The Texas–Edinburgh–Catania Silicon Array (TECSA): A detector for nuclear astrophysics and nuclear structure studies with rare isotope beams

2011 ◽  
Vol 634 (1) ◽  
pp. 71-76 ◽  
Author(s):  
B.T. Roeder ◽  
M. McCleskey ◽  
L. Trache ◽  
A.A. Alharbi ◽  
A. Banu ◽  
...  
Keyword(s):  
Nuclear Structure ◽  
Nuclear Astrophysics ◽  
Rare Isotope

scholarly journals Nuclear theory and science of the facility for rare isotope beams

2014 ◽  
Vol 29 (11) ◽  
pp. 1430010 ◽  
Author(s):  
A. B. Balantekin ◽  
J. Carlson ◽  
D. J. Dean ◽  
G. M. Fuller ◽  
R. J. Furnstahl ◽  
...  
Keyword(s):  
Nuclear Structure ◽  
Critical Role ◽  
Nuclear Astrophysics ◽  
Current Theory ◽  
Comprehensive Description ◽  
Rare Isotope ◽  
Nuclear Theory ◽  
Nuclear Science ◽  
Traditional Fields ◽  
Rare Isotopes

The Facility for Rare Isotope Beams (FRIB) will be a world-leading laboratory for the study of nuclear structure, reactions and astrophysics. Experiments with intense beams of rare isotopes produced at FRIB will guide us toward a comprehensive description of nuclei, elucidate the origin of the elements in the cosmos, help provide an understanding of matter in neutron stars and establish the scientific foundation for innovative applications of nuclear science to society. FRIB will be essential for gaining access to key regions of the nuclear chart, where the measured nuclear properties will challenge established concepts, and highlight shortcomings and needed modifications to current theory. Conversely, nuclear theory will play a critical role in providing the intellectual framework for the science at FRIB, and will provide invaluable guidance to FRIB's experimental programs. This review overviews the broad scope of the FRIB theory effort, which reaches beyond the traditional fields of nuclear structure and reactions, and nuclear astrophysics, to explore exciting interdisciplinary boundaries with other areas.

Nuclear structure far off stability —Implications for nuclear astrophysics

2010 ◽  
pp. 257-267
Author(s):  
H. Grawe ◽  
A. Blazhev ◽  
M. Górska ◽  
R. Grzywacz ◽  
H. Mach ◽  
...  
Keyword(s):  
Nuclear Structure ◽  
Nuclear Astrophysics

Nuclear structure aspects in nuclear astrophysics

2005 ◽  
Vol 54 (2) ◽  
pp. 535-613 ◽  
Author(s):  
A APRAHAMIAN ◽  
K LANGANKE ◽  
M WIESCHER
Keyword(s):  
Nuclear Structure ◽  
Nuclear Astrophysics

scholarly journals Simulation Study for the Separation of Rare Isotopes at the Seoul National University AMS Facility

Radiocarbon ◽  
2004 ◽  
Vol 46 (1) ◽  
pp. 89-95 ◽  
Author(s):  
C C Yun ◽  
C S Lee ◽  
M Youn ◽  
J C Kim
Keyword(s):  
Simulation Study ◽  
Isotope Separation ◽  
Nuclear Astrophysics ◽  
Small Mass ◽  
Beam Line ◽  
Rare Isotope ◽  
Transport Code ◽  
National University ◽  
Rare Isotopes ◽  
Seoul National University

A simulation study for the separation of rare isotopes such as beryllium and aluminum was performed for a new beam line to be attached to the 3MV Tandetron accelerator at the accelerator mass spectrometry (AMS) facility of Seoul National University in Korea. The new beam line will also be used for other scientific applications, namely, ion implantations, Rutherford backscattering, and nuclear astrophysics experiments. It mainly consists of 30° and 100° deflection dipole magnets and drift spaces. A transfer matrix for the beam line was determined by the TRANSPORT code. Simulation of the rare isotope separation was performed by a ray tracing method using the TURTLE code. The simulation results, including the effect of the energy degrader, provide feasibility for the separation of isobars with small mass differences in 10Be-10B and 26Al-26Mg.

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