Neutrino-Nucleus Reactions at MeV Region based on New Shell-Model Hamiltonians

2011 ◽  
Author(s):  
Toshio Suzuki ◽  
S. K. Singh ◽  
J. G. Morfin ◽  
Makoto Sakuda ◽  
K. D. Purohit
Keyword(s):  
Shell Model ◽  
Model Hamiltonians

scholarly journals Shell-Model Hamiltonians from Chiral Forces

2018 ◽  
Author(s):  
Sota Yoshida ◽  
Michio Kohno ◽  
Takashi Abe ◽  
Takaharu Otsuka ◽  
Naofumi Tsunoda ◽  
...  
Keyword(s):  
Shell Model ◽  
Model Hamiltonians

The structure of the spherical tensor forces in the USD and GXPF1A shell model Hamiltonians

2011 ◽  
Vol 35 (8) ◽  
pp. 753-757
Author(s):  
Han-Kui Wang ◽  
Zao-Chun Gao ◽  
Yong-Shou Chen ◽  
Jian-You Guo ◽  
Yong-Jing Chen ◽  
...  
Keyword(s):  
Shell Model ◽  
Model Hamiltonians

scholarly journals Neutrino-nucleus reactions based on new shell model Hamiltonians

2006 ◽  
Vol 74 (3) ◽  
Author(s):  
Toshio Suzuki ◽  
Satoshi Chiba ◽  
Takashi Yoshida ◽  
Toshitaka Kajino ◽  
Takaharu Otsuka
Keyword(s):  
Shell Model ◽  
Model Hamiltonians

scholarly journals Forbidden transitions in nuclear weak processes relevant to neutrino detection, nucleosynthesis and evolution of stars

2019 ◽  
Vol 223 ◽  
pp. 01063
Author(s):  
Toshio Suzuki ◽  
Satoshi Chiba ◽  
Takashi Yoshida ◽  
Koh Takahashi ◽  
Hideyuki Umeda ◽  
...  
Keyword(s):  
Shell Model ◽  
Cross Sections ◽  
Neutral Current ◽  
Expansion Method ◽  
Multipole Expansion ◽  
Reaction Cross ◽  
Model Calculations ◽  
Multipole Expansion Method ◽  
Supernova Explosions ◽  
Model Hamiltonians

The distribution of the spin-dipole strengths in 16O and neutrino-induced reactions on 16O areinvestigated by shell-model calculations with new shell-model Hamiltonians. Chargedcurrent and neutral-current reactioncross sections are valuated in various particle and γ emission channels as well as the total ones at neutrinoenergies up to Eν≈ 100 MeV. Effects of multiparticle emission channels, especially the αp emission channels, on nucleosynthesis of 11B and 11C in core-collapse supernova explosions are investigated. The MSW neutrino oscillation effects oncharged-current reaction cross sections are investigated for future supernova burst. Electron capture rates for a forbidden transition 20Ne(Og.s.+) → 20F(2g.s.+) in stellar environments are evaluated by the multipole expansion method with the use of shell model Hamiltonians, and compared with those obtained by a prescription that treats the transition as an allowed GamowTeller (GT) transition. Different electron energy dependence of the transition strengths between the two methods is found to lead to sizable differences in the weak rates of the two methods.

Sign in / Sign up

Export Citation Format

Share Document