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NSR database version of April 11, 2024.

Search: Author = S.Cristallo

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2024AM02      Phys.Rev.Lett. 132, 122701 (2024)

S.Amaducci, N.Colonna, L.Cosentino, S.Cristallo, P.Finocchiaro, M.Krticka, C.Massimi, M.Mastromarco, A.Mazzone, E.A.Maugeri, A.Mengoni, I.U.Roederer, O.Straniero, S.Valenta, D.Vescovi, O.Aberle, V.Alcayne, J.Andrzejewski, L.Audouin, V.Babiano-Suarez, M.Bacak, M.Barbagallo, S.Bennett, E.Berthoumieux, J.Billowes, D.Bosnar, A.Brown, M.Busso, M.Caamano, L.Caballero-Ontanaya, F.Calvino, M.Calviani, D.Cano-Ott, A.Casanovas, F.Cerutti, E.Chiaveri, G.Cortes, M.A.Cortes-Giraldo, L.A.Damone, P.J.Davies, M.Diakaki, M.Dietz, C.Domingo-Pardo, R.Dressler, Q.Ducasse, E.Dupont, I.Duran, Z.Eleme, B.Fernandez-Dominguez, A.Ferrari, V.Furman, K.Gobel, R.Garg, A.Gawlik-Ramiega, S.Gilardoni, I.F.Goncalves, E.Gonzalez-Romero, C.Guerrero, F.Gunsing, H.Harada, S.Heinitz, J.Heyse, D.G.Jenkins, A.Junghans, F.Kappeler, Y.Kadi, A.Kimura, I.Knapova, M.Kokkoris, Y.Kopatch, D.Kurtulgil, I.Ladarescu, C.Lederer-Woods, H.Leeb, J.Lerendegui-Marco, S.J.Lonsdale, D.Macina, A.Manna, T.Martinez, A.Masi, P.Mastinu, E.Mendoza, V.Michalopoulou, P.M.Milazzo, F.Mingrone, J.Moreno-Soto, A.Musumarra, A.Negret, R.Nolte, F.Ogallar, A.Oprea, N.Patronis, A.Pavlik, J.Perkowski, C.Petrone, L.Piersanti, E.Pirovano, I.Porras, J.Praena, J.M.Quesada, D.Ramos-Doval, T.Rauscher, R.Reifarth, D.Rochman, C.Rubbia, M.Sabate-Gilarte, A.Saxena, P.Schillebeeckx, D.Schumann, A.Sekhar, A.G.Smith, N.V.Sosnin, P.Sprung, A.Stamatopoulos, G.Tagliente, J.L.Tain, A.Tarifeno-Saldivia, L.Tassan-Got, Th.Thomas, P.Torres-Sanchez, A.Tsinganis, J.Ulrich, S.Urlass, G.Vannini, V.Variale, P.Vaz, A.Ventura, V.Vlachoudis, R.Vlastou, A.Wallner, P.J.Woods, T.Wright, P.Zugec

Measurement of the 140Ce(n, γ) Cross Section at n_TOF and Its Astrophysical Implications for the Chemical Evolution of the Universe

NUCLEAR REACTIONS 140Ce(n, γ), E<200 keV; measured reaction products, En, In, Eγ, Iγ; deduced Maxwellian averaged σ, yields, resonance parameters, impact on galactic abundances. Comparison with ENDF/B-VIII.0, JENDL-5 libraries, R-matrix code SAMMY. The neutron beam time-of-flight facility (n_TOF) at CERN.

doi: 10.1103/PhysRevLett.132.122701
Citations: PlumX Metrics


2024TA03      Eur.Phys.J. A 60, 21 (2024)

