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Artigo de periodico
Charged-particle branching ratios above the neutron threshold in F-19: Constraining N-15 production in core-collapse supernovae (2021)
Adsley, Philip ; Guimaraes, Valdir
Source: Physical Review C. Unidade: IF
Subjects: FÍSICA NUCLEAR, ASTROFÍSICA, SUPERNOVAS, ESPALHAMENTO, NÊUTRONS, HÉLIO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ADSLEY, Philip e GUIMARAES, Valdir. Charged-particle branching ratios above the neutron threshold in F-19: Constraining N-15 production in core-collapse supernovae. Physical Review C, v. 103, n. 3, 2021Tradução . . Disponível em: https://doi.org/10.1103/PhysRevC.103.035804. Acesso em: 30 jul. 2024.
APA
Adsley, P., & Guimaraes, V. (2021). Charged-particle branching ratios above the neutron threshold in F-19: Constraining N-15 production in core-collapse supernovae. Physical Review C, 103( 3). doi:10.1103/PhysRevC.103.035804
NLM
Adsley P, Guimaraes V. Charged-particle branching ratios above the neutron threshold in F-19: Constraining N-15 production in core-collapse supernovae [Internet]. Physical Review C. 2021 ; 103( 3):[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/PhysRevC.103.035804
Vancouver
Adsley P, Guimaraes V. Charged-particle branching ratios above the neutron threshold in F-19: Constraining N-15 production in core-collapse supernovae [Internet]. Physical Review C. 2021 ; 103( 3):[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/PhysRevC.103.035804
Artigo de periodico
Constraints for stellar electron-capture rates on86Kr via the86Kr(t,3He+γ)86Br reactionand the implications for core-collapse supernovae (2019)
Titus, R; Cardona, Juan Carlos Zamora
Source: Physical Review C. Unidade: IF
Assunto: SUPERNOVAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
TITUS, R e CARDONA, Juan Carlos Zamora. Constraints for stellar electron-capture rates on86Kr via the86Kr(t,3He+γ)86Br reactionand the implications for core-collapse supernovae. Physical Review C, v. 100, p. 045805(14), 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevC.100.045805. Acesso em: 30 jul. 2024.
APA
Titus, R., & Cardona, J. C. Z. (2019). Constraints for stellar electron-capture rates on86Kr via the86Kr(t,3He+γ)86Br reactionand the implications for core-collapse supernovae. Physical Review C, 100, 045805(14). doi:10.1103/PhysRevC.100.045805
NLM
Titus R, Cardona JCZ. Constraints for stellar electron-capture rates on86Kr via the86Kr(t,3He+γ)86Br reactionand the implications for core-collapse supernovae [Internet]. Physical Review C. 2019 ;100 045805(14).[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/PhysRevC.100.045805
Vancouver
Titus R, Cardona JCZ. Constraints for stellar electron-capture rates on86Kr via the86Kr(t,3He+γ)86Br reactionand the implications for core-collapse supernovae [Internet]. Physical Review C. 2019 ;100 045805(14).[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/PhysRevC.100.045805
Artigo de periodico
Stability of phantom k-essence theories (2006)
Abramo, Luis Raul Weber; Pinto Neto, N
Source: Physical Review C. Unidade: IF
Subjects: COSMOLOGIA, SUPERNOVAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ABRAMO, Luis Raul Weber e PINTO NETO, N. Stability of phantom k-essence theories. Physical Review C, v. 73, n. 3, p. 063522/1-063522/4, 2006Tradução . . Disponível em: https://doi.org/10.1103/physrevd.73.063522. Acesso em: 30 jul. 2024.
APA
Abramo, L. R. W., & Pinto Neto, N. (2006). Stability of phantom k-essence theories. Physical Review C, 73( 3), 063522/1-063522/4. doi:10.1103/physrevd.73.063522
NLM
Abramo LRW, Pinto Neto N. Stability of phantom k-essence theories [Internet]. Physical Review C. 2006 ;73( 3): 063522/1-063522/4.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/physrevd.73.063522
Vancouver
Abramo LRW, Pinto Neto N. Stability of phantom k-essence theories [Internet]. Physical Review C. 2006 ;73( 3): 063522/1-063522/4.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/physrevd.73.063522

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