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)
- Authors:
- Autor USP: VECCHI, MANUELA - IFSC
- Unidade: IFSC
- DOI: 10.1103/PhysRevLett.117.091103
- Subjects: FÍSICA DE ALTA ENERGIA; ENERGIA; RAIOS CÓSMICOS; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Publisher place: College Park
- Date published: 2016
- Source:
- Título do periódico: Physical Review Letters
- ISSN: 0031-9007
- Volume/Número/Paginação/Ano: v. 117, n. 9, p. 091103-1-091103-10, Aug. 2016
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: hybrid
- Licença: cc-by
-
ABNT
AGUILAR, M.; BUENO, E. F.; 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, College Park, v. 117, n. 9, p. 091103-1-091103-10, 2016. Disponível em: < http://dx.doi.org/10.1103/PhysRevLett.117.091103 > DOI: 10.1103/PhysRevLett.117.091103. -
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.Available from: http://dx.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.Available from: http://dx.doi.org/10.1103/PhysRevLett.117.091103 - Cosmic ray positrons: constraints on propagation parameters and dark matter searches in view of AMS-02 Data
- Precise measurements of the cosmic ray uxes with the AMS-02 experiment and implications for dark matter search
- Precision measurement of the positron fraction and the combined electron and positron flux in primary cosmic rays with the alpha magnetic spectrometer on the international space station
- Precision measurement of the monthly cosmic ray fluxes with the alpha magnetic spectrometer on the ISS
- Towards understanding the origin of cosmic-ray positrons
- Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer
- Medidas de raios cósmicos podem levar ao entendimento da matéria escura. [Depoimento a José Tadeu Arantes]
- Observation of the identical rigidity dependence of the primary cosmic rays helium, carbon and oxygen fluxes by the alpha magnetic spectrometer on the International Space Station
- Measurements of light nuclear isotopic composition in cosmic rays with the alpha magnetic spectrometer on the international space station
- Precise measurement of cosmic ray fluxes with the AMS-02 experiment
Informações sobre o DOI: 10.1103/PhysRevLett.117.091103 (Fonte: oaDOI API)
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