dorsal/arxiv
View SchemaAnalysis of the thermal cross section of the capture reaction 13C(n,gamma)14C
| Authors | H. Herndl, H. Oberhummer |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9710007 |
| URL | https://arxiv.org/abs/nucl-th/9710007 |
Abstract
We investigate the thermal cross section of the reaction 13C(n,gamma)14}C which takes place in the helium burning zones of red giant star as well as in the nucleosynthesis of Inhomogeneous Big Bang models. We find that we can reproduce the experimentally known thermal capture cross section only if we take into account a strong hindrance of the E1 transition in the nuclear interior. This effect can be explained by the strong coupling to the giant dipole resonance.
{
"annotation_id": "fb6c3a47-2ed9-4e18-90d5-41b250789bc7",
"date_created": "2026-03-02T18:00:21.104000Z",
"date_modified": "2026-03-02T18:00:21.104000Z",
"file_hash": "6e79698319845c773c94b9f9c738df829550fb4a369b6c9a7b5655b4c0807dc5",
"private": false,
"record": {
"abstract": "We investigate the thermal cross section of the reaction 13C(n,gamma)14}C\nwhich takes place in the helium burning zones of red giant star as well as in\nthe nucleosynthesis of Inhomogeneous Big Bang models. We find that we can\nreproduce the experimentally known thermal capture cross section only if we\ntake into account a strong hindrance of the E1 transition in the nuclear\ninterior. This effect can be explained by the strong coupling to the giant\ndipole resonance.",
"arxiv_id": "nucl-th/9710007",
"authors": [
"H. Herndl",
"H. Oberhummer"
],
"categories": [
"nucl-th",
"nucl-ex"
],
"title": "Analysis of the thermal cross section of the capture reaction 13C(n,gamma)14C",
"url": "https://arxiv.org/abs/nucl-th/9710007"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "296a6189-f238-4a54-b021-04fff00e17b8",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}