Investigating hadronic interactions at ultra-high energies with the pierre auger observatory (2022)
- Authors:
- USP affiliated authors: SANTOS, EDIVALDO MOURA - IF ; ARMAND, JOHNNIER PÉREZ - IF
- Unidade: IF
- Subjects: LHC; RAIOS CÓSMICOS
- Language: Inglês
- Imprenta:
-
ABNT
GOOS, Isabel e ARMAND, Johnnier Perez e SANTOS, Edivaldo Moura. Investigating hadronic interactions at ultra-high energies with the pierre auger observatory. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/2206.10938.pdf. Acesso em: 01 maio 2024. , 2022 -
APA
Goos, I., Armand, J. P., & Santos, E. M. (2022). Investigating hadronic interactions at ultra-high energies with the pierre auger observatory. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/2206.10938.pdf -
NLM
Goos I, Armand JP, Santos EM. Investigating hadronic interactions at ultra-high energies with the pierre auger observatory [Internet]. 2022 ;[citado 2024 maio 01 ] Available from: https://arxiv.org/pdf/2206.10938.pdf -
Vancouver
Goos I, Armand JP, Santos EM. Investigating hadronic interactions at ultra-high energies with the pierre auger observatory [Internet]. 2022 ;[citado 2024 maio 01 ] Available from: https://arxiv.org/pdf/2206.10938.pdf - Cosmological implications of photon-flux upper limits at ultra-high energies in scenarios of planckian-interacting massive particles for dark matter
- Search for photons above '10 POT. 19' eV with the surface detector of the Pierre Auger Observatory
- Search for spatial correlations of neutrinos with ultra-high-energy cosmic rays
- Searches for ultra-high-energy photons at the Pierre Auger Observatory
- Limits to gauge coupling in the dark sector set by the non-observation of instantoninduced decay of super-heavy dark matter in the pierre auger observatory data
- Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory
- A search for photons with energies above 2×'10 POT. 17' eV using hybrid data from the low-energy extensions of the pierre auger observatory
- Arrival directions of cosmic rays above 32 EeV from phase one of the pierre auger observatory
- A catalog of the highest-energy cosmic rays recorded during phase I of operation of the Pierre Auger Observatory
- Anisotropias no fluxo de raios cósmicos de ultra altas energias
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