Search Results - "Tumino A."

Asymptotic Normalization Coefficient Investigation of the 17O(d, p) Transfer for Astrophysical Application to the 17O(n, α)14C Reaction at Low Energies by Guardo, G. L., Lamia, L., Fernández-García, J. P., Piskor, S., La Cognata, M., D’Agata, G., Palmerini, S., Vescovi, D., Burjan, V., deBoer, R. J., Kroha, V., Lattuada, D., Mrazek, J., Oliva, A. A., Pizzone, R. G., Rapisarda, G. G., Romano, S., Sergi, M. L., Spartá, R., Tumino, A.

“…Indirect methods have proven to be a complementary approach for extending our knowledge of nuclear structure and low-energy cross sections. Among these, the…”
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Astrophysics studies with the Trojan Horse Method by Spitaleri, C., La Cognata, M., Lamia, L., Pizzone, R. G., Tumino, A.

“… The Trojan Horse Method represents an indirect approach to investigate reactions of astrophysical relevance at the energies of interest, free of Coulomb…”
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Few-Body Reactions with the Trojan Horse Method by Rapisarda, G.G., Spartá, R., Tumino, A.

“…The Trojan Horse method (THM) is a well-established experimental technique to measure nuclear reactions of astrophysical interest avoiding the suppression of…”
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Clusters and their fundamental role for Trojan Horse Method by Pizzone, R. G., Bertulani, C. A., Lamia, L., Cognata, M. La, Sergi, M. L., Spartá, R., Tumino, A.

“…The Trojan Horse Method (THM) lays its foundations on the cluster structure of light nuclei which are usually used as “Trojan horses”. Many of them were…”
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The Trojan Horse Method in nuclear astrophysics by Spitaleri, C., Mukhamedzhanov, A. M., Blokhintsev, L. D., Cognata, M. La, Pizzone, R. G., Tumino, A.

“…The study of energy production and nucleosynthesis in stars requires an increasingly precise knowledge of the nuclear reaction rates at the energies of…”
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Indirect Measurement of the 3He(n,p)3H Reaction Cross Section at Big Bang Energies by Pizzone, R. G., Sergi, M. L., Oliva, A. A., Zanatta-Martinez, T., Lamia, L., Spartá, R., Guardo, G. L., La Cognata, M., D’Agata, G., Palmerini, S., Tumino, A., Costa, M., Cittadino, D., Di Pietro, A., Figuera, P., Indelicato, I., Massara, A., Cherubini, S., Rapisarda, G. G., Romano, S., Spampinato, C., Couder, M., Tan, W., Wiescher, M., Lattuada, D., Gulino, M., Burjan, V., Mrazek, J., La Commara, M., Mazzocco, M., Prajapati, P. M., Aguilar, S., Anderson, T., Bardayan, D., Blankstein, D., Callahan, L., Clark, A., Frentz, B., Gula, A., Hall, M., Henderson, S. L., Kelmar, R., Liu, Q., Long, J., Majundar, A., McGiunness, S., Nelson, A., O’Malley, P., Seimour, C., Skulski, M., Wilkinson, J., Cha, S. M., Chae, K. Y., Kwag, M. S., Typel, S.

“…Neutron-induced nuclear reactions play an important role in the Big Bang Nucleosynthesis. Their excitation functions are, from an experimental point of view,…”
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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 by La Cognata, M., Palmerini, S., Adsley, P., Hammache, F., Di Pietro, A., Figuera, P., Dell’Agli, F., Alba, R., Cherubini, S., Guardo, G. L., Gulino, M., Lamia, L., Lattuada, D., Maiolino, C., Oliva, A., Pizzone, R. G., Prajapati, P. M., Rapisarda, G. G., Romano, S., Santonocito, D., Spartá, R., Sergi, M. L., Tumino, A., Ventura, P.

“…The abundance of 26Al carries a special role in astrophysics, since it probes active nucleosynthesis in the Milky Way and constrains the Galactic core-collapse…”
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Exploring the astrophysical energy range of the 27Al(p,α)24Mg reaction: A new recommended reaction rate by La Cognata, M., Palmerini, S., Adsley, P., Hammache, F., Di Pietro, A., Figuera, P., Alba, R., Cherubini, S., Dell'Agli, F., Guardo, G.L., Gulino, M., Lamia, L., Lattuada, D., Maiolino, C., Oliva, A., Pizzone, R.G., Prajapati, P.M., Romano, S., Santonocito, D., Spartá, R., Sergi, M.L., Tumino, A.