G.Tagliente, P.M.Milazzo, C.Paradela, S.Kopecky, D.Vescovi, G.Alaerts, L.A.Damone, J.Heyse, M.Krticka, P.Schillebeeckx, A.Mengoni, R.Wynants, S.Valenta, O.Aberle, 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, F.Cerutti, Y.H.Chen, E.Chiaveri, N.Colonna, G.P.Cortes, M.A.Cortes-Giraldo, L.Cosentino, S.Cristallo, 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, D.G.Jenkins, E.Jericha, Y.Kadi, F.Kappeler, A.Kimura, N.Kivel, M.Kokkoris, Y.Kopatch, D.Kurtulgil, I.Ladarescu, A.C.Larsen, C.Lederer-Woods, J.Lerendegui-Marco, S.Lo Meo, S.J.Lonsdale, M.Lugaro, D.Macina, A.Manna, T.Martinez, A.Masi, C.Massimi, P.F.Mastinu, M.Mastromarco, F.Matteucci, E.Maugeri, A.Mazzone, E.Mendoza, V.Michalopoulou, F.Mingrone, 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, D.Schumann, A.G.Smith, M.Spelta, N.Sosnin, A.Stamatopoulos, J.L.Tain, Z.Talip, A.E.Tarifeno-Saldivia, L.Tassan-Got, P.Torres-Sanchez, A.Tsinganis, J.Ulrich, S.Urlass, G.Vannini, V.Variale, P.Vaz, A.Ventura, V.Vlachoudis, R.Vlastou, A.Wallner, P.J.Woods, T.J.Wright, P.Zugec

High-resolution cross section measurements for neutron interactions on 89Y with incident neutron energies up to 95 keV

NUCLEAR REACTIONS 89Y(n, X), (n, γ), E<95 keV; measured reaction products, En, In, TOF; deduced yields, resonance parameters, Maxwellian-averaged σ, capture kernel. Comparison with ENDF/B-VIII.0, JENDL-5, EXFOR libraries, Atlas of Neutron Resonances, KADONIS. The CERN n_TOF facility, GELINA at JRC-Geel.

doi: 10.1140/epja/s10050-024-01243-4
Citations: PlumX Metrics


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


2022LI64      Eur.Phys.J. A 58, 216 (2022)

N.Liu, T.Stephan, S.Cristallo, D.Vescovi, R.Gallino, L.R.Nittler, C.M.O.D.Alexander, A.M.Davis

Presolar silicon carbide grains of types Y and Z: their strontium and barium isotopic compositions and stellar origins

doi: 10.1140/epja/s10050-022-00838-z
Citations: PlumX Metrics


2022MA37      Universe 8, 80 (2022)

D.Mascali, D.Santonocito, S.Amaducci, L.Ando, V.Antonuccio, S.Biri, A.Bonanno, V.P.Bonanno, S.Briefi, M.Busso, L.Celona, L.Cosentino, S.Cristallo, M.Cuffiani, C.De Angelis, G.De Angelis, D.De Salvador, L.Di Donato, J.-E.Ducret, A.Eshkevar Vakili, U.Fantz, A.Galata, C.Gallo, S.Gammino, T.Isernia, H.Koivisto, K.-L.Kratz, R.Kronholm, M.La Cognata, S.Leoni, A.Locatelli, M.Maggiore, F.Maimone, L.Malferrari, G.Mancini, L.Maunoury, G.S.Mauro, M.Mazzaglia, A.Mengoni, A.Miraglia, B.Mishra, M.Musumeci, D.R.Napoli, E.Naselli, F.Odorici, L.Palladino, G.Palmisano, S.Pavone, S.Pennisi, A.Perego, A.Pidatella, R.Racz, R.Reitano, D.Rifuggiato, M.Rinaldi, A.D.Russo, F.Russo, G.Schillaci, S.Selleri, S.Simonucci, G.Sorbello, R.Sparta, S.Taioli, K.Tinschert, G.Torrisi, A.Trifiro, S.Tsikata, A.Tumino, D.Vescovi, L.Vincetti

A Novel Approach to β-Decay: PANDORA, a New Experimental Setup for Future In-Plasma Measurements

RADIOACTIVITY 94Nb, 134Cs, 176Lu(β-); calculated stellar to terrestrial T1/2 of β- decay of these isotopes as a function of temperature from 0.5-1000 MK; reviewed novel approach to measure β- decay rates of radionuclides relevant in nuclear-astrophysics under the PANDORA (Plasmas for Astrophysics, Nuclear Decay Observation and Radiation for Archaeometry) project at the INFN-LNS-Catania facility.

doi: 10.3390/universe8020080
Citations: PlumX Metrics


2022NH02      Nucl.Phys. A1023, 122450 (2022)

N.Nhu Le, S.Cristallo, D.Vescovi, L.Tan Phuc, N.Quang Hung

Maxwellian-averaged cross section of 181Ta(n, γ) reaction and its astrophysical implications

