Search Results - "Parascandolo T."

The $$^{27}\hbox {Al}(\hbox {p},\alpha )^{24}\hbox {Mg}$$ reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the $$^2\hbox {H}(^{27}\hbox {Al},\alpha ^{24}\hbox {Mg})\hbox {n}$$ reaction by Palmerini, S., La Cognata, M., Hammache, F., Acosta, L., Alba, R., Burjan, V., Chávez, E., Cherubini, S., Cvetinović, A., D’Agata, G., de Séréville, N., Di Pietro, A., Figuera, P., Fülöp, Z., Gaitán De Los Rios, K., Guardo, G. L., Gulino, M., Hayakawa, S., Kiss, G. G., La Commara, M., Lamia, L., Maiolino, C., Manicó, G., Matei, C., Mazzocco, M., Mrazek, J., Parascandolo, T., Petruse, T., Pierroutsakou, D., Pizzone, R. G., Rapisarda, G. G., Romano, S., Santonocito, D., Sergi, M. L., Spartà, R., Tumino, A., Yamaguchi, H.

“…The $$^{27}\hbox {Al}(\hbox {p},\alpha )^{24}\hbox {Mg}$$ 27 Al ( p , α ) 24 Mg reaction, which drives the destruction of $$^{27}$$ 27 Al and the production of…”
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The 27Al(p,α)24Mg reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the 2H(27Al,α24Mg)n reaction by Palmerini, S., La Cognata, M., Hammache, F., Acosta, L., Alba, R., Burjan, V., Chávez, E., Cherubini, S., Cvetinović, A., D’Agata, G., de Séréville, N., Di Pietro, A., Figuera, P., Fülöp, Z., Gaitán De Los Rios, K., Guardo, G. L., Gulino, M., Hayakawa, S., Kiss, G. G., La Commara, M., Lamia, L., Maiolino, C., Manicó, G., Matei, C., Mazzocco, M., Mrazek, J., Parascandolo, T., Petruse, T., Pierroutsakou, D., Pizzone, R. G., Rapisarda, G. G., Romano, S., Santonocito, D., Sergi, M. L., Spartà, R., Tumino, A., Yamaguchi, H.

“…The 27 Al ( p , α ) 24 Mg reaction, which drives the destruction of 27 Al and the production of 24 Mg in stellar hydrogen burning, has been investigated via…”
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The Treiman-Yang Criterion: validating the Trojan Horse Method by experimentally probing the reaction mechanism by Perrotta, S. S., Spitaleri, C., Cherubini, S., Cvetinović, A., D’Agata, G., Dell’Aquila, D., Di Pietro, A., Figuera, P., Guardo, L., Gulino, M., Indelicato, I., Kres, I., La Cognata, M., La Commara, M., Lamia, L., Lattuada, D., Lattuada, M., Lombardo, I., Mazzocco, M., Parascandolo, T., Pizzone, R. G., Rapisarda, G. G., Romano, S., Spartà, R., Trippella, O., Tumino, A.

“…Proper selection of the quasi-free (QF) break-up channel in a three-body reaction is a key aspect for the applicability of the Trojan Horse Method (THM). The…”
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Study of the 12 C + 16 O fusion reaction in carbon burning via the Trojan Horse Method by Oliva, A. A., Tumino, A., Soic, N., Prajapati, P. M., Acosta, L., Alba, R., Barba, F., Cherubini, S., D’Agata, G., Dell’Aquila, D., Di Pietro, A., Fernandez, J.P., Figuera, P., Galaviz Redondo, D., Guardo, L., Gulino, M., Hammache, F., Jelavic Malenica, D., Kiliç, A.I., La Cognata, M., La Commara, M., Lamia, L., Lattuada, D., Maiolino, C., Manicò, G., Mazzocco, M., Milin, M., Nanru, Ma, Nurmukhanbetova, A., Nurkic, D., Palmerini, S., Parascandolo, T., Pierroutsakou, D., Pizzone, R.G., Popocovski, R., Rapisarda, G.G., Romano, S., Santonocito, D., Sergi, M.L., Shotter, A., Spartà, R., Spiridon, A., Trache, L., Vukman, N., Yamaguchi, H.

“…12 C + 12 C is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than 10 9 K when most of the carbon is…”
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The 12 C + 16 O fusion reaction in carbon burning: Study at energies of astrophysical interest using the Trojan Horse Method by Oliva, A.A., Tumino, A., Soic, N., Prajapati, M.P., Acosta, L., Alba, R., Barba, F., Cherubini, S., D’Agata, G., Dell’Aquila, D., Di Pietro, A., Fernandez, P.J., Figuera, P., Galaviz Redondo, D., Guardo, L., Gulino, M., Hammache, F., Jelavic Malenica, D., Kiliç, A.I., La Cognata, M., La Commara, M., Lamia, L., Lattuada, D., Maiolino, C., Manicò, G., Mazzocco, M., Milin, M., Nanru, Ma, Nurmukhanbetova, A., Nurkic, D., Palmerini, S., Parascandolo, T., Pierroutsakou, D., Pizzone, R.G., Popocovski, R., Rapisarda, G.G., Romano, S., Santonocito, D., Sergi, M.L., Shotter, A., Spartà, R., Spiridon, A., Trache, L., Vukman, N., Yamaguchi, H.

“…The carbon-burning process in massive stars mainly occurs via the 12 C + 12 C. However, at temperatures higher than 10 9 K and considering the increased…”
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Study of the 12C +16 O fusion reaction in carbon burning via the Trojan Horse Method by Oliva A. A., Tumino A., Soic N., Prajapati P. M., Acosta L., Alba R., Barba F., Cherubini S., D’Agata G., Dell’Aquila D., Di Pietro A., Fernandez J.P., Figuera P., Galaviz Redondo D., Guardo L., Gulino M., Hammache F., Jelavic Malenica D., Kiliç A.I., La Cognata M., La Commara M., Lamia L., Lattuada D., Maiolino C., Manicò G., Mazzocco M., Milin M., Nanru Ma, Nurmukhanbetova A., Nurkic D., Palmerini S., Parascandolo T., Pierroutsakou D., Pizzone R.G., Popocovski R., Rapisarda G.G., Romano S., Santonocito D., Sergi M.L., Shotter A., Spartà R., Spiridon A., Trache L., Vukman N., Yamaguchi H.

“…12C +12 C is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than 109K when most of the carbon is…”
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The 12C +16 O fusion reaction in carbon burning: Study at energies of astrophysical interest using the Trojan Horse Method by Oliva A.A., Tumino A., Soic N., Prajapati M.P., Acosta L., Alba R., Barba F., Cherubini S., D’Agata G., Dell’Aquila D., Di Pietro A., Fernandez P.J., Figuera P., Galaviz Redondo D., Guardo L., Gulino M., Hammache F., Jelavic Malenica D., Kiliç A.I., La Cognata M., La Commara M., Lamia L., Lattuada D., Maiolino C., Manicò G., Mazzocco M., Milin M., Nanru Ma, Nurmukhanbetova A., Nurkic D., Palmerini S., Parascandolo T., Pierroutsakou D., Pizzone R.G., Popocovski R., Rapisarda G.G., Romano S., Santonocito D., Sergi M.L., Shotter A., Spartà R., Spiridon A., Trache L., Vukman N., Yamaguchi H.

“…The carbon-burning process in massive stars mainly occurs via the 12C +12 C. However, at temperatures higher than 109K and considering the increased abundance…”
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