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NSR database version of April 27, 2024.

Search: Author = M.Gimenez Del Santo

Found 2 matches.

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2017SP04      Phys.Rev. C 95, 035801 (2017)

C.Spitaleri, S.M.R.Puglia, M.La Cognata, L.Lamia, S.Cherubini, A.Cvetinovic, G.D'Agata, M.Gulino, G.L.Guardo, I.Indelicato, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, S.Tudisco, A.Tumino, M.Gimenez Del Santo, N.Carlin, M.G.Munhoz, F.A.Souza, A.Szanto de Toledo, A.Mukhamedzhanov, C.Broggini, A.Caciolli, R.Depalo, R.Menegazzo, V.Rigato, I.Lombardo, D.Dell'Aquila

Measurement of the ¹⁰B(p, α₀)⁷Be cross section from 5 keV to 1.5 MeV in a single experiment using the Trojan horse method

NUCLEAR REACTIONS ²H(¹⁰B, α⁷Be), E=27 MeV; measured α and ⁷Be spectra using ΔE-E method at Pelletron-Linac laboratory of DFN-Sao Paulo; deduced Q-value spectrum, energy scatter plots, momentum distribution, astrophysical S(E) factors, Trojan horse method (THM) astrophysical factor, R-matrix fit of THM data ¹¹C; deduced levels, resonances, center-of-mass energies, J, π, Γ_p, Γ_α0, Γ_α1.

doi: 10.1103/PhysRevC.95.035801
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0837.

2014SP03      Phys.Rev. C 90, 035801 (2014)

C.Spitaleri, L.Lamia, S.M.R.Puglia, S.Romano, M.La Cognata, V.Crucilla, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, M.Gimenez Del Santo, N.Carlin, M.G.Munhoz, F.A.Souza, A.Szanto de Toledo, A.Tumino, B.Irgaziev, A.Mukhamedzhanov, G.Tabacaru, V.Burjan, V.Kroha, Z.Hons, J.Mrazek, S.-H.Zhou, C.Li, Q.Wen, Y.Wakabayashi, H.Yamaguchi, E.Somorjai

Measurement of the 10 keV resonance in the ¹⁰B(p, α₀)⁷Be reaction via the Trojan Horse method

NUCLEAR REACTIONS ²H(¹⁰B, α⁷Be), E=24.5 MeV; measured particle spectra by ΔE-E method using ionization chambers and position-sensitive detectors at LNS-Catania accelerator facility; analyzed data by Trojan Horse method (THM); deduced E_α-Be and E_α-n two-dimensional plots, experimental momentum distribution and its comparison with DWBA and PWIA calculations, THM bare nucleus astrophysical S(E) factors using R-matrix formalism for 5-100 keV resonances in ¹¹C, dominated by 10-keV resonance corresponding to 8699-keV, 5/2+ level in ¹¹C. ¹¹C; deduced widths of three resonances.

doi: 10.1103/PhysRevC.90.035801
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1765. Data from this article have been entered in the XUNDL database. For more information, click here.