Ultra-sensitive in-beam gamma-ray spectroscopy for nuclear astrophysics at LUNA
arXiv:0812.3223 · doi:10.1140/epja/i2008-10706-3
Abstract
Ultra-sensitive in-beam gamma-ray spectroscopy studies for nuclear astrophysics are performed at the LUNA (Laboratory for Underground Nuclear Astrophysics) 400 kV accelerator, deep underground in Italy's Gran Sasso laboratory. By virtue of a specially constructed passive shield, the laboratory gamma-ray background for E_γ< 3 MeV at LUNA has been reduced to levels comparable to those experienced in dedicated offline underground gamma-counting setups. The gamma-ray background induced by an incident alpha-beam has been studied. The data are used to evaluate the feasibility of sensitive in-beam experiments at LUNA and, by extension, at similar proposed facilities.
accepted, Eur. Phys. J. A
References in corpus (9)
- Study of the 12C+12C fusion reactions near the Gamow energy
- 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
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Cited by in corpus (14)
- LUNA: Nuclear Astrophysics Deep Underground
- LUNA: Status and Prospects
- The 14N(p,gamma)15O reaction studied with a composite germanium detector
- A new study of the Ne(p,)Na reaction deep underground: Feasibility, setup, and first observation of the 186 keV resonance
- Direct measurement of the 15N(p,gamma)16O total cross section at novae energies
- An actively vetoed Clover gamma-detector for nuclear astrophysics at LUNA
- 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
- The study of key reactions shaping the post main-sequence evolution of massive stars in underground facilities
- Experimental determination of the He(,)Be reaction cross section above the Be proton separation threshold
- First direct measurement of the 64.5 keV resonance strength in O(p,)F reaction
- Energy Acceptance of the St. George Recoil Separator
- A new study of Mg(,n)Si angular distributions at = 3 - 5 MeV
- Progress of the Felsenkeller shallow-underground accelerator for nuclear astrophysics
- Study of the Ne()Na reaction at LUNA