dorsal/arxiv
View SchemaThe stability of the relativistic three-body system and in-medium equations
| Authors | Stefano Mattiello |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0401050 |
| URL | https://arxiv.org/abs/nucl-th/0401050 |
| DOI | 10.1007/s00601-004-0032-8 |
| Journal | Few Body Syst. 34 (2004) 119-125 |
Abstract
We present a relativistic three-body equation to study the stability of the isolated three-body system and the correlations in a medium of finite temperatures and densities. Relativity is implemented utilizing the light front form. Using a zero-range force we find the relativistic analog of the Thomas collapse and investigate the possibility that the nucleon exists as a Borromean system. Within a systematic Dyson equation approach we calculate the three-body Mott transition and the critical temperature of the color-superconducting phase.
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"abstract": "We present a relativistic three-body equation to study the stability of the\nisolated three-body system and the correlations in a medium of finite\ntemperatures and densities. Relativity is implemented utilizing the light front\nform. Using a zero-range force we find the relativistic analog of the Thomas\ncollapse and investigate the possibility that the nucleon exists as a Borromean\nsystem. Within a systematic Dyson equation approach we calculate the three-body\nMott transition and the critical temperature of the color-superconducting\nphase.",
"arxiv_id": "nucl-th/0401050",
"authors": [
"Stefano Mattiello"
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"doi": "10.1007/s00601-004-0032-8",
"journal_ref": "Few Body Syst. 34 (2004) 119-125",
"title": "The stability of the relativistic three-body system and in-medium equations",
"url": "https://arxiv.org/abs/nucl-th/0401050"
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