SECAR: A recoil separator for nuclear astrophysics

Pelagia Tsintari, Ruchi Garg, Georg Berg, Jeff Blackmon, Kelly Chipps, Manoel Couder, Catherine Deibel, Nikolaos Dimitrakopoulos, Uwe Greife, Ashley Hood, Rahul Jain, Caleb Marshall, Zach Meisel, Sara Miskovich, Fernando Montes, Georgios Perdikakis, Thomas Ruland, Hendrik Schatz, Kiana Setoodehnia, Michael SmithLouis Wagner

Research output: Contribution to conferencePaperpeer-review

1 Scopus citations

Abstract

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.

Original languageEnglish
DOIs
StatePublished - Feb 24 2022
Event16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 - Chengdu, China
Duration: Sep 21 2021Sep 25 2021

Conference

Conference16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021
Country/TerritoryChina
CityChengdu
Period09/21/2109/25/21

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