1. A. Scalia:Nuovo Cimento A,105, 233 (1992).
2. A. Scalia:J. Ital. Astron. Soc., Vol. 60, N. 1-2 (1989);
3. 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);
4. A. Scalia andP. Figuera:Phys. Rev. C,46, 2610 (1992);
5. A. Scalia:Phys. Rev. C,47, 1247 (1993).