dorsal/arxiv
View SchemaAstrophysical weak-interaction processes and nuclear effective field theory
| Authors | K. Kubodera |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0404027 |
| URL | https://arxiv.org/abs/nucl-th/0404027 |
Abstract
Low-energy nuclear weak-interaction processes play important roles in many astrophysical contexts, and effective field theory is believed to be a highly useful framework for describing these processes in a model-independent manner. I present a brief account of the basic features of the nuclear effective theory approach, and some examples of actual calculations carried out in this method.
{
"annotation_id": "af24b1e3-34e0-4ed3-b6ad-ad9af9f27d86",
"date_created": "2026-03-02T18:00:01.308000Z",
"date_modified": "2026-03-02T18:00:01.308000Z",
"file_hash": "d423dcadc275f7fe423e7bd7142038286a730d693441cc6e1c8b77eac1c34045",
"private": false,
"record": {
"abstract": "Low-energy nuclear weak-interaction processes play important roles in many\nastrophysical contexts, and effective field theory is believed to be a highly\nuseful framework for describing these processes in a model-independent manner.\nI present a brief account of the basic features of the nuclear effective theory\napproach, and some examples of actual calculations carried out in this method.",
"arxiv_id": "nucl-th/0404027",
"authors": [
"K. Kubodera"
],
"categories": [
"nucl-th"
],
"title": "Astrophysical weak-interaction processes and nuclear effective field theory",
"url": "https://arxiv.org/abs/nucl-th/0404027"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "fc7ef233-fce0-436a-9eaa-75854a5af116",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}