Filtros : "MATÉRIA ESCURA" "Financiamento MCTI" Removido: "Indexado no : Scielo" Limpar

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  • Source: Boletim da Sociedade Astronômica Brasileira. Unidade: IFSC

    Subjects: GALÁXIAS, MATÉRIA ESCURA, RAIOS GAMA

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    • ABNT

      MAMPRIM, Júlia Gouvea e SOUZA, Vitor de. Optimizing the indirect search for dark matter with the CTA. Boletim da Sociedade Astronômica Brasileira, v. 35, n. 1, p. 129-132, 2024Tradução . . Disponível em: https://sab-astro.org.br/wp-content/uploads/2024/05/JuliaMamprim.pdf. Acesso em: 24 jul. 2024.
    • APA

      Mamprim, J. G., & Souza, V. de. (2024). Optimizing the indirect search for dark matter with the CTA. Boletim da Sociedade Astronômica Brasileira, 35( 1), 129-132. Recuperado de https://sab-astro.org.br/wp-content/uploads/2024/05/JuliaMamprim.pdf
    • NLM

      Mamprim JG, Souza V de. Optimizing the indirect search for dark matter with the CTA [Internet]. Boletim da Sociedade Astronômica Brasileira. 2024 ; 35( 1): 129-132.[citado 2024 jul. 24 ] Available from: https://sab-astro.org.br/wp-content/uploads/2024/05/JuliaMamprim.pdf
    • Vancouver

      Mamprim JG, Souza V de. Optimizing the indirect search for dark matter with the CTA [Internet]. Boletim da Sociedade Astronômica Brasileira. 2024 ; 35( 1): 129-132.[citado 2024 jul. 24 ] Available from: https://sab-astro.org.br/wp-content/uploads/2024/05/JuliaMamprim.pdf
  • Source: Physical Review Letters. Unidades: EEL, IFSC, IF

    Subjects: MATÉRIA ESCURA, ASTROFÍSICA, OBSERVATÓRIOS

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      HALIM, Adila Binti Abdul et al. Demonstrating agreement between radio and fluorescence measurements of the depth of maximum of extensive air showers at the Pierre Auger Observatory. Physical Review Letters, v. 132, n. Ja 2024, p. 021001-1-021001-9, 2024Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.132.021001. Acesso em: 24 jul. 2024.
    • APA

      Halim, A. B. A., Catalani, F., Souza, V. de, Oliveira, C. de, Armand, J. P., Santos, E. M., & Peixoto, C. J. T. (2024). Demonstrating agreement between radio and fluorescence measurements of the depth of maximum of extensive air showers at the Pierre Auger Observatory. Physical Review Letters, 132( Ja 2024), 021001-1-021001-9. doi:10.1103/PhysRevLett.132.021001
    • NLM

      Halim ABA, Catalani F, Souza V de, Oliveira C de, Armand JP, Santos EM, Peixoto CJT. Demonstrating agreement between radio and fluorescence measurements of the depth of maximum of extensive air showers at the Pierre Auger Observatory [Internet]. Physical Review Letters. 2024 ; 132( Ja 2024): 021001-1-021001-9.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1103/PhysRevLett.132.021001
    • Vancouver

      Halim ABA, Catalani F, Souza V de, Oliveira C de, Armand JP, Santos EM, Peixoto CJT. Demonstrating agreement between radio and fluorescence measurements of the depth of maximum of extensive air showers at the Pierre Auger Observatory [Internet]. Physical Review Letters. 2024 ; 132( Ja 2024): 021001-1-021001-9.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1103/PhysRevLett.132.021001
  • Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC

    Subjects: RAIOS GAMA, MATÉRIA ESCURA, ASTROFÍSICA

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    • ABNT

      REIS, Igor et al. Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories. Journal of Cosmology and Astroparticle Physics, v. 2024, n. 7, p. 012-1-012-23, 2024Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2024/07/012. Acesso em: 24 jul. 2024.
    • APA

      Reis, I., Moulin, E., Viana, A., & Gonçalves, V. P. (2024). Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories. Journal of Cosmology and Astroparticle Physics, 2024( 7), 012-1-012-23. doi:10.1088/1475-7516/2024/07/012
    • NLM

      Reis I, Moulin E, Viana A, Gonçalves VP. Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( 7): 012-1-012-23.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/012
    • Vancouver

      Reis I, Moulin E, Viana A, Gonçalves VP. Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( 7): 012-1-012-23.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/012
  • Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC

    Subjects: TELESCÓPIOS, GALÁXIAS, MATÉRIA ESCURA, RAIOS GAMA, ASTROFÍSICA

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    • ABNT

      KHERLAKIAN, Maria Carolina e VIANA, Aion e SOUZA, Vitor de. Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes. Journal of Cosmology and Astroparticle Physics, v. 2023, p. 025-1-025-14, 2023Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2023/03/025. Acesso em: 24 jul. 2024.
    • APA

      Kherlakian, M. C., Viana, A., & Souza, V. de. (2023). Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes. Journal of Cosmology and Astroparticle Physics, 2023, 025-1-025-14. doi:10.1088/1475-7516/2023/03/025
    • NLM

      Kherlakian MC, Viana A, Souza V de. Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes [Internet]. Journal of Cosmology and Astroparticle Physics. 2023 ; 2023 025-1-025-14.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/1475-7516/2023/03/025
    • Vancouver

      Kherlakian MC, Viana A, Souza V de. Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes [Internet]. Journal of Cosmology and Astroparticle Physics. 2023 ; 2023 025-1-025-14.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/1475-7516/2023/03/025
  • Source: Physical Review Letters. Unidades: EEL, IFSC, IF

    Subjects: MATÉRIA ESCURA, ASTROFÍSICA, OBSERVATÓRIOS

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      ABREU, Pedro T. et al. Limits to Gauge coupling in the dark sector set by the nonobservation of instanton-induced decay of super-heavy dark matter in the Pierre Auger Observatory data. Physical Review Letters, v. 130, n. 6, p. 061001-1-061001-9, 2023Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.130.061001. Acesso em: 24 jul. 2024.
    • APA

      Abreu, P. T., Catalani, F., Souza, V. de, Oliveira, C. de, Armand, J. P., Santos, E. M., & Peixoto, C. J. T. (2023). Limits to Gauge coupling in the dark sector set by the nonobservation of instanton-induced decay of super-heavy dark matter in the Pierre Auger Observatory data. Physical Review Letters, 130( 6), 061001-1-061001-9. doi:10.1103/PhysRevLett.130.061001
    • NLM

      Abreu PT, Catalani F, Souza V de, Oliveira C de, Armand JP, Santos EM, Peixoto CJT. Limits to Gauge coupling in the dark sector set by the nonobservation of instanton-induced decay of super-heavy dark matter in the Pierre Auger Observatory data [Internet]. Physical Review Letters. 2023 ; 130( 6): 061001-1-061001-9.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1103/PhysRevLett.130.061001
    • Vancouver

      Abreu PT, Catalani F, Souza V de, Oliveira C de, Armand JP, Santos EM, Peixoto CJT. Limits to Gauge coupling in the dark sector set by the nonobservation of instanton-induced decay of super-heavy dark matter in the Pierre Auger Observatory data [Internet]. Physical Review Letters. 2023 ; 130( 6): 061001-1-061001-9.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1103/PhysRevLett.130.061001

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