NUCLEAR REACTIONS 181Ta(n, γ), E<90 KeV; calculated Maxwellian-averaged σ using TALYS code. Comparison with available data.

doi: 10.1016/j.nuclphysa.2022.122450
Citations: PlumX Metrics


2021BA30      Eur.Phys.J. A 57, 197 (2021)

V.Babiano-Suarez, J.Lerendegui-Marco, J.Balibrea-Correa, L.Caballero, D.Calvo, I.Ladarescu, D.Real, C.Domingo-Pardo, F.Calvino, A.Casanovas, A.Tarifeno-Saldivia, V.Alcayne, C.Guerrero, M.A.Millan-Callado, T.Rodriguez-Gonzalez, M.Barbagallo, O.Aberle, S.Amaducci, J.Andrzejewski, L.Audouin, M.Bacak, S.Bennett, E.Berthoumieux, J.Billowes, D.Bosnar, A.Brown, M.Busso, M.Caamano, M.Calviani, D.Cano-Ott, F.Cerutti, E.Chiaveri, N.Colonna, G.Cortes, M.A.Cortes-Giraldo, L.Cosentino, S.Cristallo, L.A.Damone, P.J.Davies, M.Diakaki, M.Dietz, R.Dressler, Q.Ducasse, E.Dupont, I.Duran, Z.Eleme, B.Fernandez-Dominguez, A.Ferrari, P.Finocchiaro, V.Furman, K.Gobel, R.Garg, A.Gawlik, S.Gilardoni, I.F.Goncalves, E.Gonzalez-Romero, F.Gunsing, H.Harada, S.Heinitz, J.Heyse, D.G.Jenkins, A.Junghans, F.Kappeler, Y.Kadi, A.Kimura, I.Knapova, M.Kokkoris, Y.Kopatch, M.Krticka, D.Kurtulgil, C.Lederer-Woods, H.Leeb, S.J.Lonsdale, D.Macina, A.Manna, T.Martinez, A.Masi, C.Massimi, P.Mastinu, M.Mastromarco, E.A.Maugeri, A.Mazzone, E.Mendoza, A.Mengoni, V.Michalopoulou, P.M.Milazzo, F.Mingrone, J.Moreno-Soto, A.Musumarra, A.Negret, F.Ogallar, A.Oprea, N.Patronis, A.Pavlik, J.Perkowski, L.Persanti, C.Petrone, E.Pirovano, I.Porras, J.Praena, J.M.Quesada, D.Ramos Doval, T.Rauscher, R.Reifarth, D.Rochman, C.Rubbia, M.Sabate-Gilarte, A.Saxena, P.Schillebeeckx, D.Schumann, A.Sekhar, A.G.Smith, N.V.Sosnin, P.Sprung, A.Stamatopoulos, G.Tagliente, J.L.Tain, L.Tassan-Got, Th.Thomas, 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, T.Wright, P.Zugec

Imaging neutron capture cross sections: i-TED proof-of-concept and future prospects based on Machine-Learning techniques

NUCLEAR REACTIONS 197Au, 56Fe(n, γ), E<200 KeV; measured reaction products, Eγ, Iγ, En, In, TOF; deduced neutron spectra, signal-to-background ratio in (n, γ) σ measurements using Machine-Learning techniques.

doi: 10.1140/epja/s10050-021-00507-7
Citations: PlumX Metrics


2021BU01      Astrophys.J. 908, 55 (2021)

M.Busso, D.Vescovi, S.Palmerini, S.Cristallo, V.Antonuccio-Delogu

s-processing in AGB Stars Revisited. III. Neutron Captures from MHD Mixing at Different Metallicities and Observational Constraints

