Abstract

This paper outlines the new physics possibilities that fall within the field of nuclear structure and astrophysics based on experiments with radioactive ion beams at the future Rare Isotope Beams Accelerator facility in Korea. This ambitious multi-beam facility has both an Isotope Separation On Line (ISOL) and fragmentation capability to produce rare isotopes beams (RIBs) and will be capable of producing and accelerating beams of wide range mass of nuclides with energies of a few to hundreds MeV per nucleon. The large dynamic range of reaccelerated RIBs will allow the optimization in each nuclear reaction case with respect to cross section and channel opening. The low energy RIBs around Coulomb barrier offer nuclear reactions such as elastic resonance scatterings, one or two particle transfers, Coulomb multiple-excitations, fusion-evaporations, and direct capture reactions for the study of the very neutron-rich and proton-rich nuclides. In contrast, the high energy RIBs produced by in-flight fragmentation with reaccelerated ions from the ISOL enable to explore the study of neutron drip lines in intermediate mass regions. The proposed studies aim at investigating the exotic nuclei near and beyond the nucleon drip lines, and to explore how nuclear many-body systems change in such extreme regions by addressing the following topics: the evolution of shell structure in areas of extreme proton to neutron imbalance; the study of the weak interaction in exotic decay schemes such as beta-delayed two-neutron or two-proton emission; the change of isospin symmetry in isobaric mirror nuclei at the drip lines; two protons or two neutrons radioactivity beyond the drip lines; the role of the continuum states including resonant states above the particle-decay threshold in exotic nuclei; and the effects of nuclear reaction rates triggered by the unbound proton-rich nuclei on nuclear astrophysical processes.

Highlights

  • C Author(s) 2014041001-2 Chang-Bum MoonAIP Advances 4, 041001 (2014)20:00, August 15, 2013

  • The proposed studies aim at investigating the exotic nuclei near and beyond the nucleon drip lines, and to explore how nuclear many-body systems change in such extreme regions by addressing the following topics: the evolution of shell structure in areas of extreme proton to neutron imbalance; the study of the weak interaction in exotic decay schemes such as beta-delayed two-neutron or two-proton emission; the change of isospin symmetry in isobaric mirror nuclei at the drip lines; two protons or two neutrons radioactivity beyond the drip lines; the role of the continuum states including resonant states above the particle-decay threshold in exotic nuclei; and the effects of nuclear reaction rates triggered by the unbound proton-rich nuclei on nuclear astrophysical processes

  • We have introduced and discussed the planned experiments using rare isotopes beams (RIBs) for the Korean Rare Isotope Beams Accelerator facility

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Summary

INTRODUCTION

The explosive stellar events as novae, x-ray bursters, and supernovae are controlled by the properties of such short-lived radioactive nuclei.[2] the understanding of the nuclear structure plays a key role in establishing the nuclear reaction rates, their mechanisms, and the origin of energy in hot stars and during their explosions. The question of how shell structure develops in the finite quantum manybody systems has been a common problem among various disciplines such as nuclear physics, atomic physics, condensed matter physics, molecular physics, and biophysics. The future of nuclear physics depends to a large extent on the planning of the new facilities In this respect, the Korean Rare Isotope Beams Accelerator facility (here after called KRIA) stands on the heart of the future of nuclear physics in the world. This report aims to develop a concrete nuclear physics program at the KRIA facility with a goal for exploring new areas of the nuclei and the extreme areas of astrophysical nuclear reaction processes

NUCLEAR PHYSICS WITH RARE ISOTOPE BEAMS
He 3 4
AN OVERVIEW OF THE SHELL STRUCTURE EVOLUTION
Experiments at IFFS using
THE CHARACTERISTICS OF THE KRIA FACILITY
AN OVERVIEW OF NUCLEAR EXPERIMENTS
14 Si 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 32
THE PLANNED EXPERIMENTS
16 F 19 Na 21 Al 30 Cl 38 Sc 39 Sc 42 V 59 Ga 63 As 69 Bra 73 Rb
40 Ca 9Be 28S
40 Ca 9Be
SUMMARY AND OUTLOOK
Notes added
Full Text
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