The effective astrophysical S-factor for non-resonant reactions (1999)
- Authors:
- USP affiliated authors: HUSSEIN, MAHIR SALEH - IF ; PATO, MAURICIO PORTO - IF
- Unidade: IF
- Subjects: FÍSICA NUCLEAR; FÍSICA NUCLEAR
- Language: Inglês
- Imprenta:
-
ABNT
HUSSEIN, Mahir Saleh et al. The effective astrophysical S-factor for non-resonant reactions. . São Paulo: IFUSP. Disponível em: http://publica-sbi.if.usp.br/PDFs/pd1383.pdf. Acesso em: 15 fev. 2026. , 1999 -
APA
Hussein, M. S., Pato, M. P., Sargeant, A. J., & Ueda, M. (1999). The effective astrophysical S-factor for non-resonant reactions. São Paulo: IFUSP. Recuperado de http://publica-sbi.if.usp.br/PDFs/pd1383.pdf -
NLM
Hussein MS, Pato MP, Sargeant AJ, Ueda M. The effective astrophysical S-factor for non-resonant reactions [Internet]. 1999 ;[citado 2026 fev. 15 ] Available from: http://publica-sbi.if.usp.br/PDFs/pd1383.pdf -
Vancouver
Hussein MS, Pato MP, Sargeant AJ, Ueda M. The effective astrophysical S-factor for non-resonant reactions [Internet]. 1999 ;[citado 2026 fev. 15 ] Available from: http://publica-sbi.if.usp.br/PDFs/pd1383.pdf - Analytical treatment of heavy-ion elastic scattering at intermediate energies
- Time delay in semiclassical scattering theory
- Saturation of the width of the strenght function
- Chaos and fluctuations in the decay out of superdeformed bands
- Rainbows in 'K IND.I''ETA'' (KSI)'
- Non-linear amplification of inverse-bremsstrahlung electron acceleration
- Refraction-diffraction interference in heavy-ion elastic angular distributions
- Semiclassical analysis of the so (3,1) s-matrix
- Semiclassical analysis of the so (3,1) s - matrix
- Super collider revisited
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