NUCLEAR REACTIONS 58Fe, 64Ni, 63,65Cu, 64,66,67,68,70Zn, 69,71Ga, 70,72,73,74,76Ge, 75As, 76,77,78,82Se, 79,81Br, 80,82,83,84,86Kr, 85,87Rb, 86,87,88Sr, 89Y, 90,91,92,94,96Zr, 93Nb, 96,97,98Mo, 99,100,101,102,104Ru, 103Rh, 104,105,106,108,110Pd, 107,109Ag, 110,111,112,113,114,116Cd, 115In, 116,117,118,119,120,122,124Sn, 121,123Sb, 122,123,124,125,126,128,130Te, 127I, 128,129,130,131,132,134,136Xe, 133Cs, 134,135,136,137,138Ba, 139La, 140,142Ce, 141Pr, 142,143,144,145,146,148,150Nd, 147,148,149,150,152Sm, 151,153Eu, 152,154,155,156,157,158,160Gd, 159Tb, 160,161,162,163,164Dy, 165Ho, 166,167,168,170Er, 169Tm, 170,171,172,173,174,176Yb, 175,176Lu, 176,177,178,179,180Hf, 181Ta, 182,183,184,186W, 185,187Re, 186,187,188,189,190,192Os, 191,193Ir, 192,194,195,196,198Pt, 197Au, 198,199,200,201,202,204Hg, 203,205Tl, 204,206,207,208Pb, 209Bi(n, γ), E ∼ 30 keV; calculated s-process main component solar system abundances.

doi: 10.3847/1538-4357/abca8e
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


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.


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.


2020PR16      Mon.not.R.Astron.Soc. 491, 1832 (2020)

N.Prantzos, C.Abia, S.Cristallo, M.Limongi, A.Chieffi

Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r- process components

NUCLEAR REACTIONS 70Ge, 76Se, 80,82Kr, 86,87Sr, 96Mo, 100Ru, 104Pd, 110Cd, 116Sn, 122,123,124Te, 128,130Xe, 134,136Ba, 142Nd, 148,150Sm, 154Gd, 160Dy, 170Yb, 176Lu, 176Hf, 186Os, 192Pt, 198Hg, 204Pb(n, γ), E ∼ 30 keV; analyzed available s-process only data; calculated s-process abundances.

NUCLEAR REACTIONS 69,71Ga, 70,72,73,74,76Ge, 75As, 76,77,78,80,82Se, 79,81Br, 80,82,83,84,86Kr, 85,87Rb, 86,87,88Sr, 89Y, 90,91,92,94,96Zr, 93Nb, 95,96,97,98,100Mo, 99,100,101,102,104Ru, 103Rh, 104,105,106,108,110Pd, 107,109Ag, 110,111,112,113,114,116Cd, 115In, 116,117,118,119,120,122,124Sn, 121,123Sb, 122,123,124,125,126,128,130Te, 127I, 128,129,130,131,132,134,136Xe, 133Cs, 134,135,136,137,138Ba, 139La, 140,142Ce, 141Pr, 142,143,144,145,146,148,150Nd, 147,148,149,150,152,154Sm, 151,153Eu, 154,155,156,157,158,160Gd, 159Tb, 160,161,162,163,164Dy, 165Ho, 166,167,169,170Er, 169Tm, 170,171,172,173,174,176Yb, 175,176Lu, 176,177,178,179,180Hf, 181Ta, 182,183,184,186W, 185,187Re, 186,187,188,189,190,192Os, 191,193Ir, 192,194,195,196,198Pt, 197Au, 198,199,200,201,202,204Hg, 203,205Tl, 204,206,207,208Pb, 209Bi, 232Th, 235,238U(n, γ), E ∼ 30 keV; analyzed available data; calculated s- and r-process abundances.

doi: 10.1093/mnras/stz3154
Citations: PlumX Metrics


2019BR08      Riv.Nuovo Cimento Soc.Ital.Fis. 42, 103 (2019)

C.Broggini, O.Straniero, M.G.F.Taiuti, G.de Angelis, G.Benzoni G.E.Bruno, S.Bufalino, G.Cardella, N.Colonna, M.Contalbrigo, G.Cosentino, S.Cristallo, C.Curceanu, E.De Filippo, R.Depalo, A.Di Leva, A.Feliciello, S.Gammino, A.Galata, M.La Cognata, R.Lea, S.Leoni, I.Lombardo, V.Manzari, D.Mascali, C.Massimi, A.Mengoni, D.Mengoni, D.R.Napoli, S.Palmerini, S.Piano, S.Pirrone, R.G.Pizzone, G.Politi, P.Prati, G.Prete, P.Russotto, G.Tagliente, G.M.Urciuoli

Experimental nuclear astrophysics in Italy

doi: 10.1393/ncr/i2019-10157-1
Citations: PlumX Metrics


2018CR02      Astrophys.J. 859, 105 (2018)

