dorsal/arxiv
View SchemaQuasi-elastic barrier distribution as a tool for investigating unstable nuclei
| Authors | K. Hagino, N. Rowley |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0411055 |
| URL | https://arxiv.org/abs/nucl-th/0411055 |
| DOI | 10.1590/S0103-97332005000500047 |
| Journal | Braz.J.Phys. 35 (2005) 890-893 |
Abstract
The method of fusion barrier distribution has been widely used to interpret the effect of nuclear structure on heavy-ion fusion reactions around the Coulomb barrier. We discuss a similar, but less well known, barrier distribution extracted from large-angle quasi-elastic scattering. We argue that this method has several advantages over the fusion barrier distribution, and offers an interesting tool for investigating unstable nuclei.
{
"annotation_id": "c550376b-186f-463f-b2e2-b9fe09bae9e9",
"date_created": "2026-03-02T18:00:01.086000Z",
"date_modified": "2026-03-02T18:00:01.086000Z",
"file_hash": "db5932dfdd7ac3631fa605e5939f0508fe1fa0358510525a43f3f1cc4440febc",
"private": false,
"record": {
"abstract": "The method of fusion barrier distribution has been widely used to interpret\nthe effect of nuclear structure on heavy-ion fusion reactions around the\nCoulomb barrier. We discuss a similar, but less well known, barrier\ndistribution extracted from large-angle quasi-elastic scattering. We argue that\nthis method has several advantages over the fusion barrier distribution, and\noffers an interesting tool for investigating unstable nuclei.",
"arxiv_id": "nucl-th/0411055",
"authors": [
"K. Hagino",
"N. Rowley"
],
"categories": [
"nucl-th",
"nucl-ex"
],
"doi": "10.1590/S0103-97332005000500047",
"journal_ref": "Braz.J.Phys. 35 (2005) 890-893",
"title": "Quasi-elastic barrier distribution as a tool for investigating unstable nuclei",
"url": "https://arxiv.org/abs/nucl-th/0411055"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "e9009d1e-6772-446e-b449-3a91faf3cbdf",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}