dorsal/arxiv
View SchemaSchr\"odinger Quantization Problem and Neutron Stars
| Authors | Plamen P. Fiziev |
|---|---|
| Categories | |
| ArXiv ID | quant-ph/0310141 |
| URL | https://arxiv.org/abs/quant-ph/0310141 |
Abstract
We are discussing the possibility to find a proper unique conditions for an experimental study of the Schr\"odinger quantization problem in the neutron stars physics. A simple toy model for physically different quantizations is formulated and a possible physical consequences are derived.
{
"annotation_id": "752a4d1c-4612-4ae8-bf86-c838e62667dd",
"date_created": "2026-03-02T18:02:03.173000Z",
"date_modified": "2026-03-02T18:02:03.173000Z",
"file_hash": "7f9c643e3ff1ee1617c484f006fdb9e9b1d2cbd8b0c87b6b9fb11913774abb88",
"private": false,
"record": {
"abstract": "We are discussing the possibility to find a proper unique conditions for an\nexperimental study of the Schr\\\"odinger quantization problem in the neutron\nstars physics. A simple toy model for physically different quantizations is\nformulated and a possible physical consequences are derived.",
"arxiv_id": "quant-ph/0310141",
"authors": [
"Plamen P. Fiziev"
],
"categories": [
"quant-ph"
],
"title": "Schr\\\"odinger Quantization Problem and Neutron Stars",
"url": "https://arxiv.org/abs/quant-ph/0310141"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "6ed797d6-0289-4f97-b331-6b241e7e1bb7",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}