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NSR database version of April 27, 2024.

Search: Author = S.Palmerini

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2023CA14      Phys.Rev. C 108, 045802 (2023)

D.P.Carrasco-Rojas, M.Williams, P.Adsley, L.Lamia, B.Bastin, T.Faestermann, C.Fougeres, F.Hammache, D.S.Harrouz, R.Hertenberger, M.La Cognata, A.Meyer, F.de Oliveira Santos, S.Palmerini, R.G.Pizzone, S.Romano, N.de Sereville, A.Tumino, H.-F.Wirth

Searching for resonance states in ²²Ne(p, γ)²³Na

doi: 10.1103/PhysRevC.108.045802
Citations: PlumX Metrics
Data from this article have been entered in the XUNDL database. For more information, click here.

2023GU07      Eur.Phys.J. A 59, 65 (2023)

G.L.Guardo, T.Petruse, D.Lattuada, M.La Cognata, D.L.Balabanski, E.Aciksoz, L.Acosta, L.Capponi, D.Carbone, S.Cherubini, D.Choudhury, G.D'Agata, A.Di Pietro, P.Figuera, M.Gulino, A.I.Kilik, M.La Commara, L.Lamia, C.Matei, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, P.-A.Soderstrom, R.Sparta, A.Tumino, S.Vinals

Direct measurement of the ¹⁹F(p, α₀)¹⁶O reaction at E_cm= 0.4-0.9 using the LHASA detector array

NUCLEAR REACTIONS ¹H(¹⁹F, α), E(cm)=0.4-0.9 MeV; measured reaction products, Eα, Iα; deduced σ(θ), S-factor. Comparison with NACRE compilation, available data. INFN-Laboratori Nazionali del Sud, Catania (Italy).

doi: 10.1140/epja/s10050-023-00957-1
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Data from this article have been entered in the XUNDL database. For more information, click here.

2023LA06      J.Phys.(London) G50, 033002 (2023)

A.M.Laird, M.Lugaro, A.Kankainen, P.Adsley, D.W.Bardayan, H.E.Brinkman, B.Cote, C.M.Deibel, R.Diehl, F.Hammache, J.W.den Hartogh, J.Jose, D.Kurtulgil, C.Lederer-Woods, G.Lotay, G.Meynet, S.Palmerini, M.Pignatari, R.Reifarth, N.de Sereville, A.Sieverding, R.J.Stancliffe, T.C.L.Trueman, T.Lawson, J.S.Vink, C.Massimi, A.Mengoni

Progress on nuclear reaction rates affecting the stellar production of ²⁶Al

NUCLEAR REACTIONS ²⁵Mg, ^25,26Al(p, γ), ²⁶Al(n, p), (n, α), ²⁵Mg(α, n), ²³Na(α, p), ^24,25Mg(n, γ), E<300 KeV; analyzed available data; deduced σ, reaction rates, resonance parameters.

doi: 10.1088/1361-6471/ac9cf8
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2022HA03      Phys.Rev. C 105, 015805 (2022)

D.S.Harrouz, N.de Sereville, P.Adsley, F.Hammache, R.Longland, B.Bastin, T.Faestermann, R.Hertenberger, M.La Cognata, L.Lamia, A.Meyer, S.Palmerini, R.G.Pizzone, S.Romano, A.Tumino, H.-F.Wirth

Experimental study of the ³⁰Si(³He, d)³¹P reaction and thermonuclear reaction rate of ³⁰Si(p, γ)³¹P

NUCLEAR REACTIONS ³⁰Si(³He, d)³¹P, E=25 MeV beam from the Tandem Van de Graaff accelerator at MLL-Garching; measured E(d), I(d), σ(θ), deuterons momentum analyzed using a Q3D magnetic spectrometer, and detected in the focal plane of proportional counters. ³¹P; deduced levels, J, π, L-transfers, spectroscopic factors, single-particle widths, DWBA analysis of angular distribution data. ³⁰Si(p, γ)³¹P, T₉=0.010-10.0; deduced proton resonance energies, Γ_p, resonance strengths, astrophysical reaction rates. Comparison with previous experimental results and evaluated data for ³¹P structure, and with available data for proton resonances.

doi: 10.1103/PhysRevC.105.015805
Citations: PlumX Metrics
Data from this article have been entered in the XUNDL database. For more information, click here.

