ReP USP - Resultado da busca

Artigo de periodico
Towards understanding the origin of cosmic-ray positrons (2019)
Aguilar, M.; Bueno, E. F.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Towards understanding the origin of cosmic-ray positrons. Physical Review Letters, v. 122, n. 4, p. 041102-1-041102-9, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.122.041102. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., & Vecchi, M. (2019). Towards understanding the origin of cosmic-ray positrons. Physical Review Letters, 122( 4), 041102-1-041102-9. doi:10.1103/PhysRevLett.122.041102
NLM
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray positrons [Internet]. Physical Review Letters. 2019 ; 122( 4): 041102-1-041102-9.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.122.041102
Vancouver
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray positrons [Internet]. Physical Review Letters. 2019 ; 122( 4): 041102-1-041102-9.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.122.041102
Artigo de periodico
Towards understanding the origin of cosmic-ray electrons (2019)
Aguilar, M.; Bueno, E. F.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Towards understanding the origin of cosmic-ray electrons. Physical Review Letters, v. 122, n. 10, p. 101101-1-101101-9, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.122.101101. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., & Vecchi, M. (2019). Towards understanding the origin of cosmic-ray electrons. Physical Review Letters, 122( 10), 101101-1-101101-9. doi:10.1103/PhysRevLett.122.101101
NLM
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray electrons [Internet]. Physical Review Letters. 2019 ; 122( 10): 101101-1-101101-9.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.122.101101
Vancouver
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray electrons [Internet]. Physical Review Letters. 2019 ; 122( 10): 101101-1-101101-9.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.122.101101
Artigo de periodico
Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. et al. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051101-1-051101-7, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051101. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051101-1-051101-7. doi:10.1103/PhysRevLett.121.051101
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051101-1-051101-7.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051101
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051101-1-051101-7.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051101
Artigo de periodico
Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. et al. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051102-1-051102-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051102. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051102-1-051102-8. doi:10.1103/PhysRevLett.121.051102
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051102-1-051102-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051102
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051102-1-051102-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051102
Artigo de periodico
Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. et al. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051103-1-051103-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051103. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051103-1-051103-8. doi:10.1103/PhysRevLett.121.051103
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051103-1-051103-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051103
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051103-1-051103-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051103
Artigo de periodico
Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. et al. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 120, n. Ja 2018, p. 021101-1-021101-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.120.021101. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station. Physical Review Letters, 120( Ja 2018), 021101-1-021101-8. doi:10.1103/PhysRevLett.120.021101
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 120( Ja 2018): 021101-1-021101-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.120.021101
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 120( Ja 2018): 021101-1-021101-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.120.021101
Trabalho de evento-anais periodico
What do Galactic electrons and positrons tell us about dark matter? (2017)
Boudaud, M.; Bueno, E. F.; Caroff, S.; Putze, A.; Genolini, Y.; Lavalle, J.; Poireau, V.; Poulin, V.; Rosier, S.; Salati, P.; Vecchi, Manuela
Source: Proceedings of Science. Conference titles: International Cosmic Ray Conference - ICRC. Unidade: IFSC
Subjects: RAIOS CÓSMICOS, FÍSICA DE PARTÍCULAS
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ABNT
BOUDAUD, M. et al. What do Galactic electrons and positrons tell us about dark matter?. Proceedings of Science. Trieste: Scuola Internazionale Superiore di Studi Avanzati - SISSA. Disponível em: https://doi.org/10.22323/1.301.0915. Acesso em: 01 maio 2024. , 2017
APA
Boudaud, M., Bueno, E. F., Caroff, S., Putze, A., Genolini, Y., Lavalle, J., et al. (2017). What do Galactic electrons and positrons tell us about dark matter? Proceedings of Science. Trieste: Scuola Internazionale Superiore di Studi Avanzati - SISSA. doi:10.22323/1.301.0915
NLM
Boudaud M, Bueno EF, Caroff S, Putze A, Genolini Y, Lavalle J, Poireau V, Poulin V, Rosier S, Salati P, Vecchi M. What do Galactic electrons and positrons tell us about dark matter? [Internet]. Proceedings of Science. 2017 ; 301 915-1-915-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.22323/1.301.0915
Vancouver
Boudaud M, Bueno EF, Caroff S, Putze A, Genolini Y, Lavalle J, Poireau V, Poulin V, Rosier S, Salati P, Vecchi M. What do Galactic electrons and positrons tell us about dark matter? [Internet]. Proceedings of Science. 2017 ; 301 915-1-915-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.22323/1.301.0915
Artigo de periodico
Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station (2017)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. et al. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 119, n. 25, p. 251101-1-241101-8, 2017Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.119.251101. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2017). Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station. Physical Review Letters, 119( 25), 251101-1-241101-8. doi:10.1103/PhysRevLett.119.251101
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2017 ; 119( 25): 251101-1-241101-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.119.251101
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2017 ; 119( 25): 251101-1-241101-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.119.251101
Artigo de periodico
The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements (2017)
Boudaud, M.; Bueno, E. F.; Caroff, S.; Genolini, Y.; Poulin, V.; Poireau, V.; Putze, A.; Rosier, S.; Salati, P.; Vecchi, Manuela
Source: Astronomy and Astrophysics. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
BOUDAUD, M. et al. The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements. Astronomy and Astrophysics, v. 605, p. A17-1-A17-16, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201630321. Acesso em: 01 maio 2024.
