Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facility

Thermonuclear reaction cross sections of astrophysical interest decrease exponentially with energy, approaching the level of femtobarn or less at the Gamow window. Experimental investigations of such small reaction rates in laboratories at the earth’s surface are hampered by the cosmic-ray backgroun...

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Main Authors: A. Lemut, M. Couder, D. Winklehner, U. Greife, A. Hodgkinson, D. Leitner, M. Leitner, J. S. Saba, P. A. Vetter, W. L. Waldron, M. Wiescher
Format: Article
Language:English
Published: American Physical Society 2011-10-01
Series:Physical Review Special Topics. Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevSTAB.14.100101
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spelling doaj-6dc41eec23774618a8fb0ef2881b42602020-11-25T00:11:01ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022011-10-01141010010110.1103/PhysRevSTAB.14.100101Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facilityA. LemutM. CouderD. WinklehnerU. GreifeA. HodgkinsonD. LeitnerM. LeitnerJ. S. SabaP. A. VetterW. L. WaldronM. WiescherThermonuclear reaction cross sections of astrophysical interest decrease exponentially with energy, approaching the level of femtobarn or less at the Gamow window. Experimental investigations of such small reaction rates in laboratories at the earth’s surface are hampered by the cosmic-ray background into detectors. For such studies, Dakota Ion Accelerator for Nuclear Astrophysics, a deep underground, high detector efficiency, high target density, high beam intensity accelerator facility is being designed. We report on a 100 mA, 400 kV accelerator design. To take into account the beam space-charge effects, advanced three-dimensional transportation calculations have been performed. These highly realistic beam calculations demonstrate that high beam currents can be transported to a gas-jet target with a diameter of few millimeters.http://doi.org/10.1103/PhysRevSTAB.14.100101
collection DOAJ
language English
format Article
sources DOAJ
author A. Lemut
M. Couder
D. Winklehner
U. Greife
A. Hodgkinson
D. Leitner
M. Leitner
J. S. Saba
P. A. Vetter
W. L. Waldron
M. Wiescher
spellingShingle A. Lemut
M. Couder
D. Winklehner
U. Greife
A. Hodgkinson
D. Leitner
M. Leitner
J. S. Saba
P. A. Vetter
W. L. Waldron
M. Wiescher
Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facility
Physical Review Special Topics. Accelerators and Beams
author_facet A. Lemut
M. Couder
D. Winklehner
U. Greife
A. Hodgkinson
D. Leitner
M. Leitner
J. S. Saba
P. A. Vetter
W. L. Waldron
M. Wiescher
author_sort A. Lemut
title Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facility
title_short Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facility
title_full Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facility
title_fullStr Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facility
title_full_unstemmed Design of a 400 kV deep underground, high detector efficiency, high target density, high beam intensity accelerator facility
title_sort design of a 400 kv deep underground, high detector efficiency, high target density, high beam intensity accelerator facility
publisher American Physical Society
series Physical Review Special Topics. Accelerators and Beams
issn 1098-4402
publishDate 2011-10-01
description Thermonuclear reaction cross sections of astrophysical interest decrease exponentially with energy, approaching the level of femtobarn or less at the Gamow window. Experimental investigations of such small reaction rates in laboratories at the earth’s surface are hampered by the cosmic-ray background into detectors. For such studies, Dakota Ion Accelerator for Nuclear Astrophysics, a deep underground, high detector efficiency, high target density, high beam intensity accelerator facility is being designed. We report on a 100 mA, 400 kV accelerator design. To take into account the beam space-charge effects, advanced three-dimensional transportation calculations have been performed. These highly realistic beam calculations demonstrate that high beam currents can be transported to a gas-jet target with a diameter of few millimeters.
url http://doi.org/10.1103/PhysRevSTAB.14.100101
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