dorsal/arxiv
View SchemaHow the alteration of a thin wall for soliton-anti soliton di quark pairs signifies an Einstein constant dominated cosmology and a role for Extra dimensions in initial nucleation of a new universe
| Authors | A. W. Beckwith |
|---|---|
| Categories | |
| ArXiv ID | physics/0509167 |
| URL | https://arxiv.org/abs/physics/0509167 |
Abstract
We use as a model of how nucleation of a new universe occurs, assuming a di quark identification for soliton-anti soliton constituent parts of a scalar field. We construct a model showing evolutin from a dark matter dark energy mix to a pure cosmological constant cosmology due to changes in the slope of a graph of the resulting scalar field. The initial potential system employed is semi classical in nature, becoming non classical at the end of chaotic inflation at the same time cosmological expansion is dominated by the Einstein cosmological constant. We use Scherrer's derivation of a sound speed being zero during initial inflationary cosmology and change it afterwards as the slope of the scalar field moves away from a thin wall approximation. Furthermore, the results in Bo Qin's article about extra dimensions from dark matter, permit us to show the impact of dimensionality upon the rule of semi classical approximations to inflation models. We conclude that the new force law specified by Bo Qin and additional dimensions would play a role in the early universe and be extremely important to the onset of inflationary expansion due to nucleation of di quark pairs in a soliton-anti soliton configuration.
{
"annotation_id": "25dcc50e-647a-4ea7-afcb-6aed0169dd4b",
"date_created": "2026-03-02T18:01:00.801000Z",
"date_modified": "2026-03-02T18:01:00.801000Z",
"file_hash": "fa534eb26a2c8ce7c00d3df6c658b9af59a4cf23fe0a4933bc19cc606cdf4aca",
"private": false,
"record": {
"abstract": "We use as a model of how nucleation of a new universe occurs, assuming a di\nquark identification for soliton-anti soliton constituent parts of a scalar\nfield. We construct a model showing evolutin from a dark matter dark energy mix\nto a pure cosmological constant cosmology due to changes in the slope of a\ngraph of the resulting scalar field. The initial potential system employed is\nsemi classical in nature, becoming non classical at the end of chaotic\ninflation at the same time cosmological expansion is dominated by the Einstein\ncosmological constant. We use Scherrer\u0027s derivation of a sound speed being zero\nduring initial inflationary cosmology and change it afterwards as the slope of\nthe scalar field moves away from a thin wall approximation. Furthermore, the\nresults in Bo Qin\u0027s article about extra dimensions from dark matter, permit us\nto show the impact of dimensionality upon the rule of semi classical\napproximations to inflation models. We conclude that the new force law\nspecified by Bo Qin and additional dimensions would play a role in the early\nuniverse and be extremely important to the onset of inflationary expansion due\nto nucleation of di quark pairs in a soliton-anti soliton configuration.",
"arxiv_id": "physics/0509167",
"authors": [
"A. W. Beckwith"
],
"categories": [
"physics.gen-ph"
],
"title": "How the alteration of a thin wall for soliton-anti soliton di quark pairs signifies an Einstein constant dominated cosmology and a role for Extra dimensions in initial nucleation of a new universe",
"url": "https://arxiv.org/abs/physics/0509167"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "77ceb69b-5f1f-4d31-8e54-7efb4a35cd6b",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}