S.Cristallo, M.La Cognata, C.Massimi, A.Best, S.Palmerini, O.Straniero, O.Trippella, M.Busso, G.F.Ciani, F.Mingrone, L.Piersanti, D.Vescovi

The Importance of the 13C(α, n)16O Reaction in Asymptotic Giant Branch Stars

NUCLEAR REACTIONS 13C(α, n), E not given; analyzed available data; deduced impact of reaction rate variations on variations of the element surface distributions.

doi: 10.3847/1538-4357/aac177
Citations: PlumX Metrics


2017DI09      Phys.Rev. C 95, 045803 (2017)

A.Di Leva, G.Imbriani, R.Buompane, L.Gialanella, A.Best, S.Cristallo, M.De Cesare, A.D'Onofrio, J.G.Duarte, L.R.Gasques, L.Morales-Gallegos, A.Pezzella, G.Porzio, D.Rapagnani, V.Roca, M.Romoli, D.Schurmann, O.Straniero, F.Terrasi

Measurement of 1323 and 1487 keV resonances in 15N(α, γ)19F with the recoil separator ERNA

NUCLEAR REACTIONS 4He(15N, γ)19F, E(cm)=1323, 1487 keV; measured 19F recoils and reaction yields using the ERNA separator at CIRCE-Italy. 19F; deduced levels, resonances, Γα and Γγ, fractional contribution of resonances and direct capture (DC) component to the total reaction rate of 15N(α, γ)19F, as function of the temperature. Relevance for AGB nucleosynthesis.

doi: 10.1103/PhysRevC.95.045803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2409. Data from this article have been entered in the XUNDL database. For more information, click here.


2017MA15      Phys.Lett. B 768, 1 (2017)

C.Massimi, S.Altstadt, J.Andrzejewski, L.Audouin, M.Barbagallo, V.Becares, F.Becvar, F.Belloni, E.Berthoumieux, J.Billowes, S.Bisterzo, D.Bosnar, M.Brugger, M.Calviani, F.Calvino, D.Cano-Ott, C.Carrapico, D.M.Castelluccio, F.Cerutti, E.Chiaveri, L.Cosentino, M.Chin, G.Clai, N.Colonna, G.Cortes, M.A.Cortes-Giraldo, S.Cristallo, M.Diakaki, C.Domingo-Pardo, I.Duran, R.Dressler, C.Eleftheriadis, A.Ferrari, P.Finocchiaro, K.Fraval, S.Ganesan, A.R.Garcia, G.Giubrone, I.F.Goncalves, E.Gonzalez-Romero, E.Griesmayer, C.Guerrero, F.Gunsing, A.Hernandez-Prieto, D.G.Jenkins, E.Jericha, Y.Kadi, F.Kappeler, D.Karadimos, N.Kivel, P.Koehler, M.Kokkoris, S.Kopecky, M.Krticka, J.Kroll, C.Lampoudis, C.Langer, E.Leal-Cidoncha, C.Lederer, H.Leeb, L.S.Leong, S.Lo Meo, R.Losito, A.Mallick, A.Manousos, J.Marganiec, T.Martinez, P.F.Mastinu, M.Mastromarco, E.Mendoza, A.Mengoni, P.M.Milazzo, F.Mingrone, M.Mirea, W.Mondelaers, A.Musumarra, C.Paradela, A.Pavlik, J.Perkowski, M.Pignatari, L.Piersanti, A.Plompen, J.Praena, J.M.Quesada, T.Rauscher, R.Reifarth, A.Riego, M.S.Robles, C.Rubbia, M.Sabate-Gilarte, R.Sarmento, A.Saxena, P.Schillebeeckx, S.Schmidt, D.Schumann, G.Tagliente, J.L.Tain, D.Tarrio, L.Tassan-Got, A.Tsinganis, S.Valenta, G.Vannini, I.Van Rijs, V.Variale, P.Vaz, A.Ventura, M.J.Vermeulen, V.Vlachoudis, R.Vlastou, A.Wallner, T.Ware, M.Weigand, C.Weiss, R.Wynants, T.Wright, P.Zugec

Neutron spectroscopy of 26Mg states: Constraining the stellar neutron source 22Ne(α, n)25Mg

NUCLEAR REACTIONS 25Mg(n, γ), (n, X), E<300 KeV; measured reaction products, En, In, Eγ, Iγ; deduced yields, σ, resonance parameters and corresponding excitation energies of the 26Mg compound nucleus, Maxwellian-averaged cross sections, reaction rates for inverse reactions. R-matrix analysis of the experimental data.

doi: 10.1016/j.physletb.2017.02.025
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23327. Data from this article have been entered in the XUNDL database. For more information, click here.


