Complete 0ℏω shell model Monte Carlo calculations of 94Ru, 96Pd, 96,98Cd and 100Sn

D. J. Dean; S. E. Koonin; T. T S Kuo; K. Langanke; P. B. Radha

doi:10.1016/0370-2693(95)01446-2

Complete 0ℏω shell model Monte Carlo calculations of ⁹⁴Ru, ⁹⁶Pd, ^96,98Cd and ¹⁰⁰Sn

D. J. Dean, S. E. Koonin, T. T S Kuo, K. Langanke, P. B. Radha

Research output: Contribution to journal › Article › peer-review

Abstract

We perform shell model Monte Carlo calculations for nuclei in the ¹⁰⁰Sn region within the complete 0g-1d-2s oscillator shell using an effective interaction derived from the Paris nucleon-nucleon potential. We find good agreement with empirically calculated masses, and reproduce the observed quenching of the total Gamow-Teller strengths in this mass region. The Gamow-Teller strength in ¹⁰⁰Sn is predicted to be nearly a factor of 3 smaller than the single particle estimate.

Original language	English (US)
Pages (from-to)	17-20
Number of pages	4
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	367
Issue number	1-4
DOIs	https://doi.org/10.1016/0370-2693(95)01446-2
State	Published - Jan 18 1996

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/0370-2693(95)01446-2

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@article{9bec2e226c6f40fba8bd20ff4cd1c32e,

title = "Complete 0ℏω shell model Monte Carlo calculations of 94Ru, 96Pd, 96,98Cd and 100Sn",

abstract = "We perform shell model Monte Carlo calculations for nuclei in the 100Sn region within the complete 0g-1d-2s oscillator shell using an effective interaction derived from the Paris nucleon-nucleon potential. We find good agreement with empirically calculated masses, and reproduce the observed quenching of the total Gamow-Teller strengths in this mass region. The Gamow-Teller strength in 100Sn is predicted to be nearly a factor of 3 smaller than the single particle estimate.",

author = "Dean, {D. J.} and Koonin, {S. E.} and Kuo, {T. T S} and K. Langanke and Radha, {P. B.}",

note = "Funding Information: This work was supportedin part by the National ScienceF oundationG, rant Nos. PHY94-12818a nd PHY94-20470a, ndb y the US Departmenotf Energy underC ontractN o. DE-AC05-84GR21 400m anaged by LockheedM artin Energy SystemsW. e acknowl- edgea granto f computationcayl cleso n theM aui SP-2 operatedb y theP hillipsL aboratoryA, ir ForceM a-terialC ommandU, SAF, underc ooperativaeg reement numberF 29601-93-2-000D1.. J.D. acknowledgeasn E.P. WignerF ellowshipf rom ORNL.",

year = "1996",

month = jan,

day = "18",

doi = "10.1016/0370-2693(95)01446-2",

language = "English (US)",

volume = "367",

pages = "17--20",

journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",

issn = "0370-2693",

publisher = "Elsevier B.V.",

number = "1-4",

}

TY - JOUR

T1 - Complete 0ℏω shell model Monte Carlo calculations of 94Ru, 96Pd, 96,98Cd and 100Sn

AU - Dean, D. J.

AU - Koonin, S. E.

AU - Kuo, T. T S

AU - Langanke, K.

AU - Radha, P. B.

N1 - Funding Information: This work was supportedin part by the National ScienceF oundationG, rant Nos. PHY94-12818a nd PHY94-20470a, ndb y the US Departmenotf Energy underC ontractN o. DE-AC05-84GR21 400m anaged by LockheedM artin Energy SystemsW. e acknowl- edgea granto f computationcayl cleso n theM aui SP-2 operatedb y theP hillipsL aboratoryA, ir ForceM a-terialC ommandU, SAF, underc ooperativaeg reement numberF 29601-93-2-000D1.. J.D. acknowledgeasn E.P. WignerF ellowshipf rom ORNL.

PY - 1996/1/18

Y1 - 1996/1/18

N2 - We perform shell model Monte Carlo calculations for nuclei in the 100Sn region within the complete 0g-1d-2s oscillator shell using an effective interaction derived from the Paris nucleon-nucleon potential. We find good agreement with empirically calculated masses, and reproduce the observed quenching of the total Gamow-Teller strengths in this mass region. The Gamow-Teller strength in 100Sn is predicted to be nearly a factor of 3 smaller than the single particle estimate.

AB - We perform shell model Monte Carlo calculations for nuclei in the 100Sn region within the complete 0g-1d-2s oscillator shell using an effective interaction derived from the Paris nucleon-nucleon potential. We find good agreement with empirically calculated masses, and reproduce the observed quenching of the total Gamow-Teller strengths in this mass region. The Gamow-Teller strength in 100Sn is predicted to be nearly a factor of 3 smaller than the single particle estimate.

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UR - http://www.scopus.com/inward/citedby.url?scp=0003147326&partnerID=8YFLogxK

U2 - 10.1016/0370-2693(95)01446-2

DO - 10.1016/0370-2693(95)01446-2

M3 - Article

AN - SCOPUS:0003147326

SN - 0370-2693

VL - 367

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EP - 20

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

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

IS - 1-4

ER -

Complete 0ℏω shell model Monte Carlo calculations of ⁹⁴Ru, ⁹⁶Pd, ^96,98Cd and ¹⁰⁰Sn

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