The cosmic-ray spectrum in the PeV to EeV energy range
Fuente:
arXiv
Guardado en:
| Autores principales: | Kang, Donghwa, Haungs, Andreas |
|---|---|
| Formato: | Preprint |
| Publicado: |
2025
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Cosmic-Ray Physics in the PeV to EeV Energy Range with the IceCube-Gen2 Surface Array (ICRC 2025)
por: Schröder, Frank G.
Publicado: (2025)
por: Schröder, Frank G.
Publicado: (2025)
Irregularity in spectrum of the primary cosmic rays mass composition at an energy of ~ 10 PeV
por: Pyatovsky, S. E.
Publicado: (2024)
por: Pyatovsky, S. E.
Publicado: (2024)
Recent measurements of the spectrum and composition of cosmic rays between 10 TeV and 1 EeV from EAS experiments
por: Arteaga-Velázquez, J. C.
Publicado: (2025)
por: Arteaga-Velázquez, J. C.
Publicado: (2025)
What do we know about cosmic rays with energies above 5 EeV?
por: Biteau, Jonathan
Publicado: (2024)
por: Biteau, Jonathan
Publicado: (2024)
Measurement of the cosmic-ray energy spectrum above 2.5 EeV using 19 years of operation of the Pierre Auger Observatory
por: Ravignani, Diego
Publicado: (2025)
por: Ravignani, Diego
Publicado: (2025)
Combined fit above 0.1 EeV to the cosmic-ray spectrum and composition measured with the Pierre Auger Observatory
por: Roulet, Esteban
Publicado: (2025)
por: Roulet, Esteban
Publicado: (2025)
Microquasar remnants as reservoirs of PeV cosmic rays
por: Abaroa, Leandro, et al.
Publicado: (2026)
por: Abaroa, Leandro, et al.
Publicado: (2026)
The puzzle of composition of cosmic rays with energies (2-12.5) EeV according to muon detectors data of the Yakutsk EAS array
por: Glushkov, A. V., et al.
Publicado: (2026)
por: Glushkov, A. V., et al.
Publicado: (2026)
Imprints of PeV cosmic-ray sources on the diffuse gamma-ray emission
por: Kaci, Samy, et al.
Publicado: (2024)
por: Kaci, Samy, et al.
Publicado: (2024)
The flavor composition of ultra-high-energy cosmic neutrinos: measurement forecasts for in-ice radio-based EeV neutrino telescopes
por: Coleman, Alan, et al.
Publicado: (2024)
por: Coleman, Alan, et al.
Publicado: (2024)
Evidence of cosmic-ray acceleration up to sub-PeV energies in the supernova remnant IC 443
por: Cao, Zhen, et al.
Publicado: (2025)
por: Cao, Zhen, et al.
Publicado: (2025)
Emergence of a neutrino flux above 5 PeV and implications for ultrahigh energy cosmic rays
por: Muzio, Marco S., et al.
Publicado: (2025)
por: Muzio, Marco S., et al.
Publicado: (2025)
Blazars Jets and prospects for TeV-PeV neutrinos & gamma-rays through cosmic-ray interactions
por: Sasse, Rodrigo, et al.
Publicado: (2025)
por: Sasse, Rodrigo, et al.
Publicado: (2025)
XMM-Newton observations of the extragalactic microquasar S26 and their implications for PeV cosmic rays
por: Abaroa, L., et al.
Publicado: (2024)
por: Abaroa, L., et al.
Publicado: (2024)
HESS J1745$-$290 spectrum explained by a transition in the diffusion regime of PeV cosmic rays in the Sgr A* accretion flow
por: Muena, Claudio, et al.
Publicado: (2024)
por: Muena, Claudio, et al.
Publicado: (2024)
The cosmic-ray sea explains the Galactic $γ$-ray and $ν$ diffuse emissions from GeV to PeV
por: Luque, Pedro De La Torre, et al.
Publicado: (2025)
por: Luque, Pedro De La Torre, et al.
Publicado: (2025)
The cosmic-ray sea explains the diffuse Galactic gamma-ray and neutrino emission from GeV to PeV
por: Luque, Pedro De La Torre, et al.
Publicado: (2025)
por: Luque, Pedro De La Torre, et al.
Publicado: (2025)
Measurement of the cosmic p+He energy spectrum from 50 GeV to 0.5 PeV with the DAMPE space mission
por: DAMPE Collaboration, et al.
Publicado: (2023)
por: DAMPE Collaboration, et al.
Publicado: (2023)
PeV proton acceleration in Gamma-ray Binaries
por: Bykov, A. M., et al.
Publicado: (2024)
por: Bykov, A. M., et al.
Publicado: (2024)
Searching for EeV photons with Telescope Array Surface Detector and neural networks
por: Telescope Array Collaboration, et al.
Publicado: (2025)
por: Telescope Array Collaboration, et al.
Publicado: (2025)
A Unified Framework for 10 TeV to EeV Diffuse Neutrino Sky and KM3-230213A
por: Yu, Shiqi, et al.
