NSR Query Results

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NSR database version of April 11, 2024.

Search: Author = D.A.Scott

Found 10 matches.

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2018BE17      Europhys.Lett. 122, 52001 (2018)

D.Bemmerer, F.Cavanna, R.Depalo, M.Aliotta, M.Anders, A.Boeltzig, C.Broggini, C.Bruno, A.Caciolli, T.Chillery, P.Corvisiero, T.Davinson, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, R.Menegazzo, V.Mossa, F.R.Pantaleo, P.Prati, D.A.Scott, K.Stocker, O.Straniero, T.Szucs, M.P.Takacs, D.Trezzi

Effect of beam energy straggling on resonant yield in thin gas targets: The cases ²²Ne(p, γ)²³Na and ¹⁴N(p, γ)¹⁵O

NUCLEAR REACTIONS ²²Ne, ¹⁴N(p, γ), E<300 keV; analyzed available data; deduced correction for narrow resonance yields.

doi: 10.1209/0295-5075/122/52001
Citations: PlumX Metrics

2017TR01      Astropart.Phys. 89, 57 (2017)

D.Trezzi, M.Anders, M.Aliotta, A.Bellini, D.Bemmerer, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, P.Corvisiero, H.Costantini, T.Davinson, R.Depalo, Z.Elekes, M.Erhard, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, V.Mossa, F.Pantaleo, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, T.Szucs, M.Takacs

Big Bang ⁶Li nucleosynthesis studied deep underground (LUNA collaboration)

NUCLEAR REACTIONS ²H(α, γ), E(cm)=80, 93, 120, 133 keV; measured reaction products, Eγ, Iγ; deduced σ, S-factor, thermonuclear reaction rates. Comparison with available data.

doi: 10.1016/j.astropartphys.2017.01.007
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, 18}O(p, α)^{14, 15}N 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.

2015CA27      Phys.Rev.Lett. 115, 252501 (2015); Erratum Phys.Rev.Lett. 120, 239901 (2018)

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

Three New Low-Energy Resonances in the ²²Ne(p, γ)²³Na Reaction

NUCLEAR REACTIONS ^20,21,22Ne(p, γ), E=70-300 keV; measured reaction products, Eγ, Iγ; deduced resonance energies and strengths, thermonuclear reaction rates. Comparison with available data.

doi: 10.1103/PhysRevLett.115.252501
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4330. Data from this article have been entered in the XUNDL database. For more information, click here.

2014AN05      Phys.Rev.Lett. 113, 042501 (2014)

M.Anders, D.Trezzi, R.Menegazzo, M.Aliotta, A.Bellini, D.Bemmerer, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, T.Davinson, Z.Elekes, M.Erhard, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, T.Szucs, for the LUNA Collaboration

First Direct Measurement of the ²H(α, γ)⁶Li Cross Section at Big Bang Energies and the Primordial Lithium Problem

NUCLEAR REACTIONS ²H(α, γ), E=400 keV; measured reaction products, Eγ, Iγ; deduced S-factor, σ. Comparison with available data.

doi: 10.1103/PhysRevLett.113.042501
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2188.

2014CA47      Eur.Phys.J. A 50, 179 (2014)

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

A new study of the ²²Ne(p, γ)²³Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance

NUCLEAR REACTIONS ²²Ne(p, γ), E=120-400 keV; measured Eγ, Iγ at LUNA. ²³Na deduced γ transitions, 186 keV resonance.

doi: 10.1140/epja/i2014-14179-5
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2237. 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.

2014FO06      Nucl.Instrum.Methods Phys.Res. A742, 258 (2014)

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

Cross-section measurements at astrophysically relevant energies: The LUNA experiment

NUCLEAR REACTIONS ¹⁷O(p, γ), E(cm)=183 keV; measured reaction products, Eγ, Iγ; deduced σ, resonance strength, S-factor. Comparison with available data.

doi: 10.1016/j.nima.2013.11.082
Citations: PlumX Metrics

2013SC27      Nucl.Instrum.Methods Phys.Res. A718, 481 (2013)

D.A.Scott, C.Bruno, A.Caciolli

¹⁷O(p, α)¹⁴N study at the LUNA accelerator

NUCLEAR REACTIONS ¹⁷O(p, α), E=70 keV; analyzed sensitivity for the 193 keV resonance, tested detectors and Al foils. Comparison with GEANT4 simulations.

doi: 10.1016/j.nima.2012.11.079
Citations: PlumX Metrics
Data from this article have been entered in the XUNDL database. For more information, click here.

2012SC16      Phys.Rev.Lett. 109, 202501 (2012)

D.A.Scott, for the LUNA Collaboration

First Direct Measurement of the ¹⁷O(p, γ)¹⁸F Reaction Cross Section at Gamow Energies for Classical Novae

NUCLEAR REACTIONS ¹⁷O(p, γ), E(cm)=200-400 keV; measured reaction products, Eγ, Iγ; deduced S-factors, σ, reaction rates. Comparison with calculations.

doi: 10.1103/PhysRevLett.109.202501
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.