2022LA01      Phys.Lett. B 826, 136917 (2022)

M.La Cognata, S.Palmerini, P.Adsley, F.Hammache, A.Di Pietro, P.Figuera, R.Alba, S.Cherubini, F.Dell'Agli, G.L.Guardo, M.Gulino, L.Lamia, D.Lattuada, C.Maiolino, A.Oliva, R.G.Pizzone, P.M.Prajapati, S.Ramano, D.Santonocito, R.Sparta, M.L.Sergi, A.Tumino

Exploring the astrophysical energy range of the ²⁷Al(p, α)²⁴Mg reaction: A new recommended reaction rate

NUCLEAR REACTIONS ²H(²⁷Al, α²⁴Mg)¹NN, E<1.5 MeV; measured reaction products. ²⁸Si, ²⁴Mg; deduced σ(θ, E), strengths of the levels, astrophysical reaction rates. The indirect Trojan Horse method (THM), INFN-LNS Tandem accelerator (Catania, Italy).

doi: 10.1016/j.physletb.2022.136917
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Data from this article have been entered in the XUNDL database. For more information, click here.

2022LA14      Astrophys.J. 941, 96 (2022)

M.La Cognata, S.Palmerini, P.Adsley, F.Hammache, A.Di Pietro, P.Figuera, F.Dell'Agli, R.Alba, S.Cherubini, G.L.Guardo, M.Gulino, L.Lamia, D.Lattuada, C.Maiolino, A.Oliva, R.G.Pizzone, P.M.Prajapati, G.G.Rapisarda, S.Romano, D.Santonocito, R.Sparta, M.L.Sergi, A.Tumino, P.Ventura

A New Reaction Rate of the ²⁷Al(p/α)²⁴Mg Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for ²⁷Al Yields of Intermediate-mass Stars

NUCLEAR REACTIONS ²H(²⁷Al, α²⁴Mg), E=80 MeV; measured reaction products. ²⁸Si, ²⁴Mg; deduced σ(θ), σ(θ, E), resonance strengths. Comparison with Monte Carlo code RatesMC. Indirect Trojan Horse Method (THM), the INFN-LNS Tandem (Catania, Italy).

doi: 10.3847/1538-4357/ac9c5e
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Data from this article have been entered in the XUNDL database. For more information, click here.

2021AD01      Phys.Rev. C 103, 015805 (2021)

P.Adsley, U.Battino, A.Best, A.Caciolli, A.Guglielmetti, G.Imbriani, H.Jayatissa, M.La Cognata, L.Lamia, E.Masha, C.Massimi, S.Palmerini, A.Tattersall, R.Hirschi

Reevaluation of the ²²Ne(α, γ)²⁶Mg and ²²Ne(α, n)²⁵Mg reaction rates

NUCLEAR REACTIONS ²²Ne(α, γ); ²⁵Mg(n, γ); ²²Ne(⁶Li, d); ²⁶Mg(γ, γ'), (p, p'), (d, d'), (α, α'); ¹¹B(¹⁶O, p); evaluated experimental data. ²⁶Mg; evaluated nuclear data for levels, resonances, J, π, resonance energies and resonance strengths for (α, γ) and (α, n) reactions, Γ_α, Γ_p, Γ_n. ²²Ne(α, γ)²⁶Mg, T=0.010-1.250 GK; ²²Ne(α, n)²⁵Mg, T=0.030-1.250 GK; recommended reaction rates, ratios of reaction rates, based on present evaluation and using different statistical methods. Comparison with theoretical predictions. Relevance to weak s process in evolved massive stars and in the helium flash in low-mass AGB stars.

doi: 10.1103/PhysRevC.103.015805
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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, ^{64,66,67,68,70}Zn, ^69,71Ga, ^{70,72,73,74,76}Ge, ⁷⁵As, ^76,77,78,82Se, ^79,81Br, ^{80,82,83,84,86}Kr, ^85,87Rb, ^86,87,88Sr, ⁸⁹Y, ^{90,91,92,94,96}Zr, ⁹³Nb, ^96,97,98Mo, ^{99,100,101,102,104}Ru, ¹⁰³Rh, ^{104,105,106,108,110}Pd, ^107,109Ag, ^{110,111,112,113,114,116}Cd, ¹¹⁵In, ^{116,117,118,119,120,122,124}Sn, ^121,123Sb, ^{122,123,124,125,126,128,130}Te, ¹²⁷I, ^{128,129,130,131,132,134,136}Xe, ¹³³Cs, ^{134,135,136,137,138}Ba, ¹³⁹La, ^140,142Ce, ¹⁴¹Pr, ^{142,143,144,145,146,148,150}Nd, ^{147,148,149,150,152}Sm, ^151,153Eu, ^{152,154,155,156,157,158,160}Gd, ¹⁵⁹Tb, ^{160,161,162,163,164}Dy, ¹⁶⁵Ho, ^{166,167,168,170}Er, ¹⁶⁹Tm, ^{170,171,172,173,174,176}Yb, ^175,176Lu, ^{176,177,178,179,180}Hf, ¹⁸¹Ta, ^{182,183,184,186}W, ^185,187Re, ^{186,187,188,189,190,192}Os, ^191,193Ir, ^{192,194,195,196,198}Pt, ¹⁹⁷Au, ^{198,199,200,201,202,204}Hg, ^203,205Tl, ^{204,206,207,208}Pb, ²⁰⁹Bi(n, γ), E ∼ 30 keV; calculated s-process main component solar system abundances.

