6533b7dbfe1ef96bd127087c

RESEARCH PRODUCT

Gamow-Teller Transitions Studied in ([sup 3]He, t) Reaction and Analogous β decay

Y. FujitaB. RubioF. MolinaW. GelletlyRicardo AlarconPhil ColeAndres J. KreinerHugo F. Arellano

subject

Nuclear physicsPhysicsNuclear reactionNucleosynthesisIsospinHadronElementary particleAtomic physicsNucleonIsotopes of heliumRadioactive decay

description

Due to the simplicity of the στ operator that causes Gamow‐Teller (GT) transitions, they are the most popular nuclear weak process in the Universe. The GT transitions in pf‐shell nuclei, for example, starting from stable Tz = +1 and proton‐rich Tz = +1 nuclei, where Tz = (N−Z)/2, play important roles in the supernova‐explosion or rp‐process nucleosynthesis. In the β‐decay study of pf‐shell nuclei, half‐lives can be measured rather accurately. On the other hand, in a high‐resolution (3He, t) charge‐exchange reaction at 0°, individual GT transitions up to high excitations can be studied. In order to derive reliable GT transition strengths B(GT), we present a unique analysis that combines the strength distribution form the (3He, t) measurement with the information from the study of mirror β decay, where good isospin symmetry of Tz = ±1→0 transitions is assumed.

https://doi.org/10.1063/1.3480153