Overview of the KoRIA Facility for Rare Isotope Beams

Title
Overview of the KoRIA Facility for Rare Isotope Beams
Authors
J.K. AhnB.H. ChoiS.H. HwangS.H. KimC.H. LeeH.S. LeeJ.Y. ParkS.Y. RyuI.-K. YooS.Y. YuS.I. BakJ.-S. ChaiH.J. ChoiJang Min HanS.-W. HongD. JeongY. KadiD.Y. KimJ.T. KimB.N. LeeS.D. LeeV.K. ManchandaJ.H. OhJ.A. ParkT.-S. ParkH. SakaiJ.W. ShinS.W. ShinH.S. SongC. TenreiroZ. TongY.K. YangY.H. YeonY. BlumenfeldB.-G. CheonC. I. ChoiD. Y. JangB. H. KangY. K. KimM. S. RyuM.-K. CheounE. J. HaC. Y. RyuD. ChoB. HongG. JhangE. JooKyong Sei LeeK. S. SimY. S. ChoJ. H. HaJae Min HanI. G. KimC. W. LeeY.-O. LeeB. H. OhS. H. ParkT. Y. SongE. M. ChoiM. S. ChoiS. K. LeeS. ChoiT. K. ChoiY. S. ChoiD. L. KimK. H. ChungD. U. KimS. K. KoK. O. LeeY. Y. LeeW. NamkungH. J. SeoW. J. YiI. S. HahnA. KimW. HongG. D. Kim김준곤H. J. WooC. H. HyunJ. JangS. KimH.-R. YangD. JeonS.-H. KimS.-C. JeongH. S. KangE. J. KimH.-Ch. KimJ. W. KimW. KimY. OhM. KwonY. K. KwonC. S. LeeJ. H. LeeC. C. YunB. Y. LeeH. J. LeeY. S. LeeW.-Y. ParkH.-S. LeeK. H. ParkKang Seog LeeS. D. LeeS. H. LeeV. K. ManchandaC. B. MoonS. NamB. G. YuJ. A. NolenB. Y. ParkH. SakaiY. YanoP. SiggW. Y. SoB. J. SuhC. TenreiroR. E. TribbleD. H. Yu
Issue Date
2013-03
Publisher
Few-body systems
Citation
VOL 54, NO 1-4, 197-204
Abstract
The Korea Rare Isotope Accelerator, currently referred to as KoRIA, is briefly presented. The KoRIA facility is aimed to enable cutting-edge sciences in a wide range of fields. It consists of a 70 kW isotope separator on-line (ISOL) facility driven by a 70 MeV, 1 mA proton cyclotron and a 400 kW in-flight fragmentation (IFF) facility. The ISOL facility uses a superconducting (SC) linac for post-acceleration of rare isotopes up to about 18 MeV/u, while the SC linac of IFF facility is capable of accelerating uranium beams up to 200 MeV/u, 8 pμA and proton beams up to 600 MeV, 660 μA. Overall features of the KoRIA facility are presented with a focus on the accelerator design.
URI
https://pubs.kist.re.kr/handle/201004/44654
ISSN
01777963
Appears in Collections:
KIST Publication > Article
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