doi: 10.3847/1538-4357/abca8e
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
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2021DA04      Phys.Rev. C 103, 015806 (2021)

G.D'Agata, A.I.Kilic, V.Burjan, J.Mrazek, V.Glagolev, V.Kroha, G.L.Guardo, M.La Cognata, L.Lamia, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, C.Spitaleri, I.Sivacek, A.Tumino

²⁶Si(p, γ)²⁷P direct proton capture by means of the asymptotic normalization coefficients method for mirror nuclei

NUCLEAR REACTIONS ²⁶Mg(d, p)²⁷Mg, E=19.2 MeV; measured reaction products, σ(θ) for ground and first excited states using ΔE-E telescopes at INFN-LNS-Catania accelerator facility; deduced Optical Model Potential parameters for entrance and exit channels using DWBA calculations. ²⁶Mg(n, γ)²⁷Mg; ²⁶Si(p, γ)²⁷P; deduced spectroscopic factors and asymptotic normalization coefficients (ANCs) for capture in the ground and first excited states, width Γ_p for first resonance in ²⁷P using the ANC methodology for mirror nuclei. ²⁶Si(p, γ)²⁷P, T₉=0.1-2.0; calculated astrophysical reaction rates.

doi: 10.1103/PhysRevC.103.015806
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD1035. Data from this article have been entered in the XUNDL database. For more information, click here.

2021HA53      Astrophys.J. 915, L13 (2021)

S.Hayakawa, M.La Cognata, L.Lamia, H.Yamaguchi, D.Kahl, K.Abe, H.Shimizu, L.Yang, O.Beliuskina, S.M.Cha, K.Y.Chae, S.Cherubini, P.Figuera, Z.Ge, M.Gulino, J.Hu, A.Inoue, N.Iwasa, A.Kim, D.Kim, G.Kiss, S.Kubono, M.La Commara, M.Lattuada, E.J.Lee, J.Y.Moon, S.Palmerini, C.Parascandolo, S.Y.Park, V.H.Phong, D.Pierroutsakou, R.G.Pizzone, G.G.Rapisarda, S.Romano, C.Spitaleri, X.D.Tang, O.Trippella, A.Tumino, N.T.Zhang

Constraining the Primordial Lithium Abundance: New Cross Section Measurement of the ⁷Be + n Reactions Updates the Total ⁷Be Destruction Rate

NUCLEAR REACTIONS ²H(⁷Be, p⁷Li)¹H, E=3.16 MeV/nucleon; measured reaction products. ⁸Be; deduced σ, low-lying resonance parameters, astrophysical reaction rates for ⁷Be(n, p) and ⁷Be(n, α) reactions. Comparison with available data. the Trojan Horse Method (THM), Center-for-Nuclear-Study RI Beam separator (CRIB), the University of Tokyo, located atthe RI Beam Factory, RIKEN.

doi: 10.3847/2041-8213/ac061f
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23652.