Publicado: (2026)
por: Yu, Shiqi, et al.
Publicado: (2026)
Uncertainties in astrophysical gamma-ray and neutrino fluxes from proton-proton cross-sections in the GeV to PeV range
por: Dörner, Julien, et al.
Publicado: (2025)
por: Dörner, Julien, et al.
Publicado: (2025)
TeV to PeV neutrinos from AGN coronae
por: Sotirov, Simon
Publicado: (2024)
por: Sotirov, Simon
Publicado: (2024)
Cosmic ray contributions from rapidly rotating stellar mass black holes: Cosmic Ray GeV to EeV proton and anti-proton sources
por: Allen, M. L., et al.
Publicado: (2024)
por: Allen, M. L., et al.
Publicado: (2024)
Ultra-high-energy $γ$-ray imprints from PeV particles accelerated by supernova remnants
por: Cao, Zhen, et al.
Publicado: (2026)
por: Cao, Zhen, et al.
Publicado: (2026)
Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies
por: Yang, Qi-Rui, et al.
Publicado: (2026)
por: Yang, Qi-Rui, et al.
Publicado: (2026)
A discussion on the origin of the sub-PeV Galactic gamma-ray emission
por: Kato, S., et al.
Publicado: (2025)
por: Kato, S., et al.
Publicado: (2025)
Design and Initial Performance of the Askaryan Radio Array Prototype EeV Neutrino Detector at the South Pole
por: Allison, P., et al.
Publicado: (2011)
por: Allison, P., et al.
Publicado: (2011)
Machine-learning correction for the calorimeter saturation of cosmic-ray ions with the Dark Matter Particle Explorer: towards the PeV scale
por: Serpolla, Andrea, et al.
Publicado: (2025)
por: Serpolla, Andrea, et al.
Publicado: (2025)
Modeling gamma-ray signatures of particle acceleration in stellar clusters from GeV to PeV
por: Inventar, A., et al.
Publicado: (2025)
por: Inventar, A., et al.
Publicado: (2025)
The Trinity-One PeV-Neutrino Telescope
por: O., David A. Raudales, et al.
Publicado: (2025)
por: O., David A. Raudales, et al.
Publicado: (2025)
Evidence for particle acceleration approaching PeV energies in the W51 complex
por: The LHAASO Collaboration, et al.
Publicado: (2024)
por: The LHAASO Collaboration, et al.
Publicado: (2024)
Angular Power Spectrum of TeV-PeV Cosmic Ray Anisotropies
por: Bian, Wenyi, et al.
Publicado: (2024)
por: Bian, Wenyi, et al.
Publicado: (2024)
Improved measurements of the TeV-PeV extragalactic neutrino spectrum from joint analyses of IceCube tracks and cascades
por: Abbasi, R., et al.
Publicado: (2025)
por: Abbasi, R., et al.
Publicado: (2025)
Particle acceleration to PeV energies in Pulsar Wind Nebula: a two zone model
por: Mahanta, Gunindra Krishna, et al.
Publicado: (2026)
por: Mahanta, Gunindra Krishna, et al.
Publicado: (2026)
The results of the development of the SPHERE-3 detector for studying the PCR mass composition in the 1-1000 PeV energy range. The status of 2025
por: Chernov, D. V., et al.
Publicado: (2025)
por: Chernov, D. V., et al.
Publicado: (2025)
Status of the Trinity PeV Neutrino Observatory
por: Stepanoff, S., et al.
Publicado: (2025)
por: Stepanoff, S., et al.
Publicado: (2025)
Optimizing HERON for 100 PeV Neutrino Detection
por: Zeolla, Andrew, et al.
Publicado: (2025)
por: Zeolla, Andrew, et al.
Publicado: (2025)
Towards the Composition of sub-PeV Cosmic Rays at IceCube
por: Saffer, Julian
Publicado: (2025)
por: Saffer, Julian
Publicado: (2025)
Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory
por: The Pierre Auger Collaboration, et al.
Publicado: (2025)
por: The Pierre Auger Collaboration, et al.
Publicado: (2025)
Ejemplares similares
-
Cosmic-Ray Physics in the PeV to EeV Energy Range with the IceCube-Gen2 Surface Array (ICRC 2025)
por: Schröder, Frank G.
Publicado: (2025) -
Irregularity in spectrum of the primary cosmic rays mass composition at an energy of ~ 10 PeV
por: Pyatovsky, S. E.
Publicado: (2024) -
Recent measurements of the spectrum and composition of cosmic rays between 10 TeV and 1 EeV from EAS experiments
por: Arteaga-Velázquez, J. C.
Publicado: (2025) -
What do we know about cosmic rays with energies above 5 EeV?
por: Biteau, Jonathan
Publicado: (2024) -
Measurement of the cosmic-ray energy spectrum above 2.5 EeV using 19 years of operation of the Pierre Auger Observatory
por: Ravignani, Diego
Publicado: (2025)