dorsal/arxiv
View SchemaHow soliton- anti soliton di quark pairs signify an Einstein constant dominated cosmology and facilitate reconstruction of initial dark matter contributions to CMB
| Authors | A. W. Beckwith |
|---|---|
| Categories | |
| ArXiv ID | physics/0510039 |
| URL | https://arxiv.org/abs/physics/0510039 |
| DOI | 10.1063/1.2220425 |
Abstract
We review the results of 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. The intial 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 cange it afterwards as the slope of the scalar field moves away from a thin wall approximation. All this is to aid in a data reconstruction problem of how to account for the initial origins of CMB due to dark matter since effective field theories as presently constructed require a cut off value for applicability of their potential structure. This is often at the cost of, especially in early universe theoretical models, of clearly defined baryogenesis, and of a well defined mechanism of phase transitions. The material below is now a proposal, in part accepted as a point of discussion as a white paper (appropriately) submitted to the Dark Energy Task Force, in its mission to advise (through its parent committees) the NSF, NASA and DOE. This was for helping to select both ground-based and space-based techniques for analyzing data as well as recommending the science requirements for a space-based dark energy mission.
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"abstract": "We review the results of a model of how nucleation of a new universe occurs,\nassuming a di quark identification for soliton-anti soliton constituent parts\nof a scalar field. The intial potential system employed is semi classical in\nnature, becoming non-classical at the end of chaotic inflation at the same time\ncosmological expansion is dominated by the Einstein cosmological constant. We\nuse Scherrer\u0027s derivation of a sound speed being zero during initial\ninflationary cosmology, and cange it afterwards as the slope of the scalar\nfield moves away from a thin wall approximation. All this is to aid in a data\nreconstruction problem of how to account for the initial origins of CMB due to\ndark matter since effective field theories as presently constructed require a\ncut off value for applicability of their potential structure. This is often at\nthe cost of, especially in early universe theoretical models, of clearly\ndefined baryogenesis, and of a well defined mechanism of phase transitions. The\nmaterial below is now a proposal, in part accepted as a point of discussion as\na white paper (appropriately) submitted to the Dark Energy Task Force, in its\nmission to advise (through its parent committees) the NSF, NASA and DOE. This\nwas for helping to select both ground-based and space-based techniques for\nanalyzing data as well as recommending the science requirements for a\nspace-based dark energy mission.",
"arxiv_id": "physics/0510039",
"authors": [
"A. W. Beckwith"
],
"categories": [
"physics.gen-ph"
],
"doi": "10.1063/1.2220425",
"title": "How soliton- anti soliton di quark pairs signify an Einstein constant dominated cosmology and facilitate reconstruction of initial dark matter contributions to CMB",
"url": "https://arxiv.org/abs/physics/0510039"
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