J. Stasielak; G. Farrar; L. Ochilo; R.J. Barreira Luz; R.J. Barreira Luz; Xavier Bertou; A. Blanco; A. Blanco; Martina Bohacova; M. J. Cooper; A. Śmiałkowski; Katrin Link; M. Ambrosio; Samo Stanič; I. Naranjo; G. van Aar; Max Malacari; C. Porowski; J. Alvarez Castillo; Norberto Fazzini; Tim Huege; S. J. De Jong; B. Vargas Cárdenas; Carla Bonifazi; I.M. Brancus; B. Wundheiler; A. Filipčič; M. Schauer; J. Neuser; André Schulz; L. Perrone; Pavel Horvath; Andrej Dundovic; Trent D. Grubb; Peter Buchholz; J. W. Cronin; Marcus Niechciol; S. J. Sciutto; Marco Aglietta; Marco Aglietta; N. Kunka; R.C. dos Anjos; D. Martello; J. Hulsman; S. Messina; Tim Niggemann; S. Jansen; Benedikt Zimmermann; A. Fuster; P. Sanchez-Lucas; V. Novotny; Lorenzo Caccianiga; Christine Peters; Thomas Harrison; M. Trini; Ingomar Allekotte; L. Niemietz; M. Zavrtanik; R. López; F. Sánchez; E. Santos; G. Torralba Elipe; Nicolás González; M. Risse; Francesco Strafella; H. Wilczyński; Gualberto Avila; Harald Schieler; L. Molina-Bueno; Heino Falcke; John N. Matthews; Alan Watson; Kai Daumiller; Octavian Fratu; Gaia Silli; Alberto Daniel Supanitsky; P. Ristori; I. A. Minaya; M. Erfani; Johannes Schulz; F. Montanet; A. Lucero; R. Squartini; J. Vicha; F. Canfora; Paula Gina Isar; S. Mathys; Lili Yang; A. Kuotb Awad; Martin Urban; Alexandru Balaceanu; J. J. Masías Meza; P. Abreu; P. Abreu; F. Diogo; J. Ridky; Charles Timmermans; Carlos Hojvat; H. Nožka; C. J. Todero Peixoto; A. G. Mariazzi; R. Gaior; L. Nellen; Philipp Papenbreer; Foteini Oikonomou; R. Legumina; A. G. Chavez; Luis A. Nunez; Peter Mazur; M. Prouza; L. Valore; Darko Veberič; Mihai Niculescu-Oglinzanu; M. Plum; David Wittkowski; E.M. Holt; Corbin Covault; Florian Lukas Briechle; L. Lopes; S. Querchfeld; Paul M. Mantsch; Hernán Asorey; Hernán Asorey; Lukas Middendorf; A. Parra; Denise Boncioli; P. Pieroni; E. Kemp; Enrique Zas; R. Ramos-Pollan; R. Sarmento;We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles range from $10^{-19}$ (cm$^{2}$ sr s)$^{-1}$ for a Lorentz factor $��=10^9$ to $2.5 \times10^{-21}$ (cm$^{2}$ sr s)$^{-1}$ for $��=10^{12}$. These results - the first obtained with a UHECR detector - improve previously published limits by up to an order of magnitude. Published version. Corrected title. Added journal reference and DOI. Added Report Number
Archivio Istituziona... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2016Data sources: Bielefeld Academic Search Engine (BASE)https://link.aps.org/accepted/...ArticleLicense: publisher-specific, author manuscriptData sources: UnpayWallRecolector de Ciencia Abierta, RECOLECTAArticle . 2016Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2016 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2016Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2016Data sources: INRIA a CCSD electronic archive serverhttps://doi.org/10.1103/physre...Article . 2016 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://hdl.handle.net/11370/e...Article . 2016Data sources: DANS (Data Archiving and Networked Services)https://dx.doi.org/10.48550/ar...Article . 2016License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.94.082002&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 15 citations 15 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2016Data sources: Bielefeld Academic Search Engine (BASE)https://link.aps.org/accepted/...ArticleLicense: publisher-specific, author manuscriptData sources: UnpayWallRecolector de Ciencia Abierta, RECOLECTAArticle . 2016Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2016 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2016Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2016Data sources: INRIA a CCSD electronic archive serverhttps://doi.org/10.1103/physre...Article . 2016 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://hdl.handle.net/11370/e...Article . 2016Data sources: DANS (Data Archiving and Networked Services)https://dx.doi.org/10.48550/ar...Article . 2016License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2016Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.94.082002&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Preprint , Book 2022Embargo end date: 01 Jan 2022 Germany, FrancePublisher:American Astronomical Society Funded by:ANR | MICRO, ANR | P2IO, ANR | IPSANR| MICRO ,ANR| P2IO ,ANR| IPSQuentin Luce; Sullivan Marafico; Jonathan Biteau; Antonio Condorelli; Olivier Deligny;Abstract Interactions of ultra-high energy cosmic rays (UHECRs) accelerated in specific astrophysical environments have been shown to shape the energy production rate of nuclei differently from that of the secondary neutrons escaping from the confinement zone. Here, we aim at testing a generic scenario of in-source interactions through phenomenological modeling of the flux and composition of UHECRs. We fit a model in which nucleons and nuclei follow different particle energy distributions to the all-particle energy spectrum and proton spectrum below the ankle energy and distributions of maximum shower depths above this energy, as inferred at the Pierre Auger Observatory. We obtain that the data can be reproduced using a spatial distribution of sources that follows the density of extragalactic matter on both local and large scales, providing hence a realistic set of constraints for the emission mechanisms in cosmic accelerators, for their energetics, and for the abundances of elements at escape from their environments. While the quasi monoelemental increase of the cosmic-ray mass number observed on Earth from ≃2 EeV up to the highest energies calls for nuclei accelerated with a hard spectral index, the inferred flux of protons down to ≃0.6 EeV is shown to require for this population a spectral index significantly softer than that generally obtained up to now. We demonstrate that modeling UHECR data across the ankle substantiates the conjecture of in-source interactions in a robust statistical framework, although pushing the mechanism to the extreme.
KITopen (Karlsruhe I... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Book . 2024License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2022License: CC BYData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ac81cc&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 11 citations 11 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert KITopen (Karlsruhe I... arrow_drop_down KITopen (Karlsruhe Institute of Technologie)Article . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Book . 2024License: CC BYData sources: Bielefeld Academic Search Engine (BASE)KITopen (Karlsruhe Institute of Technologie)Article . 2022License: CC BYData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ac81cc&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu