{
  "annotation_id": "aa999dcb-5a2a-4608-901a-9de320de01b9",
  "date_created": "2026-03-02T18:00:22.318000Z",
  "date_modified": "2026-03-02T18:00:22.318000Z",
  "file_hash": "340091767e2267d1cb75439d3fa51db2fa9632a34ac7da3a0665fc2e015f9aee",
  "private": false,
  "record": {
    "abstract": "Assuming a binary reaction mechanism, the yield of isotopes near the heaviest\n$N=Z$ neutron-deficit nucleus $^{100}$Sn is studied with a microscopic\ntransport model. The large influence of nuclear shell structure and isotope\ncomposition of the colliding nuclei on the production of exotic nuclei is\ndemonstrated. It is shown that the reaction $^{54}$Fe+$^{106}$Cd seems to be\nmost favourable for producing primary exotic Sn isotopes which may survive if\nthe excitation energy in the entrance reaction channel is less than about 100\nMeV. In the case of large differences in the charge (mass) numbers between\nentrance and exit channels the light fragment yield is essentially fed from the\ndecay of excited primary heavier fragments. The existence of optimal energies\nfor the production of some oxygen isotopes in the binary mechanism is\ndemonstrated for the $^{32}$S+$^{197}$Au reaction.",
    "arxiv_id": "nucl-th/9711037",
    "authors": [
      "N. V. Antonenko",
      "A. K. Nasirov",
      "T. M. Shneidman",
      "V. D. Toneev"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.57.1832",
    "journal_ref": "Phys.Rev.C57:1832-1838,1998",
    "title": "Towards exotic nuclei via binary reaction mechanism",
    "url": "https://arxiv.org/abs/nucl-th/9711037"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f85cefc7-7772-4a7c-9963-30f7a3d72dc1",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}