Evaluation of effective astrophysical S factor for non-resont reactions (2002)
- Authors:
- USP affiliated authors: PATO, MAURICIO PORTO - IF ; HUSSEIN, MAHIR SALEH - IF
- Unidade: IF
- Subjects: FÍSICA NUCLEAR; PARTÍCULAS ELEMENTARES; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Source:
- Título: Progress of Theoretical Physics Supplement
- ISSN: 0375-9687
- Volume/Número/Paginação/Ano: v. 146, p. 634-635, 2002
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ABNT
UEDA, Manabu et al. Evaluation of effective astrophysical S factor for non-resont reactions. Progress of Theoretical Physics Supplement, v. 146, p. 634-635, 2002Tradução . . Acesso em: 15 out. 2024. -
APA
Ueda, M., Sargeant, A. J., Pato, M. P., & Hussein, M. S. (2002). Evaluation of effective astrophysical S factor for non-resont reactions. Progress of Theoretical Physics Supplement, 146, 634-635. -
NLM
Ueda M, Sargeant AJ, Pato MP, Hussein MS. Evaluation of effective astrophysical S factor for non-resont reactions. Progress of Theoretical Physics Supplement. 2002 ; 146 634-635.[citado 2024 out. 15 ] -
Vancouver
Ueda M, Sargeant AJ, Pato MP, Hussein MS. Evaluation of effective astrophysical S factor for non-resont reactions. Progress of Theoretical Physics Supplement. 2002 ; 146 634-635.[citado 2024 out. 15 ] - Inverse free electron laser acceleration
- Forward glory phenomenon in the dark-side of heavy-ion nuclear rainbown scattering
- Inverse dynamics in the classical Fermi accelerator
- Saturation of the width of the strength function
- Causal classical theory of radiation damping
- Attenuation of the intensity within a superdeformed band
- Fractal strucuture of random matrices
- Uniform expansion of the thermonuclear reaction rate formula
- Chaotic effects in nuclear tunnelling phenomena
- Energy averages and fluctuations in the decay out of superdeformed bands
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