dorsal/arxiv
View SchemaShell model Monte Carlo calculations for Dy-170
| Authors | D. J. Dean, S. E. Koonin, G. H. Lang, P. B. Radha, W. E. Ormand |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9309027 |
| URL | https://arxiv.org/abs/nucl-th/9309027 |
| DOI | 10.1016/0370-2693(93)90995-T |
Abstract
We present the first auxiliary field Monte Carlo calculations for a rare earth nucleus, Dy-170. A pairing plus quadrupole Hamiltonian is used to demonstrate the physical properties that can be studied in this region. We calculate various static observables for both uncranked and cranked systems and show how the shape distribution evolves with temperature. We also introduce a discretization of the path integral that allows a more efficient Monte Carlo sampling.
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"date_created": "2026-03-02T18:00:11.328000Z",
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"record": {
"abstract": "We present the first auxiliary field Monte Carlo calculations for a rare\nearth nucleus, Dy-170. A pairing plus quadrupole Hamiltonian is used to\ndemonstrate the physical properties that can be studied in this region. We\ncalculate various static observables for both uncranked and cranked systems and\nshow how the shape distribution evolves with temperature. We also introduce a\ndiscretization of the path integral that allows a more efficient Monte Carlo\nsampling.",
"arxiv_id": "nucl-th/9309027",
"authors": [
"D. J. Dean",
"S. E. Koonin",
"G. H. Lang",
"P. B. Radha",
"W. E. Ormand"
],
"categories": [
"nucl-th"
],
"doi": "10.1016/0370-2693(93)90995-T",
"title": "Shell model Monte Carlo calculations for Dy-170",
"url": "https://arxiv.org/abs/nucl-th/9309027"
},
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"source": {
"execution_id": "28c20bb2-7858-42b2-b159-cc5e8a68cdfc",
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"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
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