“…•A new indirect measurement of the 27Al(p,α)24Mg has been carried out down to astrophysical energies.•The strength of the 84.3 keV resonance has been measured,…”
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On the Determination of the 7Be(n, )4He Reaction Cross Section at BBN Energies by Lamia, L., Spitaleri, C., Bertulani, C. A., Hou, S. Q., Cognata, M. La, Pizzone, R. G., Romano, S., Sergi, M. L., Tumino, A.

“…7Be destruction channels are currently a matter of study because of their influence on the 7Li cosmological abundances. Here, we determine the cross section of…”
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An increase in the 12C + 12C fusion rate from resonances at astrophysical energies by Tumino, A., Spitaleri, C., La Cognata, M., Cherubini, S., Guardo, G. L., Gulino, M., Hayakawa, S., Indelicato, I., Lamia, L., Petrascu, H., Pizzone, R. G., Puglia, S. M. R., Rapisarda, G. G., Romano, S., Sergi, M. L., Spartá, R., Trache, L.

“…Carbon burning powers scenarios that influence the fate of stars, such as the late evolutionary stages of massive stars 1 (exceeding eight solar masses) and…”
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New Improved Indirect Measurement of the 19F(p, )16O Reaction at Energies of Astrophysical Relevance by Indelicato, I., La Cognata, M., Spitaleri, C., Burjan, V., Cherubini, S., Gulino, M., Hayakawa, S., Hons, Z., Kroha, V., Lamia, L., Mazzocco, M., Mrazek, J., Pizzone, R. G., Romano, S., Strano, E., Torresi, D., Tumino, A.

“…Fluorine abundance determination is of great importance in stellar physics to understand s-elements production and mixing processes in asymptotic giant branch…”
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Theoretical Predictions of Surface Light Element Abundances in Protostellar and Pre-Main Sequence Phase by Tognelli, E., Degl’Innocenti, S., Prada Moroni, P. G., Lamia, L., Pizzone, R. G., Tumino, A., Spitaleri, C., Chiavassa, A.

“…Theoretical prediction of surface stellar abundances of light elements–lithium, beryllium, and boron–represents one of the most interesting open problems in…”
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The 10B(n,α)7Li cross sections at ultra-low energy through the Trojan Horse Method applied to the 2H(10B,α7Li)1H by Guardo, G. L., Spitaleri, C., Lamia, L., Spartá, R., Carlin, N., Cherubini, S., Gimenez Del Santo, G., Indelicato, I., La Cognata, M., Lattuada, D., Messina, S., Munhoz, M., Perrotta, S. S., Pizzone, R. G., Rapisarda, G. G., Romano, S., Sergi, M. L., Souza, F. A., Szanto de Toledo, A., Tudisco, S., Tumino, A.

“… In the framework of the experimental campaign of the ( p , α ) and ( n , α ) reactions cross sections measurement involving the 10, 11 B isotopes, different…”
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Publisher Correction: An increase in the 12C + 12C fusion rate from resonances at astrophysical energies by Tumino, A., Spitaleri, C., La Cognata, M., Cherubini, S., Guardo, G. L., Gulino, M., Hayakawa, S., Indelicato, I., Lamia, L., Petrascu, H., Pizzone, R. G., Puglia, S. M. R., Rapisarda, G. G., Romano, S., Sergi, M. L., Spartá, R., Trache, L.

