Role of Tensor Force in Light Nuclei based on The Tensor Optimized Shell Model

Journal Article · Thu Aug 12 00:00:00 EDT 2010 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.3485167· OSTI ID:21435992

Myo, Takayuki ^[1]; Toki, Hiroshi ^[2]; Ikeda, Kiyomi ^[3]

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1. Osaka Institute of Technology, Osaka, Osaka 535-8585 (Japan)
2. Research Center for Nuclear Physics (RCNP), Ibaraki, Osaka 567-0047 (Japan)
3. RIKEN Nishina Center, Wako, Saitama 351-0198 (Japan)

We propose a new method to describe nuclear structure using bare nuclear interaction, in which the tensor and short-range correlations are described by using the tensor optimized shell model (TOSM) and the unitary correlation operator method (UCOM), respectively.

• OSTI ID: 21435992
• Journal Information: AIP Conference Proceedings, Vol. 1269, Issue 1; Conference: OMEG-2010: 10. international symposium on origin of matter and evolution of galaxies, Osaka (Japan), 8-10 Mar 2010; Other Information: DOI: 10.1063/1.3485167; (c) 2010 American Institute of Physics; ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
CORRELATIONS
LIGHT NUCLEI
MONTE CARLO METHOD
NUCLEAR FORCES
NUCLEAR STRUCTURE
NUCLEON-NUCLEON INTERACTIONS
SHELL MODELS
SUPERNOVAE
TENSOR FORCES
TENSORS
BARYON-BARYON INTERACTIONS
BINARY STARS
CALCULATION METHODS
ERUPTIVE VARIABLE STARS
HADRON-HADRON INTERACTIONS
INTERACTIONS
MATHEMATICAL MODELS
NUCLEAR MODELS
NUCLEI
PARTICLE INTERACTIONS
STARS
VARIABLE STARS