APA
Boudaud, M., Bueno, E. F., Caroff, S., Genolini, Y., Poulin, V., Poireau, V., et al. (2017). The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements. Astronomy and Astrophysics, 605, A17-1-A17-16. doi:10.1051/0004-6361/201630321
NLM
Boudaud M, Bueno EF, Caroff S, Genolini Y, Poulin V, Poireau V, Putze A, Rosier S, Salati P, Vecchi M. The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements [Internet]. Astronomy and Astrophysics. 2017 ; 605 A17-1-A17-16.[citado 2024 maio 01 ] Available from: https://doi.org/10.1051/0004-6361/201630321
Vancouver
Boudaud M, Bueno EF, Caroff S, Genolini Y, Poulin V, Poireau V, Putze A, Rosier S, Salati P, Vecchi M. The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements [Internet]. Astronomy and Astrophysics. 2017 ; 605 A17-1-A17-16.[citado 2024 maio 01 ] Available from: https://doi.org/10.1051/0004-6361/201630321
Trabalho de evento-resumo
Effect of the primary cosmic ray flux on the secondary positron flux (2016)
Bueno, E. F.; Vecchi, Manuela; Caroff, S.; Boudad, M.
Source: Livro de Resumos. Conference titles: Semana Integrada do Instituto de Física de São Carlos - SIFSC. Unidade: IFSC
Subjects: RAIOS CÓSMICOS, PARTÍCULAS (FÍSICA NUCLEAR)
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ABNT
BUENO, E. F. et al. Effect of the primary cosmic ray flux on the secondary positron flux. 2016, Anais.. São Carlos: Universidade de São Paulo - USP, Instituto de Física de São Carlos - IFSC, 2016. Disponível em: http://sifsc.ifsc.usp.br/2016/livro_de_resumos_2016.pdf. Acesso em: 01 maio 2024.
APA
Bueno, E. F., Vecchi, M., Caroff, S., & Boudad, M. (2016). Effect of the primary cosmic ray flux on the secondary positron flux. In Livro de Resumos. São Carlos: Universidade de São Paulo - USP, Instituto de Física de São Carlos - IFSC. Recuperado de http://sifsc.ifsc.usp.br/2016/livro_de_resumos_2016.pdf
NLM
Bueno EF, Vecchi M, Caroff S, Boudad M. Effect of the primary cosmic ray flux on the secondary positron flux [Internet]. Livro de Resumos. 2016 ;[citado 2024 maio 01 ] Available from: http://sifsc.ifsc.usp.br/2016/livro_de_resumos_2016.pdf
Vancouver
Bueno EF, Vecchi M, Caroff S, Boudad M. Effect of the primary cosmic ray flux on the secondary positron flux [Internet]. Livro de Resumos. 2016 ;[citado 2024 maio 01 ] Available from: http://sifsc.ifsc.usp.br/2016/livro_de_resumos_2016.pdf
Artigo de periodico
Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station (2016)
Aguilar, M.; Bueno, E. F.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station. Physical Review Letters, v. 117, n. 9, p. 091103-1-091103-10, 2016Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.117.091103. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., & Vecchi, M. (2016). Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station. Physical Review Letters, 117( 9), 091103-1-091103-10. doi:10.1103/PhysRevLett.117.091103
NLM
Aguilar M, Bueno EF, Vecchi M. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station [Internet]. Physical Review Letters. 2016 ; 117( 9): 091103-1-091103-10.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.117.091103
Vancouver
Aguilar M, Bueno EF, Vecchi M. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station [Internet]. Physical Review Letters. 2016 ; 117( 9): 091103-1-091103-10.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.117.091103
Artigo de periodico
Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station (2016)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. et al. Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 117, n. 23, p. 231102-1-231102-8, 2016Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.117.231102. Acesso em: 01 maio 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2016). Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 117( 23), 231102-1-231102-8. doi:10.1103/PhysRevLett.117.231102
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2016 ; 117( 23): 231102-1-231102-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.117.231102
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2016 ; 117( 23): 231102-1-231102-8.[citado 2024 maio 01 ] Available from: https://doi.org/10.1103/PhysRevLett.117.231102

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