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NSR database version of April 27, 2024.

Search: Author = L.Roberti

Found 3 matches.

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2024BO09      Universe 10, 148 (2024)

L.Boccioli, L.Roberti

The Physics of Core-Collapse Supernovae: Explosion Mechanism and Explosive Nucleosynthesis

doi: 10.3390/universe10030148
Citations: PlumX Metrics


2021CH38      Astrophys.J. 916, 79 (2021)

A.Chieffi, L.Roberti, M.Limongi, M.La Cognata, L.Lamia, S.Palmerini, R.G.Pizzone, R.Sparta, A.Tumino

Impact of the New Measurement of the 12C + 12C Fusion Cross Section on the Final Compactness of Massive Stars

NUCLEAR REACTIONS 12C(12C, X)24Mg, E<1 MeV; analyzed available data; deduced impact on the dependence of the compactness on the initial mass with respect to previous findings by adopting the classical cross section.

doi: 10.3847/1538-4357/ac06ca
Citations: PlumX Metrics


2021TE06      Phys.Rev. C 104, 015806 (2021)

M.Tessler, J.Zappala, S.Cristallo, L.Roberti, M.Paul, S.Halfon, T.Heftrich, W.Jiang, D.Kijel, A.Kreisel, M.Limongi, Z.-T.Lu, P.Muller, R.Purtschert, R.Reifarth, A.Shor, D.Veltum, D.Vescovi, M.Weigand, L.Weissman

Stellar s-process neutron capture cross sections on 78, 80, 84, 86Kr determined via activation, atom trap trace analysis, and decay counting

NUCLEAR REACTIONS 78,80,84,86Kr(n, γ)79Kr/79mKr/80Kr/81Kr/81mKr/84Kr/85Kr/85mKr/87Kr, kT=42.5 keV, quasi-Maxwellian; 80,86Kr(γ, n)79Kr/85mKr, E=14.6, 17.6 MeV; measured Eγ, Iγ, average σ(E), 81Kr/80Kr and 85Kr/84Kr isotopic ratios in (n, γ) reactions by activation method, Atom Trap Trace Analysis (ATTA) and decay counting at SARAF-LiLiT facility, Argonne National Laboratory and low-level counting (LLC) facility of the University of Bern; deduced Maxwellian-averaged cross sections (MACS) at kt=3-300 keV, and stellar reaction rates for s-process in 0.01-4 GK range for (n, γ) reactions. 197Au(n, γ)198Au, kT=42.5 keV; 197Au(γ, n)196Au, E=14.6, 17.6 MeV; measured Eγ, Iγ, used as monitor reactions. Comparison with previous experimental cross sections, and with data in JEFF-3.3 library. Discussed astrophysical implications, and impact on s-process calculations of abundances of krypton and neighboring nuclides.

RADIOACTIVITY 79Kr(EC); 85mKr(IT); 85mKr, 87Kr(β-)[from 78,84,86Kr(n, γ), kT=42.5 keV]; measured half-lives from γ-decay curves and compared with evaluated data.

doi: 10.1103/PhysRevC.104.015806
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset31837. Data from this article have been entered in the XUNDL database. For more information, click here.


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