Ultra-sensitive in-beam gamma-ray spectroscopy for nuclear astrophysics at LUNA

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dc.creatorCaciolli, A.
dc.creatorAgostino, L.
dc.creatorBemmerer, D.
dc.creatorBonetti, R.
dc.creatorBroggini, C.
dc.creatorConfortola, F.
dc.creatorCorvisiero, P.
dc.creatorCostantini, H.
dc.creatorElekes, Z.
dc.creatorFormicola, A.
dc.creatorFulop, Zs.
dc.creatorGervino, G.
dc.creatorGuglielmetti, A.
dc.creatorGustavino, C.
dc.creatorGyurky, Gy.
dc.creatorImbriani, G.
dc.creatorJunker, M.
dc.creatorLaubenstein, M.
dc.creatorLemut, A.
dc.creatorLimata, B.
dc.creatorMarta, M.
dc.creatorMazzocchi, C.
dc.creatorMenegazzo, R.
dc.creatorPrati, P.
dc.creatorRoca, V.
dc.creatorRolfs, C.
dc.creatorAlvarez, C. Rossi
dc.creatorSomorjai, E.
dc.creatorStraniero, O.
dc.creatorStrieder, F.
dc.creatorTerrasi, F.
dc.creatorTrautvetter, H. P.
dc.date2008-12-17
dc.date.accessioned2026-07-07T12:37:12Z
dc.date.available2026-07-07T12:37:12Z
dc.descriptionUltra-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.
dc.descriptionaccepted, Eur. Phys. J. A
dc.identifierhttps://arxiv.org/abs/0812.3223
dc.identifierhttp://arxiv.org/abs/0812.3223
dc.identifierEur. Phys. J. A 39, 179 (2009)
dc.identifierdoi:10.1140/epja/i2008-10706-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218357
dc.subjectNuclear Experiment
dc.titleUltra-sensitive in-beam gamma-ray spectroscopy for nuclear astrophysics at LUNA
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