2016BO10      Eur.Phys.J. A 52, 75 (2016)

A.Boeltzig, C.G.Bruno, F.Cavanna, S.Cristallo, T.Davinson, R.Depalo, R.J.deBoer, A.Di Leva, F.Ferraro, G.Imbriani, P.Marigo, F.Terrasi, M.Wiescher

Shell and explosive hydrogen burning - Nuclear reaction rates for hydrogen burning in RGB, AGB and Novae

COMPILATION 15N(p, γ0), (p, γ), E(cm)=0.01-2 MeV;15N, 17O, 22Ne, 23Na, 25Mg(p, γ), T=0.01-1 GK;17O(p, α), T=0.01-1 GK; compiled data on reaction rates. 15N(p, γ0); deduced S-factor using R-matrix.

doi: 10.1140/epja/i2016-16075-4
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2013AV02      Astrophys.J. 768, L18 (2013)

J.N.Avila, T.R.Ireland, M.Lugaro, F.Gyngard, E.Zinner, S.Cristallo, P.Holden, T.Rauscher

Europium s-process Signature at Close-to-solar Metallicity in Stardust SiC Grains from Asymptotic Giant Branch Stars

doi: 10.1088/2041-8205/768/1/L18
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2013HE10      Astrophys.J. 768, L11 (2013)

R.P.Hedrosa, C.Abia, M.Busso, S.Cristallo, I.Dominguez, S.Palmerini, B.Plez, O.Straniero

Nitrogen Isotopes in Asymptotic Giant Branch Carbon Stars and Presolar SiC Grains: A Challenge for Stellar Nucleosynthesis

doi: 10.1088/2041-8205/768/1/L11
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2010CR05      J.Phys.:Conf.Ser. 202, 012033 (2010)

S.Cristallo, L.Piersanti, R.Gallino, O.Straniero, F.Kappeler, I.Dominguez, P.Mohr

The long-standing problem of 176Lu/176Hf branching: A new approach with full stellar evolutionary models

NUCLEAR REACTIONS 175Lu(n, γ), E above 15 keV; calculated long-term time behaviour of 176Lu and 176Hf [product of β-decay of excited 176Lu].

doi: 10.1088/1742-6596/202/1/012033
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2006ST35      Nucl.Phys. A777, 311 (2006)

O.Straniero, R.Gallino, S.Cristallo

s process in low-mass asymptotic giant branch stars

doi: 10.1016/j.nuclphysa.2005.01.011
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2005CR04      Nucl.Phys. A758, 509c (2005)

S.Cristallo, O.Straniero, R.Gallino

S-process nucleosynthesis in low mass AGB Stars: do we really need an improved determination of the 13C(α, n)16O reaction rate?

doi: 10.1016/j.nuclphysa.2005.05.181
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2005GA39      Nucl.Phys. A758, 485c (2005)

R.Gallino, D.Delaude, L.Husti, S.Cristallo, O.Straniero, S.Ryan

Predictions of s-process Lead in low-metallicity stars compared with spectroscopic observations

doi: 10.1016/j.nuclphysa.2005.05.089
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2003GA27      Nucl.Phys. A718, 181c (2003)

R.Gallino, E.Arnone, S.Cristallo, S.Masera, C.Travaglio, D.L.Lambert, M.Lugaro, F.Kappeler, H.Van Winckel, M.Reyniers, O.Straniero, A.M.Davis

Minute steps on the quest of the s-process

doi: 10.1016/S0375-9474(03)00711-5
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2001CR05      Nucl.Phys. A688, 217c (2001)

S.Cristallo, O.Straniero, R.Gallino, F.Herwig, A.Chieffi, M.Limongi, M.Busso

The Formation of the 13C Pocket in Asymptotic Giant Branch Stars and Related Nucleosynthesis

doi: 10.1016/S0375-9474(01)00701-1
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