Summary
“Door” energies are found in the framework of the “shadow” model for sub-barrier at very low energy. It is suggested to solve the solar-neutrino problem by using these “door” energies.
References
A. Scalia:Nuovo Cimento A,105, 233 (1992).
A. Scalia:J. Ital. Astron. Soc., Vol. 60, N. 1-2 (1989);Nuovo Cimento A,100, 559 (1988);101, 355, 795 (1989);102, 953, 1101, 1105 (1989);103, 85, 213, 255, 927, 1177 (1990).The nuclear fusion for the reaction 3H(d, n)4He,Proceedings of the International Nuclear Physics Conference, Sao Paulo, Brasil, 1989; The reaction, rate for light systems by using the extended elastic model III, Proceedings of the Fourth International Conference on Nucleus-Nucleus Collision, Kanazawa, Japan, 1991; The sub-barrier fusion process obtained as the “shadow” of the elastic scattering, Proceedings of the International Nuclear Physics Conference, Weisbaden, Germany, 1992;A. Scalia, R. Giordano, P. Figuera andS. Pirrone:Nuovo Cimento A,103, 465 (1990);A. Scalia andP. Figuera:Phys. Rev. C,46, 2610 (1992);A. Scalia:Phys. Rev. C,47, 1247 (1993).
Gallex Collaboration:Solar neutrinos observed by Gallex at Gran Sasso, submitted toPhys. Lett. B (1992);Implications of the Gallex determination of the solar neutrino flux, submitted toPhys. Lett. B (1992).
J. N. Bahacall:Neutrino Astrophysics (Cambridge University Press, Cambridge, 1989).
R. Davis, D. S. Harmer andK. C. Hoffman:Phys. Rev. Lett.,20, 1205 (1968);R. Davis:Proceedings of the XXI International Cosmic Ray Conference, edited byR. J. Protheroe (University of Adelaide Press, Adelaide, 1992), Vol. 12, p. 143;K. S. Hirata et al.: Phys. Rev. Lett.,65, 1297 (1990);66, 6 (1991).
C. Rolfs, H. P. Trautvetter andW. S. Rodney:Rep. Prog. Phys.,50, 233 (1987)
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Scalia, A. “Door” energies in sub-barrier fusion at very low energy. Nuov Cim A 106, 855–858 (1993). https://doi.org/10.1007/BF02771499
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DOI: https://doi.org/10.1007/BF02771499