dorsal/arxiv
View SchemaLight-Front Dynamics
| Authors | V. A. Karmanov |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9907037 |
| URL | https://arxiv.org/abs/nucl-th/9907037 |
Abstract
The wave function in relativity is defined, in four-dimensional space, on a space-like three-dimensional plane. The plane, most close to the time-like region, is the light-front plane $ct+z=0$. Corresponding dynamical approach - the light-front dynamics - has considerable advantages. We describe, in a field-theoretical framework, the construction of light-front dynamics and illustrate it by some examples.
{
"annotation_id": "2c2c9379-a743-4e38-b2f1-3d5b881d36a7",
"date_created": "2026-03-02T18:00:25.528000Z",
"date_modified": "2026-03-02T18:00:25.528000Z",
"file_hash": "f109875bb7603fc51ffd5aea30daca21b4f149c5529a08da6525a7258641ce7f",
"private": false,
"record": {
"abstract": "The wave function in relativity is defined, in four-dimensional space, on a\nspace-like three-dimensional plane. The plane, most close to the time-like\nregion, is the light-front plane $ct+z=0$. Corresponding dynamical approach -\nthe light-front dynamics - has considerable advantages. We describe, in a\nfield-theoretical framework, the construction of light-front dynamics and\nillustrate it by some examples.",
"arxiv_id": "nucl-th/9907037",
"authors": [
"V. A. Karmanov"
],
"categories": [
"nucl-th",
"hep-ph",
"hep-th"
],
"title": "Light-Front Dynamics",
"url": "https://arxiv.org/abs/nucl-th/9907037"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "46873ad2-348c-4798-99d2-4397528866f8",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}