### Abstract

We present the first auxiliary field Monte Carlo calculations for a rare earth nucleus, ^{170}Dy. We calculate various static Hamiltonian is used to demonstrate the physical properties that can be studied in this region. We calculate various static observables for both uncranked and crancked 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.

Original language | English (US) |
---|---|

Pages (from-to) | 275-280 |

Number of pages | 6 |

Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |

Volume | 317 |

Issue number | 3 |

DOIs | |

State | Published - Nov 11 1993 |

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### ASJC Scopus subject areas

- Nuclear and High Energy Physics

### Cite this

*Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics*,

*317*(3), 275-280. https://doi.org/10.1016/0370-2693(93)90995-T

**Shell model Monte Carlo calculations for 170Dy.** / Dean, D. J.; Koonin, S. E.; Lang, G. H.; Ormand, W. E.; Radha, P. B.

Research output: Contribution to journal › Article

*Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics*, vol. 317, no. 3, pp. 275-280. https://doi.org/10.1016/0370-2693(93)90995-T

}

TY - JOUR

T1 - Shell model Monte Carlo calculations for 170Dy

AU - Dean, D. J.

AU - Koonin, S. E.

AU - Lang, G. H.

AU - Ormand, W. E.

AU - Radha, P. B.

PY - 1993/11/11

Y1 - 1993/11/11

N2 - We present the first auxiliary field Monte Carlo calculations for a rare earth nucleus, 170Dy. We calculate various static Hamiltonian is used to demonstrate the physical properties that can be studied in this region. We calculate various static observables for both uncranked and crancked 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.

AB - We present the first auxiliary field Monte Carlo calculations for a rare earth nucleus, 170Dy. We calculate various static Hamiltonian is used to demonstrate the physical properties that can be studied in this region. We calculate various static observables for both uncranked and crancked 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.

UR - http://www.scopus.com/inward/record.url?scp=0000681658&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0000681658&partnerID=8YFLogxK

U2 - 10.1016/0370-2693(93)90995-T

DO - 10.1016/0370-2693(93)90995-T

M3 - Article

AN - SCOPUS:0000681658

VL - 317

SP - 275

EP - 280

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

SN - 0370-2693

IS - 3

ER -