2021KI06      Phys.Rev. C 104, 015807 (2021)

G.G.Kiss, M.La Cognata, R.Yarmukhamedov, K.I.Tursunmakhatov, I.Wiedenhover, L.T.Baby, S.Cherubini, A.Cvetinovic, G.D'Agata, P.Figuera, G.L.Guardo, M.Gulino, S.Hayakawa, I.Indelicato, L.Lamia, M.Lattuada, F.Mudo, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, C.Spitaleri, O.Trippella, A.Tumino, M.Anastasiou, S.A.Kuvin, N.Rijal, B.Schmidt, S.B.Igamov, S.B.Sakuta, Zs.Fulop, Gy.Gyurky, T.Szucs, Z.Halasz, E.Somorjai, Z.Hons, J.Mrazek, R.E.Tribble, A.M.Mukhamedzhanov

Indirect determination of the astrophysical S factor for the ⁶Li (p, γ)⁷Be reaction using the asymptotic normalization coefficient method

NUCLEAR REACTIONS ⁶Li(³He, d)⁷Be, E=3, 5 MeV; measured E(d), I(d), σ(θ) using ΔE-E silicon detector telescopes at the University of Catania and the FN tandem accelerator of Florida State University. ⁷Be; deduced levels, asymptotic normalization coefficient (ANCs) for the g.s. and the first excited state at 429 keV of ⁷Be from DWBA analysis of angular distributions. ⁶Li(p, γ)⁷Be, E=0.05-0.35 MeV; deduced asymptotic normalization coefficient (ANCs) using results from the ⁶Li(³He, d) reaction. ⁶Li(p, γ)⁷Be, E<1.0 MeV; analyzed available experimental data; deduced astrophysical S factor from direct experimental data, as well as present indirect method from ANCs determined in ⁶Li(³He, d) experiment. Relevance to big-bang and stellar nucleosynthesis.

doi: 10.1103/PhysRevC.104.015807
Citations: PlumX Metrics
Data from this article have been entered in the XUNDL database. For more information, click here.

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

2021SP03      Eur.Phys.J. A 57, 170 (2021)

R.Sparta, L.Lamia, M.La Cognata, C.Spitaleri, G.G.Rapisarda, G.L.Guardo, S.Cherubini, G.D'Agata, A.Di Pietro, P.Figuera, M.Gulino, D.Lattuada, M.Lattuada, S.Palmerini, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino, S.Typel

¹⁰B(n, α₀)⁷Li and ¹⁰B(n, α₁)⁷Li reactions measured via Trojan Horse Method

NUCLEAR REACTIONS ²H(¹⁰B, α⁷Be), E=28 MeV; measured reaction products, Eα, Iα; deduced momentum distribution for the spectator particle, σ(θ), σ(E), ¹⁰B(n, α) σ using the Trojan Horse Method.

doi: 10.1140/epja/s10050-021-00481-0
Citations: PlumX Metrics

2020KI11      Phys.Lett. B 807, 135606 (2020)

G.G.Kiss, M.La Cognata, C.Spitaleri, R.Yarmukhamedov, I.Wiedenhover, L.T.Baby, S.Cherubini, A.Cvetinovic, G.D'Agata, P.Figuera, G.L.Guardo, M.Gulino, S.Hayakawa, I.Indelicato, L.Lamia, M.Lattuada, F.Mudo, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, O.Trippella, A.Tumino, M.Anastasiou, S.A.Kuvin, N.Rijal, B.Schmidt, S.B.Igamov, S.B.Sakuta, K.I.Tursunmakhatov, Zs.Fulop, G.Gyurky, T.Szucs, Z.Halasz, E.Somorjai, Z.Hons, J.Mrazek, R.E.Tribble, A.M.Mukhamedzhanov

Astrophysical S-factor for the ³He(α, γ)⁷Be reaction via the asymptotic normalization coefficient (ANC) method

NUCLEAR REACTIONS ⁶Li(³He, d)⁷Be, E=3, 5 MeV; measured reaction products; deduced σ(θ), S-factor, external capture contribution using the Asymptotic Normalization Coefficient (ANC) technique.

doi: 10.1016/j.physletb.2020.135606
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2598. Data from this article have been entered in the XUNDL database. For more information, click here.

2020PI11      Eur.Phys.J. A 56, 199 (2020)

R.G.Pizzone, C.Spampinato, R.Sparta, M.Couder, W.Tan, V.Burjan, G.D'Agata, G.L.Guardo, M.La Cognata, L.Lamia, J.Mrazek, S.Palmerini, S.Typel, A.Tumino, M.Wiescher, S.Anguilar, D.Bardayan, D.Blankstein, L.Boccioli, L.Callahan, S.M.Cha, K.Y.Chae, A.M.Clark, B.Frentz, M.R.Hall, A.Gula, S.Henderson, R.Kelmar, M.S.Kwag, I.Indelicato, M.La Commara, D.Lattuada, Q.Liu, J.Long, M.Mazzocco, A.Majumdar, S.McGuinness, A.Nelson, A.A.Oliva, P.O'Malley, P.M.Prajapati, G.G.Rapisarda, S.Romano, M.L.Sergi, C.Seymour, M.Skulski, C.Spitaleri, J.Wilkinson

Indirect measurement of the ³He(n, p)³H reaction cross section at Big Bang energies

NUCLEAR REACTIONS ²H(³He, pt), E=9 MeV; measured reaction products, Ep, Ip; deduced σ for ³He(n, p) reaction using the Trojan Horse Method (THM).

doi: 10.1140/epja/s10050-020-00212-x
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset14716.

