TY - CONF
T1 - SECAR
T2 - 16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021
AU - Tsintari, Pelagia
AU - Garg, Ruchi
AU - Berg, Georg
AU - Blackmon, Jeff
AU - Chipps, Kelly
AU - Couder, Manoel
AU - Deibel, Catherine
AU - Dimitrakopoulos, Nikolaos
AU - Greife, Uwe
AU - Hood, Ashley
AU - Jain, Rahul
AU - Marshall, Caleb
AU - Meisel, Zach
AU - Miskovich, Sara
AU - Montes, Fernando
AU - Perdikakis, Georgios
AU - Ruland, Thomas
AU - Schatz, Hendrik
AU - Setoodehnia, Kiana
AU - Smith, Michael
AU - Wagner, Louis
N1 - Publisher Copyright:
© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
PY - 2022/2/24
Y1 - 2022/2/24
N2 - Proton- and alpha-capture reactions on unstable proton-rich nuclei power astrophysical explosions like novae and X-ray bursts. Direct measurements of these reactions are crucial for understanding the mechanisms behind these explosions and the nucleosynthesis at such sites. The recoil mass separator, SECAR (SEparator for CApture Reactions) at the National Superconducting Cyclotron Laboratory (NSCL) and the Facility for Rare Isotope Beams (FRIB), has been designed with the required sensitivity to study (p,γ) and (α,γ) reactions, directly at astrophysical energies in inverse kinematics, with radioactive beams of masses up to about A = 65. The complete SECAR system, including two Wien Filters for high mass resolution, has been installed at Michigan State University and is currently being commissioned. The present article introduces the SECAR concept, its scientific goals, and provides an update of the current status of the project.
AB - Proton- and alpha-capture reactions on unstable proton-rich nuclei power astrophysical explosions like novae and X-ray bursts. Direct measurements of these reactions are crucial for understanding the mechanisms behind these explosions and the nucleosynthesis at such sites. The recoil mass separator, SECAR (SEparator for CApture Reactions) at the National Superconducting Cyclotron Laboratory (NSCL) and the Facility for Rare Isotope Beams (FRIB), has been designed with the required sensitivity to study (p,γ) and (α,γ) reactions, directly at astrophysical energies in inverse kinematics, with radioactive beams of masses up to about A = 65. The complete SECAR system, including two Wien Filters for high mass resolution, has been installed at Michigan State University and is currently being commissioned. The present article introduces the SECAR concept, its scientific goals, and provides an update of the current status of the project.
UR - http://www.scopus.com/inward/record.url?scp=85183876409&partnerID=8YFLogxK
U2 - 10.1051/epjconf/202226011044
DO - 10.1051/epjconf/202226011044
M3 - Paper
AN - SCOPUS:85183876409
Y2 - 21 September 2021 through 25 September 2021
ER -