Towards exotic nuclei via binary reaction mechanism

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dc.creatorAntonenko, N. V.
dc.creatorNasirov, A. K.
dc.creatorShneidman, T. M.
dc.creatorToneev, V. D.
dc.date1997-11-19
dc.date.accessioned2026-07-07T11:11:26Z
dc.date.available2026-07-07T11:11:26Z
dc.descriptionAssuming a binary reaction mechanism, the yield of isotopes near the heaviest $N=Z$ neutron-deficit nucleus $^{100}$Sn is studied with a microscopic transport model. The large influence of nuclear shell structure and isotope composition of the colliding nuclei on the production of exotic nuclei is demonstrated. It is shown that the reaction $^{54}$Fe+$^{106}$Cd seems to be most favourable for producing primary exotic Sn isotopes which may survive if the excitation energy in the entrance reaction channel is less than about 100 MeV. In the case of large differences in the charge (mass) numbers between entrance and exit channels the light fragment yield is essentially fed from the decay of excited primary heavier fragments. The existence of optimal energies for the production of some oxygen isotopes in the binary mechanism is demonstrated for the $^{32}$S+$^{197}$Au reaction.
dc.description17 pages, RevTex, 8 Postscript figures, submitted to Phys. Rev. C
dc.identifierhttps://arxiv.org/abs/nucl-th/9711037
dc.identifierhttp://arxiv.org/abs/nucl-th/9711037
dc.identifierPhys.Rev.C57:1832-1838,1998
dc.identifierdoi:10.1103/PhysRevC.57.1832
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191096
dc.subjectNuclear Theory
dc.titleTowards exotic nuclei via binary reaction mechanism
dc.typetext

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