{
  "annotation_id": "d3ae34f3-4b93-4792-b782-9b0f25b184b0",
  "date_created": "2026-03-02T18:00:04.824000Z",
  "date_modified": "2026-03-02T18:00:04.824000Z",
  "file_hash": "fa2e701f39fb6be74c99c97ac5a996b1f2338b33e55c2f1168bbe8dddb92ce66",
  "private": false,
  "record": {
    "abstract": "Shell model calculations have been done for interpreting two representative\nisomeric states in neutron rich $^{132}Sn$ region using SMN and SMPN\nHamiltonians. They are, (i) 2.91 min isomer in $^{138}Cs$ and (ii) the 0.57\n$\\mu s$ isomer in $^{136}$Sb nuclei. The results are compared with those\nobtained with KH5082 and CW5082 Hamiltonians. How the results clearly\ndistinguish the most appropriate interaction has been discussed.",
    "arxiv_id": "nucl-th/0507034",
    "authors": [
      "S. Sarkar",
      "M. Saha Sarkar"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Study of isomers in neutron-rich magic $^{132}$Sn region",
    "url": "https://arxiv.org/abs/nucl-th/0507034"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "2b6985e5-1a04-4c8d-a79b-ab6d413df8d2",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}