NSR Query Results


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NSR database version of March 21, 2024.

Search: Author = E.Napolitani

Found 6 matches.

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2021BE19      Eur.Phys.J. A 57, 177 (2021)

S.Bertoldo, G.Maggioni, W.Raniero, C.Carraro, S.Riccetto, F.Sgarbossa, D.Scarpa, A.Andrighetto, A.Mazzolari, A.Gadea, D.R.Napoli, E.Napolitani, D.De Salvador

New method for the production of thin and stable, segmented n+contacts in HPGe detectors

doi: 10.1140/epja/s10050-021-00487-8
Citations: PlumX Metrics


2018MA23      Eur.Phys.J. A 54, 34 (2018)

G.Maggioni, S.Carturan, W.Raniero, S.Riccetto, F.Sgarbossa, V.Boldrini, R.Milazzo, D.R.Napoli, D.Scarpa, A.Andrighetto, E.Napolitani, D.De Salvador

Pulsed laser diffusion of thin hole-barrier contacts in high purity germanium for gamma radiation detectors

doi: 10.1140/epja/i2018-12471-0
Citations: PlumX Metrics


2017NA09      Acta Phys.Pol. B48, 387 (2017)

D.R.Napoli, G.Maggioni, S.Carturan, J.Eberth, V.Boldrini, D.De Salvador, E.Napolitani, P.Cocconi, G.Della Mea, M.Gelain, R.Gunnella, M.G.Grimaldi, M.Loriggiola, G.Mariotto, N.Pinto, W.Raniero, S.J.Rezvani, S.Riccetto, D.Rosso, F.Sgarbossa, S.Tati

New Developments in HPGe Detectors for High Resolution Detection

doi: 10.5506/APhysPolB.48.387
Citations: PlumX Metrics


2016BE14      Eur.Phys.J. A 52, 72 (2016)

A.Best, A.Caciolli, Zs.Fulop, Gy.Gyurky, M.Laubenstein, E.Napolitani, V.Rigato, V.Roca, T.Szucs

Underground nuclear astrophysics: Why and how

doi: 10.1140/epja/i2016-16072-7
Citations: PlumX Metrics


2015BR09      Eur.Phys.J. A 51, 94 (2015)

C.G.Bruno, D.A.Scott, A.Formicola, M.Aliotta, T.Davinson, M.Anders, A.Best, D.Bemmerer, C.Broggini, A.Caciolli, F.Cavanna, P.Corvisiero, R.Depalo, A.Di Leva, Z.Elekes, Zs.Fulop, G.Gervino, C.J.Griffin, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, E.Napolitani, P.Prati, E.Somorjai, O.Straniero, F.Strieder, T.Szucs, D.Trezzi, for the LUNA Collaboration

Resonance strengths in the 17, 18O(p, α)14, 15N reactions and background suppression underground - Commissioning of a new setup for charged-particle detection at LUNA

NUCLEAR REACTIONS 17,18O(p, α), E=151, 193 keV; measured Eα, Iα; deduced resonance strength, energy, thick target yield as a by-product of commissioning of new setup.

doi: 10.1140/epja/i2015-15094-y
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2275. Data from this article have been entered in the XUNDL database. For more information, click here.


2014DI01      Phys.Rev. C 89, 015803 (2014), Erratum Phys.Rev. C 90, 019902 (2014)

A.Di Leva, D.A.Scott, A.Caciolli, A.Formicola, F.Strieder, M.Aliotta, M.Anders, D.Bemmerer, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, J.Jose, M.Junker, M.Laubenstein, R.Menegazzo, E.Napolitani, P.Prati, V.Rigato, V.Roca, E.Somorjai, C.Salvo, O.Straniero, T.Szucs, F.Terrasi, D.Trezzi

Underground study of the 17O(p, γ)18F reaction relevant for explosive hydrogen burning

NUCLEAR REACTIONS 17O(p, γ)18F, E(cm)=160-370 keV; measured Eγ, Iγ, on- and off-resonance γ spectra, γ-branching ratios from decay of resonances, half-life using activation method at underground LUNA accelerator at Gran Sasso National Laboratory; deduced S factors for secondary transitions, total S factor, resonance strength, astrophysical S factor and reaction rates. 18F; deduced levels, analysis of astrophysically important 183-keV resonance. Comparison with previous experimental results. 15N, 18,19F, 18O; evaluated abundances by Nova model calculations.

RADIOACTIVITY 18F(β+)[from 17O(p, γ), E(cm)=160-370 keV]; measured Eγ, Iγ, half-life.

doi: 10.1103/PhysRevC.89.015803
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2098. Data from this article have been entered in the XUNDL database. For more information, click here.


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