“…In equation (1) of this Letter, the closing bracket was missing; in Extended Data Fig. 1 and the accompanying legend, ‘ Φ ( p d )’ should have been ‘ Φ 2 ( p d…”
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Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method by Kiss, G.G., La Cognata, M., Spitaleri, C., Yarmukhamedov, R., Wiedenhöver, I., Baby, L.T., Cherubini, S., Cvetinović, A., D'Agata, G., Figuera, P., Guardo, G.L., Gulino, M., Hayakawa, S., Indelicato, I., Lamia, L., Lattuada, M., Mudò, F., Palmerini, S., Pizzone, R.G., Rapisarda, G.G., Romano, S., Sergi, M.L., Spartà, R., Trippella, O., Tumino, A., Anastasiou, M., Kuvin, S.A., Rijal, N., Schmidt, B., Igamov, S.B., Sakuta, S.B., Tursunmakhatov, K.I., Fülöp, Zs, Gyürky, Gy, Szücs, T., Halász, Z., Somorjai, E., Hons, Z., Mrázek, J., Tribble, R.E., Mukhamedzhanov, A.M.

“…The detection of the neutrinos produced in the p−p chain and in the CNO cycle can be used to test the Standard Solar Model. The 3He(α,γ)7Be reaction is the…”
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10B(n,α0)7Li and 10B(n,α1)7Li reactions measured via Trojan Horse Method by Spartà, R., Lamia, L., La Cognata, M., Spitaleri, C., Rapisarda, G. G., Guardo, G. L., Cherubini, S., D’Agata, G., Di Pietro, A., Figuera, P., Gulino, M., Lattuada, D., Lattuada, M., Palmerini, S., Pizzone, R. G., Romano, S., Sergi, M. L., Tumino, A., Typel, S.

“…The neutron capture reaction 10 B(n, α ) 7 Li has been investigated via the Trojan Horse Method from 0 to 1 MeV. The α 0 and α 1 channels, corresponding to 7…”
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The determination of the astrophysical S-factor of the direct 18O(p,γ)19F capture by the ANC method by Burjan, V., Hons, Z., Kroha, V., Mrázek, J., Piskoř, Š., Mukhamedzhanov, A. M., Trache, L., Tribble, R. E., La Cognata, M., Lamia, L., Pizzone, R. G., Romano, S., Spitaleri, C., Tumino, A.

“… The depletion of 18 O via the ( p , γ ) capture competes with the ( p , α ) capture during the CNO cycles in AGB stars. Despite the fact that the ( p , α )…”
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Cross-section Measurement of the Cosmologically Relevant 7Be(n, )4He Reaction over a Broad Energy Range in a Single Experiment by Lamia, L., Mazzocco, M., Pizzone, R. G., Hayakawa, S., La Cognata, M., Spitaleri, C., Bertulani, C. A., Boiano, A., Boiano, C., Broggini, C., Caciolli, A., Cherubini, S., D'Agata, G., da Silva, H., Depalo, R., Galtarossa, F., Guardo, G. L., Gulino, M., Indelicato, I., La Commara, M., La Rana, G., Menegazzo, R., Mrazek, J., Pakou, A., Parascandolo, C., Piatti, D., Pierroutsakou, D., Puglia, S. M. R., Romano, S., Rapisarda, G. G., Sánchez-Benítez, A. M., Sergi, M. L., Sgouros, O., Soramel, F., Soukeras, V., Spartá, R., Strano, E., Torresi, D., Tumino, A., Yamaguchi, H., Zhang, G. L.

“…Studying interactions of radioactive ions with neutrons is particularly demanding and has been performed only in a few cases. Some of these interactions are…”
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Triple α resonances in the 6Li + 6Li → 3α reaction at low energy by Tumino, A., Bonasera, A., Giuliani, G., Lattuada, M., Milin, M., Pizzone, R.G., Spitaleri, C., Tudisco, S.

“…The 6Li + 6Li → 3α reaction has been measured in a kinematically complete experiment at 3.1 MeV of beam energy. The reaction mainly proceeds via intermediate…”
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Low-energy d+d fusion reactions via the Trojan Horse Method by Tumino, A., Spitaleri, C., Mukhamedzhanov, A.M., Typel, S., Aliotta, M., Burjan, V., del Santo, M. Gimenez, Kiss, G.G., Kroha, V., Hons, Z., La Cognata, M., Lamia, L., Mrazek, J., Pizzone, R.G., Piskor, S., Rapisarda, G.G., Romano, S., Sergi, M.L., Spartà, R.

“…The bare nucleus S(E) factors for the H2(d,p)H3 and H2(d,n)He3 reactions have been measured for the first time via the Trojan Horse Method off the proton in…”
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