@inproceedings{12f5b685215747918de558be67467962,
title = "Impact of the 26mAl(p, γ) reaction to galactic 26Al yield",
abstract = "Astrophysical observables that are directly linked to nuclear physics inputs provide critical and stringent constraints on nucleosynthetic models. As 26Al was the first specific radioactivity observed in the Galaxy, its origin has fascinated the nuclear astrophysics community for nearly forty years. Despite extensive research, the precise origins of 26Al remain elusive. At present, the sum of all putative stellar contributions generally overestimates the 26Al mass in the interstellar medium. Among the many reactions that influence the yield of 26Al, radiative proton capture on its isomer 26mAl is one of the least constrained reactions by experimental data. To this end, we developed a 26Al isomeric beam and performed proton elastic scattering to search for low-spin states in 27Si. The experimental method and the preliminary results of this on-going study will be presented.",
author = "D. Kahl and H. Shimizu and H. Yamaguchi and K. Abe and O. Beliuskina and Cha, {S. M.} and Chae, {K. Y.} and Chen, {A. A.} and Z. Ge and S. Hayakawa and N. Imai and N. Iwasa and A. Kim and Kim, {D. H.} and Kim, {M. J.} and S. Kubono and Kwag, {M. S.} and J. Liang and Moon, {J. Y.} and S. Nishimura and S. Oka and Park, {S. Y.} and A. Psaltis and T. Teranishi and Y. Ueno and L. Yang",
note = "Funding Information: This experiment was performed at RI Beam Factory operated by RIKEN Nishina Center and CNS, University of Tokyo. This work was partly supported by grants from the Science and Technology Facilities Council (STFC) in the United Kingdom, the JSPS KAKENHI (Grants No. 25800125 and 16K05369) in Japan, grants from the National Research Foundation (NRF) funded by the Korea government (MEST) (No. NRF-2014S1A2A2028636, NRF-2015R1D1A1A01056918, NRF-2016K1A3A7A09005579, and NRF-2016R1A5A1013277), and the Natural Sciences and Engineering Council of Canada. We also sincerely thank both the CNS and RIKEN staff for operation of the ion source and accelerator during the machine time. Funding Information: This work was partly supported by grants from the Science and Technology Facilities Council (STFC) in the United Kingdom, the JSPS KAKENHI (Grants No. 25800125 and 16K05369) in Japan, grants from the National Research Foundation (NRF) funded by the Korea government (MEST) (No. NRF-2014S1A2A2028636, NRF- 2015R1D1A1A01056918, NRF-2016K1A3A7A09005579, and NRF-2016R1A5A1013277), and the Natural Sciences and Engineering Council of Canada. Publisher Copyright: {\textcopyright} 2018 Author(s).; 14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017 ; Conference date: 27-06-2017 Through 30-06-2017",
year = "2018",
month = apr,
day = "25",
doi = "10.1063/1.5030807",
language = "English",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics Inc.",
editor = "Hahn, {Kevin Insik} and Lee, {Young Sun} and Sunchan Jeong and Kim, {Sang Chul} and Myung-Ki Cheoun and Kyujin Kwak and Sung-Chul Yoon",
booktitle = "14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017",
}