An actively vetoed Clover gamma-detector for nuclear astrophysics at LUNA
arXiv:1003.6072 · doi:10.1140/epja/i2010-10967-1
Abstract
An escape-suppressed, composite high-purity germanium detector of the Clover type has been installed at the Laboratory for Underground Nuclear Astrophysics (LUNA) facility, deep underground in the Gran Sasso Laboratory, Italy. The laboratory gamma-ray background of the Clover detector has been studied underground at LUNA and, for comparison, also in an overground laboratory. Spectra have been recorded both for the single segments and for the virtual detector formed by online addition of all four segments. The effect of the escape-suppression shield has been studied as well. Despite their generally higher intrinsic background, escape-suppressed detectors are found to be well suited for underground nuclear astrophysics studies. As an example for the advantage of using a composite detector deep underground, the weak ground state branching of the Ep = 223 keV resonance in the 24Mg(p,gamma)25Al reaction is determined with improved precision.
arXiv comment8 pages, 6 figures, 3 tables; as accepted by Eur. Phys. J. A
References in corpus (12)
- New Solar Composition: The Problem With Solar Models Revisited
- S-factor of 14N(p,gamma)15O at astrophysical energies
- The solar chemical composition
- First Measurement of the He3+He3-->He4+2p Cross Section down to the Lower Edge of the Solar Gamow Peak
- Activation measurement of the 3He(alpha,gamma)7Be cross section at low energy
- Astrophysical S-factor of the 3He(alpha,gamma)7Be reaction measured at low energy via prompt and delayed gamma detection
- First measurement of the 14N(p,gamma)15O cross section down to 70 keV
- LUNA: a Laboratory for Underground Nuclear Astrophysics
- Precision study of ground state capture in the 14N(p,gamma)15O reaction
- Ultra-sensitive in-beam gamma-ray spectroscopy for nuclear astrophysics at LUNA
- Feasibility of low energy radiative capture experiments at the LUNA underground accelerator facility
- Direct measurement of the 15N(p,gamma)16O total cross section at novae energies
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- A new study of the Ne(p,)Na reaction deep underground: Feasibility, setup, and first observation of the 186 keV resonance
- Underground nuclear astrophysics: why and how
- Neutron-induced background by an alpha-beam incident on a deuterium gas target and its implications for the study of the 2H(alpha,gamma)6Li reaction at LUNA
- New proton-capture rates on carbon isotopes and their impact on the astrophysical ratio
- Background in -ray detectors and carbon beam tests in the Felsenkeller shallow-underground accelerator laboratory
- Cosmic-ray induced background intercomparison with actively shielded HPGe detectors at underground locations
- The Felsenkeller shallow-underground laboratory for nuclear astrophysics
- Progress of the Felsenkeller shallow-underground accelerator for nuclear astrophysics
- Study of the Ne()Na reaction at LUNA