T. Hayakawa   K. Ogata   S. Miyamoto   T. Mochizuki   K. Horikawa   S. Amano   K. Imazaki   D. Li   Y. Izawa   S. Chiba   
ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2013 1594 326-331 2014年 [査読有り]
The M1 strengths (or level density of 1(+) states) are of importance for estimation of interaction strengths between neutrinos and nuclei for the study of the supernova neutrino-process. In 1957, Agodi predicted theoretically angular distribution ...