Filtros : "SANTOS, EDIVALDO MOURA" "Financiamento CNPq" Removido: "IFSC" Limpar

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  • Unidade: IF

    Subjects: COSMOLOGIA, MATÉRIA ESCURA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      ACERBI, F et al. Flow and thermal modelling of the argon volume in the DarkSide-20k TPC. 2025Tradução . . Disponível em: https://doi.org/10.1088/1748-0221/20/06/P06046. Acesso em: 06 nov. 2025.
    • APA

      Acerbi, F., Albuquerque, I. F., Ave, M., Costa, B. S., Dias, L. K., Kemmerich, N., et al. (2025). Flow and thermal modelling of the argon volume in the DarkSide-20k TPC. doi:https://doi.org/10.1088/1748-0221/20/06/P06046
    • NLM

      Acerbi F, Albuquerque IF, Ave M, Costa BS, Dias LK, Kemmerich N, Pérez R, Santos EM. Flow and thermal modelling of the argon volume in the DarkSide-20k TPC [Internet]. 2025 ;[citado 2025 nov. 06 ] Available from: https://doi.org/10.1088/1748-0221/20/06/P06046
    • Vancouver

      Acerbi F, Albuquerque IF, Ave M, Costa BS, Dias LK, Kemmerich N, Pérez R, Santos EM. Flow and thermal modelling of the argon volume in the DarkSide-20k TPC [Internet]. 2025 ;[citado 2025 nov. 06 ] Available from: https://doi.org/10.1088/1748-0221/20/06/P06046
  • Source: Journal of Cosmology and Astroparticle Physics. Unidade: IF

    Assunto: MÉTODO DE MONTE CARLO

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    • ABNT

      XAVIER, Matheus Genaro Dantas et al. Simultaneously unveiling the EBL and intrinsic spectral parameters of gamma-ray sources with Hamiltonian Monte Carlo. Journal of Cosmology and Astroparticle Physics, 2024Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2024/03/020. Acesso em: 06 nov. 2025.
    • APA

      Xavier, M. G. D., Pereira, L. A. S., Pimentel, D. R. de M., & Santos, E. M. (2024). Simultaneously unveiling the EBL and intrinsic spectral parameters of gamma-ray sources with Hamiltonian Monte Carlo. Journal of Cosmology and Astroparticle Physics. doi:10.1088/1475-7516/2024/03/020
    • NLM

      Xavier MGD, Pereira LAS, Pimentel DR de M, Santos EM. Simultaneously unveiling the EBL and intrinsic spectral parameters of gamma-ray sources with Hamiltonian Monte Carlo [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ;[citado 2025 nov. 06 ] Available from: https://doi.org/10.1088/1475-7516/2024/03/020
    • Vancouver

      Xavier MGD, Pereira LAS, Pimentel DR de M, Santos EM. Simultaneously unveiling the EBL and intrinsic spectral parameters of gamma-ray sources with Hamiltonian Monte Carlo [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ;[citado 2025 nov. 06 ] Available from: https://doi.org/10.1088/1475-7516/2024/03/020
  • Unidades: IF, EEL

    Assunto: RAIOS CÓSMICOS

    Acesso à fonteHow to cite
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    • ABNT

      HALIM, A Abdul et al. Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/2305.16693.pdf. Acesso em: 06 nov. 2025. , 2023
    • APA

      Halim, A. A., Armand, J. P., Santos, E. M., Catalani, F., & Peixoto, C. J. T. (2023). Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/2305.16693.pdf
    • NLM

      Halim AA, Armand JP, Santos EM, Catalani F, Peixoto CJT. Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory [Internet]. 2023 ;[citado 2025 nov. 06 ] Available from: https://arxiv.org/pdf/2305.16693.pdf
    • Vancouver

      Halim AA, Armand JP, Santos EM, Catalani F, Peixoto CJT. Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory [Internet]. 2023 ;[citado 2025 nov. 06 ] Available from: https://arxiv.org/pdf/2305.16693.pdf

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