Author:
Yang Z. H.,Kubota Y.,Corsi A.,Authelet G.,Baba H.,Caesar C.,Calvet D.,Delbart A.,Dozono M.,Feng J.,Flavigny F.,Gheller J.-M.,Gibelin J.,Giganon A.,Gillibert A.,Hasegawa K.,Isobe T.,Kanaya Y.,Kawakami S.,Kim D.,Kiyokawa Y.,Kobayashi M.,Kobayashi N.,Kobayashi T.,Kondo Y.,Korkulu Z.,Koyama S.,Lapoux V.,Maeda Y.,Marqués F. M.,Motobayashi T.,Miyazaki T.,Nakamura T.,Nakatsuka N.,Nishio Y.,Obertelli A.,Ohkura A.,Orr N. A.,Ota S.,Otsu H.,Ozaki T.,Panin V.,Paschalis S.,Pollacco E. C.,Reichert S.,Roussé J.-Y.,Saito A. T.,Sakaguchi S.,Sako M.,Santamaria C.,Sasano M.,Sato H.,Shikata M.,Shimizu Y.,Shindo Y.,Stuhl L.,Sumikama T.,Sun Y.,Tabata M.,Togano Y.,Tsubota J.,Uesaka T.,Yasuda J.,Yoneda K.,Zenihiro J.
Abstract
Abstract
Spectroscopy of 16B plays an essential role in understanding the halo structure in 17B, but very limited knowledge has so far been obtained. We have carried out a kinematically complete measurement on the spectroscopy of 16B by using quasi-free (p,pn) reaction on 17B. The level scheme of 16B up to 5 MeV was made clear for the first time.
Subject
General Physics and Astronomy