Imbriani, Gianluca and Limata, Benedicta Norman and Roca, Vincenzo (2009) Ultra-sensitive in-beam g-ray spectroscopy for nuclear astrophysics at LUNA. [Pubblicazione in rivista scientifica]

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Tipologia del documento: Pubblicazione in rivista scientifica
Lingua: English
Titolo: Ultra-sensitive in-beam g-ray spectroscopy for nuclear astrophysics at LUNA
Autori:
AutoreEmail
Imbriani, Gianluca[non definito]
Limata, Benedicta Norman[non definito]
Roca, Vincenzo[non definito]
Autore/i: A. Caciolli, L. Agostino, D. Bemmerer, R. Bonetti, C. Broggini, F. Confortola, P. Corvisiero, H. Costantini, Z. Elekes, A. Formicola, Zs. F¨ul¨op, G. Gervino, A. Guglielmetti, C. Gustavino, Gy. Gy¨urky, G. Imbriani, M. Junker, M. Laubenstein, A. Lemut, B.
Data: 2009
Numero di pagine: 8
Dipartimento: Scienze fisiche
Numero identificativo: 10.1140/epja/i2008-10706-3
Titolo del periodico: THE EUROPEAN PHYSICAL JOURNAL. A, HADRONS AND NUCLEI
Data: 2009
Volume: 39
Intervallo di pagine: pp. 179-186
Numero di pagine: 8
Parole chiave: Radiative capture, 3H-, 3He-, and 4He-induced reactions – Electrostatic accelerators, X- and g-ray spectroscopy
Numero identificativo: 10.1140/epja/i2008-10706-3
Depositato il: 21 Ott 2010 06:56
Ultima modifica: 30 Apr 2014 19:43
URI: http://www.fedoa.unina.it/id/eprint/7366

Abstract

Ultra-sensitive in-beam -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 gray background for Eg < 3 MeV at LUNA has been reduced to levels comparable to those experienced in dedicated offline underground g-counting setups. The g-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.

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