NSR Query Results


Output year order : Descending
Format : Normal

NSR database version of April 11, 2024.

Search: Author = R.Mucciola

Found 4 matches.

Back to query form



2022GE08      Universe 8, 255 (2022)

G.Gervino, O.Aberle, A.-P.Bernardes, N.Colonna, S.Cristallo, M.Diakaki, S.Fiore, A.Manna, C.Massimi, P.Mastinu, A.Mengoni, R.Mucciola, E.Musacchio Gonzalez, N.Patronis, E.Stamati, P.Vaz, R.Vlastou

NEAR: A New Station to Study Neutron-Induced Reactions of Astrophysical Interest at CERN-n_TOF

NUCLEAR REACTIONS 64Ni, 88,89,90Sr, 89Y, 94Zr, 135,136Cs(n, γ), E=5-30, 15-90 keV; reviewed planned and conceptualized experiments for measurements of cross sections and Maxwellian Averaged Cross Section (MACS) at different temperatures relevant to s-process in AGB stars and s-process in massive stars at the new NEAR irradiation center and activation laboratory close to the CERN-n_TOF neutron source.

doi: 10.3390/universe8050255
Citations: PlumX Metrics


2022MU17      Nucl.Instrum.Methods Phys.Res. B531, 100 (2022)

R.Mucciola, C.Paradela, G.Alaerts, S.Kopecky, C.Massimi, A.Moens, P.Schillebeeckx, R.Wynants

Evaluation of resonance parameters for neutron interactions with molybdenum

NUCLEAR REACTIONS 92,94,95,96,97,98,100Mo(n, X), E<5 keV; analyzed available data; deduced resonance parameters. Transmission data obtained at the time-of-flight facility GELINA.

doi: 10.1016/j.nimb.2022.09.019
Citations: PlumX Metrics


2021PA36      Astrophys.J. 921, 7 (2021)

S.Palmerini, M.Busso, D.Vescovi, E.Naselli, A.Pidatella, R.Mucciola, S.Cristallo, D.Mascali, A.Mengoni, S.Simonucci, S.Taioli

Presolar Grain Isotopic Ratios as Constraints to Nuclear and Stellar Parameters of Asymptotic Giant Branch Star Nucleosynthesis

NUCLEAR REACTIONS 84,85Kr, 93,94Mo, 93,94Nb, 93,94,95,96Zr, 134,135Cs(n, γ), E ∼ 30 keV; calculated stellar abundances. Comparison with available data.

doi: 10.3847/1538-4357/ac1786
Citations: PlumX Metrics


2020MA14      Phys.Lett. B 804, 135405 (2020)

A.Mazzone, S.Cristallo, O.Aberle, G.Alaerts, V.Alcayne, S.Amaducci, J.Andrzejewski, L.Audouin, V.Babiano-Suarez, M.Bacak, M.Barbagallo, V.Becares, F.Becvar, G.Bellia, E.Berthoumieux, J.Billowes, D.Bosnar, A.S.Brown, M.Busso, M.Caamano, L.Caballero, M.Calviani, F.Calvino, D.Cano-Ott, A.Casanovas, D.M.Castelluccio, F.Cerutti, Y.H.Chen, E.Chiaveri, G.Clai, N.Colonna, G.P.Cortes, M.A.Cortes-Giraldo, L.Cosentino, L.A.Damone, M.Diakaki, M.Dietz, C.Domingo-Pardo, R.Dressler, E.Dupont, I.Duran, Z.Eleme, B.Fernandez-Domingez, A.Ferrari, I.Ferro-Goncalves, P.Finocchiaro, V.Furman, R.Garg, A.Gawlik, S.Gilardoni, T.Glodariu, K.Gobel, E.Gonzalez-Romero, C.Guerrero, F.Gunsing, S.Heinitz, J.Heyse, D.G.Jenkins, E.Jericha, Y.Kadi, F.Kappeler, A.Kimura, N.Kivel, M.Kokkoris, Y.Kopatch, S.Kopecky, M.Krticka, D.Kurtulgil, I.Ladarescu, C.Lederer-Woods, J.Lerendegui-Marco, S.Lo Meo, S.-J.Lonsdale, D.Macina, A.Manna, T.Martinez, A.Masi, C.Massimi, P.F.Mastinu, M.Mastromarco, F.Matteucci, E.Maugeri, E.Mendoza, A.Mengoni, V.Michalopoulou, P.M.Milazzo, F.Mingrone, R.Mucciola, A.Musumarra, A.Negret, R.Nolte, F.Ogallar, A.Oprea, N.Patronis, A.Pavlik, J.Perkowski, L.Piersanti, I.Porras, J.Praena, J.M.Quesada, D.Radeck, D.Ramos Doval, R.Reifarth, D.Rochman, C.Rubbia, M.Sabate-Gilarte, A.Saxena, P.Schillebeeckx, D.Schumann, A.G.Smith, N.Sosnin, A.Stamatopoulos, G.Tagliente, J.L.Tain, Z.Talip, A.E.Tarifeno-Saldivia, L.Tassan-Got, P.Torres-Sanchez, A.Tsinganis, J.Ulrich, S.Urlass, S.Valenta, G.Vannini, V.Variale, P.Vaz, A.Ventura, D.Vescovi, V.Vlachoudis, R.Vlastou, A.Wallner, P.J.Woods, R.Wynants, T.J.Wright, P.Zugec

Measurement of the 154Gd(n, γ) cross section and its astrophysical implications

NUCLEAR REACTIONS 154Gd(n, γ), E=0.001-300 keV; measured reaction products, En, In, Eγ, Iγ; deduced capture yields, transmissions, capture σ. Comparison with ENDF/B-VIII library and KADoNiS.

doi: 10.1016/j.physletb.2020.135405
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23459.


Back to query form