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Single-particle energies in neutron-rich nuclei by shell model sum rule
One of the most striking features in neutron-rich nuclei is the disappearance of magic number N=8 or 20, which indicates a change of single-particle energy spectra and the disappearance of a large energy gap at the magic number. A sum-rule method is formulated, based on the shell model, for the eval...
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Published in: | Physical review. C, Nuclear physics Nuclear physics, 2006-09, Vol.74 (3) |
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description | One of the most striking features in neutron-rich nuclei is the disappearance of magic number N=8 or 20, which indicates a change of single-particle energy spectra and the disappearance of a large energy gap at the magic number. A sum-rule method is formulated, based on the shell model, for the evaluation of single-particle energies. It is shown that the triplet-even central component of the NN interaction plays a decisive role through the monopole interaction for a change of single-particle energy spectra, leading to a rapid decrease of the energy gap at N=8 and 20. The triplet-even attraction is due partly to the original central interaction and partly to the second-order tensor correlations of the one-pion exchange potential. A multipole expansion analysis of NN interactions shows that the contribution to the single-particle energy from the monopole interactions between two orbits depends on the nodal quantum numbers of the orbits. |
doi_str_mv | 10.1103/PHYSREVC.74.034330 |
format | article |
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A sum-rule method is formulated, based on the shell model, for the evaluation of single-particle energies. It is shown that the triplet-even central component of the NN interaction plays a decisive role through the monopole interaction for a change of single-particle energy spectra, leading to a rapid decrease of the energy gap at N=8 and 20. The triplet-even attraction is due partly to the original central interaction and partly to the second-order tensor correlations of the one-pion exchange potential. 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A sum-rule method is formulated, based on the shell model, for the evaluation of single-particle energies. It is shown that the triplet-even central component of the NN interaction plays a decisive role through the monopole interaction for a change of single-particle energy spectra, leading to a rapid decrease of the energy gap at N=8 and 20. The triplet-even attraction is due partly to the original central interaction and partly to the second-order tensor correlations of the one-pion exchange potential. A multipole expansion analysis of NN interactions shows that the contribution to the single-particle energy from the monopole interactions between two orbits depends on the nodal quantum numbers of the orbits.</description><subject>CORRELATIONS</subject><subject>ENERGY GAP</subject><subject>ENERGY SPECTRA</subject><subject>EVALUATION</subject><subject>NEUTRON-RICH ISOTOPES</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>NUCLEON-NUCLEON INTERACTIONS</subject><subject>OPE MODEL</subject><subject>OPE POTENTIAL</subject><subject>ORBITS</subject><subject>PIONS</subject><subject>QUANTUM NUMBERS</subject><subject>SHELL MODELS</subject><subject>SINGLE-PARTICLE MODEL</subject><subject>SUM RULES</subject><subject>TENSORS</subject><subject>TRIPLETS</subject><issn>0556-2813</issn><issn>1089-490X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNotj0FLwzAYhoMoWKd_wFPAc2aSL0nTo5S5CQPFqehptOnXNZKl0rQH__0K-l6ewwMPvITcCr4UgsP9y-Zr97r6KJe5WnJQAPyMZILbgqmCf56TjGttmLQCLslVSt98HoDJyHrn4yEg-6mG0buAFCMOB4-J-kgjTuPQRzZ419E4zdrT-pemDkOgx77BQNN0pMMU8JpctFVIePPPBXl_XL2VG7Z9Xj-VD1vWCwEjk7UVojZOVbytW7To8qKpwWrdCK0QbVugNlUrpJa6zfX8oLbGKKyMMA1oWJC7v26fRr9Pzo_oOtfHiG7cS24NWC7hBMCOTzI</recordid><startdate>20060915</startdate><enddate>20060915</enddate><creator>Umeya, A.</creator><creator>Muto, K.</creator><scope>OTOTI</scope></search><sort><creationdate>20060915</creationdate><title>Single-particle energies in neutron-rich nuclei by shell model sum rule</title><author>Umeya, A. ; Muto, K.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-o113t-2b811b6c4a0fbfe8ec79db3855d154ee8f9e56af12525f75089b8664ea616d353</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>CORRELATIONS</topic><topic>ENERGY GAP</topic><topic>ENERGY SPECTRA</topic><topic>EVALUATION</topic><topic>NEUTRON-RICH ISOTOPES</topic><topic>NUCLEAR PHYSICS AND RADIATION PHYSICS</topic><topic>NUCLEON-NUCLEON INTERACTIONS</topic><topic>OPE MODEL</topic><topic>OPE POTENTIAL</topic><topic>ORBITS</topic><topic>PIONS</topic><topic>QUANTUM NUMBERS</topic><topic>SHELL MODELS</topic><topic>SINGLE-PARTICLE MODEL</topic><topic>SUM RULES</topic><topic>TENSORS</topic><topic>TRIPLETS</topic><toplevel>online_resources</toplevel><creatorcontrib>Umeya, A.</creatorcontrib><creatorcontrib>Muto, K.</creatorcontrib><collection>OSTI.GOV</collection><jtitle>Physical review. C, Nuclear physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Umeya, A.</au><au>Muto, K.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Single-particle energies in neutron-rich nuclei by shell model sum rule</atitle><jtitle>Physical review. C, Nuclear physics</jtitle><date>2006-09-15</date><risdate>2006</risdate><volume>74</volume><issue>3</issue><issn>0556-2813</issn><eissn>1089-490X</eissn><abstract>One of the most striking features in neutron-rich nuclei is the disappearance of magic number N=8 or 20, which indicates a change of single-particle energy spectra and the disappearance of a large energy gap at the magic number. A sum-rule method is formulated, based on the shell model, for the evaluation of single-particle energies. It is shown that the triplet-even central component of the NN interaction plays a decisive role through the monopole interaction for a change of single-particle energy spectra, leading to a rapid decrease of the energy gap at N=8 and 20. The triplet-even attraction is due partly to the original central interaction and partly to the second-order tensor correlations of the one-pion exchange potential. A multipole expansion analysis of NN interactions shows that the contribution to the single-particle energy from the monopole interactions between two orbits depends on the nodal quantum numbers of the orbits.</abstract><cop>United States</cop><doi>10.1103/PHYSREVC.74.034330</doi></addata></record> |
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subjects | CORRELATIONS ENERGY GAP ENERGY SPECTRA EVALUATION NEUTRON-RICH ISOTOPES NUCLEAR PHYSICS AND RADIATION PHYSICS NUCLEON-NUCLEON INTERACTIONS OPE MODEL OPE POTENTIAL ORBITS PIONS QUANTUM NUMBERS SHELL MODELS SINGLE-PARTICLE MODEL SUM RULES TENSORS TRIPLETS |
title | Single-particle energies in neutron-rich nuclei by shell model sum rule |
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