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

2018DA14      Astrophys.J. 860, 61 (2018)

G.D'Agata, R.G.Pizzone, M.La Cognata, I.Indelicato, C.Spitaleri, S.Palmerini, O.Trippella, D.Vescovi, S.Blagus, S.Cherubini, P.Figuera, L.Grassi, G.L.Guardo, M.Gulino, S.Hayakawa, R.Kshetri, L.Lamia, M.Lattuada, T.Mijatovic, M.Milin, D.Miljanic, L.Prepolec, G.G.Rapisarda, S.Romano, M.L.Sergi, N.Skukan, N.Soic, V.Tokic, A.Tumino, M.Uroic

The ¹⁹F(α, p)²²Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars

NUCLEAR REACTIONS ¹⁹F(⁶Li, p²²Ne), E=6 MeV; measured reaction products. ²³Na; deduced yields, σ(θ), σ, reaction rates. Comparison with available data.

doi: 10.3847/1538-4357/aac207
Citations: PlumX Metrics

2017PA45      Geochim.Cosmochim.Act. 221, 21 (2017)

S.Palmerini, O.Trippella, M.Busso, D.Vescovi, M.Petrelli, A.Zucchini, F.Frondini

s-Processing from MHD-induced mixing and isotopic abundances in presolar SiC grains

NUCLEAR REACTIONS ¹³C(α, n)¹⁶O, E not given; analyzed available data; deduced isotopic abundance ratios of s-elements in presolar SiC grains.

doi: 10.1016/j.gca.2017.05.030
Citations: PlumX Metrics

2017RA13      Nucl.Instrum.Methods Phys.Res. B407, 217 (2017); Reprint Nucl.Instrum.Methods Phys.Res. B414, 195 (2018)

D.Rapagnani, R.Buompane, A.Di Leva, L.Gialanella, M.Busso, M.De Cesare, G.De Stefano, J.G.Duarte, L.R.Gasques, L.Morales-Gallegos, S.Palmerini, M.Romoli, F.Tufariello

A supersonic jet target for the cross section measurement of the ¹²C(a, γ)¹⁶O reaction with the recoil mass separator ERNA

NUCLEAR REACTIONS ¹²C(α, γ), E(cm)=1.9 MeV; measured reaction products, ¹⁶O; deduced design study of a jet target for the recoil mass separator ERNA, aiming to measure σ. Comparison with CFD calculations.

doi: 10.1016/j.nimb.2017.07.003
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2015LA12      Astrophys.J. 805, 128 (2015)

M.La Cognata, S.Palmerini, C.Spitaleri, I.Indelicato, A.M.Mukhamedzhanov, I.Lombardo, O.Trippella

Updated THM astrophysical factor of the ¹⁹F(p, α)¹⁶O reaction and direct data at astrophysical energies

NUCLEAR REACTIONS ¹⁹F(p, α)¹⁶O, E(cm)=600-800 keV; analyzed available data; deduced renormalized data, form factor. Trojan Horse Method (THM).

doi: 10.1088/0004-637X/805/2/128
Citations: PlumX Metrics

2014TR02      Astrophys.J. 787, 41 (2014)

O.Trippella, M.Busso, E.Maiorca, F.Kappeler, S.Palmerini

s-Processing in AGB Stars Revisited. I. Does the Main Component Constrain the Neutron Source in the ¹³C Pocket?

doi: 10.1088/0004-637X/787/1/41
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2011LA13      Astrophys.J. 739, L54 (2011)

M.La Cognata, A.M.Mukhamedzhanov, C.Spitaleri, I.Indelicato, M.Aliotta, V.Burjan, S.Cherubini, A.Coc, M.Gulino, Z.Hons, G.G.Kiss, V.Kroha, L.Lamia, J.Mrazek, S.Palmerini, S.Piskor, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Tumino

The Fluorine Destruction in Stars: First Experimental Study of the ¹⁹F(p, α₀)¹⁶O Reaction at Astrophysical Energies

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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0674.

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