NSR Query Results
Output year order : Descending NSR database version of April 29, 2024. Search: Author = R.Mancino Found 4 matches. 2022CO04 Phys.Rev. C 105, 034312 (2022) L.Coraggio, N.Itaco, G.De Gregorio, A.Gargano, R.Mancino, F.Nowacki Shell-model calculation of 100Mo double -β decay NUCLEAR STRUCTURE 100Mo; calculated neutron effective single-particle, proton and neutron single-particle energy spacings, running sum of B(GT) strength up to 3 MeV. 100Mo, 100Ru; calculated levels, J, π, B(E2). Effective shell-model Hamiltonian with realistic nucleon-nucleon potential. Comparison to experimental data. RADIOACTIVITY 100Mo(2β-); calculated nuclear matrix elements for double β-decay and neutrinoless double β-decay to yrare and yrast 0+ states in 100Ru. Effective shell-model Hamiltonian with realistic nucleon-nucleon potential and decay operators derived within the many-body perturbation theory. Comparison to available experimental data and other theoretical predictions.
doi: 10.1103/PhysRevC.105.034312
2022SI17 Phys.Rev. C 106, 015803 (2022) A.Sieverding, J.S.Randhawa, D.Zetterberg, R.J.deBoer, T.Ahn, R.Mancino, G.Martinez-Pinedo, W.R.Hix Role of low-lying resonances for the 10Be(p, α)7Li reaction rate and implications for the formation of the Solar System NUCLEAR REACTIONS 10Be(p, α), (α, n), E not given; 10Be(ν, e-), E=2.8-10 MeV; analyzed reaction rates, σ; deduced influence on the content of 10Be in supernovae environment. 10Be(p, α), E<1.5 MeV; analyzed reaction rate, experimental data on resonance in 11B at 193 keV, ; deduced reaction rate, astrophysical S-factor. Showed that, with the new reaction rate, a low-mass corecollapse supernovae is unlikely to produce enough 10Be to explain the observed 10Be/9Be ratio in meteorites. Comparison to data from JINA-REACLIB.
doi: 10.1103/PhysRevC.106.015803
2020CO05 Phys.Rev. C 101, 044315 (2020) L.Coraggio, A.Gargano, N.Itaco, R.Mancino, F.Nowacki Calculation of the neutrinoless double-β decay matrix element within the realistic shell model RADIOACTIVITY 48Ca, 76Ge, 82Se, 130Te, 136Xe(2β-); calculated nuclear matrix element, and neutron pair contributions to nuclear matrix element of 0νββ decay using shell model with realistic nucleon-nucleon potential. Comparison with other theoretical calculations.
doi: 10.1103/PhysRevC.101.044315
2020CO16 Universe 6, 233 (2020) L.Coraggio, N.Itaco, G.De Gregorio, A.Gargano, R.Mancino, S.Pastore Present Status of Nuclear Shell-Model Calculations of 0νββ Decay Matrix Elements
doi: 10.3390/universe6120233
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