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87 results on '"Puglia, Sebastiana"'

1. The 19F(p, α1,2) reaction studied via Trojan Horse Method in astrophysical range of interest

Author

Vukman Nikola, Su Xuedou D., Rapisarda Giuseppe Gabriele, Oliva Alessandro Alberto, La Cognata Marco, Mazzocco Marco, Palmerini Sara, Becherini Bernardo, Cherubini Silvio, Guardo Giovanni Luca, Gulino Marissa, Hayakawa Seiya, Indelicato Iolanda, Lamia Livio, Pizzone Rosario Gianluca, Puglia Sebastiana Maria, Romano Stefano, Spitaleri Claudio, Trippella Oscar, and Tumino Aurora

Subjects
Physics, QC1-999
Abstract

The complex reaction network connected to the 19F stellar abundance is very sensitive to the physical condition in stars. To overcome difficulties present in the direct measurements, mainly the very low cross section in the astrophysical energy range due to the Coulomb repulsion, an indirect measurement of the 19F(p, α) reaction, with the Trojan Horse Method (THM), was performed at INFN-LNS. While the method had been successfully used to study α0 channel, in the present analysis focus was given to the α1,2 channels, where better knowledge of the reaction rates at low energies is required, obtainable by employing the THM method.

Published
2024
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2. Characterization of low-energy argon recoils with the ReD experiment

Author

Pandola, Luciano, primary, Ahmad, Iftikhar, additional, Albergo, Sebastiano, additional, Albuquerque, Ivone F.M., additional, Atzori Corona, Matteo, additional, Ave, Maximo, additional, Bottino, Bianca, additional, Cadeddu, Matteo, additional, Caminata, Alessio, additional, Canci, Nicola, additional, Cesarano, Raoul, additional, Davini, Stefano, additional, Dias, Lucas K.S., additional, DI CAPUA, FRANCESCO, additional, Dolganov, Grigory, additional, Fiorillo, Giuliana, additional, Franco, Davide, additional, Gulino, Marisa, additional, Kemmerich, Nikolas, additional, Kimura, Masato, additional, Kuzniak, Marcin, additional, La Commara, Marco, additional, Matteucci, Giuseppe, additional, Moura Santos, Edivaldo, additional, Oleynikov, Vladislav, additional, Perez Varona, Ramon, additional, Pino, Noemi, additional, Puglia, Sebastiana M.R., additional, Rescigno, Marco, additional, Sales Costa, Barbara, additional, Sanfilippo, Simone, additional, Sunny, Clea, additional, Suvorov, Yury, additional, Tartaglia, Roberto, additional, Testera, Gemma, additional, Tricomi, Alessia, additional, Wada, Masayuki, additional, Wang, Yi, additional, Wojaczynski, Rafal, additional, and Zakhary, Paules, additional

Published
2024
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3. Radiation Damage by Heavy Ions in Silicon and Silicon Carbide Detectors

Author

Altana, Carmen, primary, Calcagno, Lucia, additional, Ciampi, Caterina, additional, La Via, Francesco, additional, Lanzalone, Gaetano, additional, Muoio, Annamaria, additional, Pasquali, Gabriele, additional, Pellegrino, Domenico, additional, Puglia, Sebastiana, additional, Rapisarda, Giuseppe, additional, and Tudisco, Salvatore, additional

Published
2023
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4. Trojan Horse Method for n-induced reaction investigations at astrophysical energies

Author

Sergi, Maria Letizia, primary, Lamia, Livio, additional, Rapisarda, Giuseppe Gabriele, additional, Mazzocco, Marco, additional, Cherubini, Silvio, additional, D'Agata, Giuseppe, additional, Di Pietro, Alessia, additional, Fernandez-Garcia, Juan Pablo, additional, Figuera, Pierpaolo, additional, Fisichella, Maria, additional, Guardo, Giovanni L., additional, Gulino, Marisa, additional, Hayakawa, Seiya, additional, La Cognata, Marco, additional, Lattuada, Marcello, additional, Oliva, Alessandro Alberto, additional, Palmerini, Sara, additional, Pizzone, Rosario G., additional, Puglia, Sebastiana Maria Regina, additional, Romano, Stefano, additional, Spartà, Roberta, additional, Spitaleri, Claudio, additional, Torresi, Domenico, additional, and Tumino, Aurora, additional

Published
2022
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5. The 10B(p,α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method

Author

Puglia Sebastiana Maria Regina, Spitaleri Claudio, La Cognata Marco, Lamia Livio, Broggini Carlo, Caciolli Antonio, Carlin Nelson, Cherubini Silvio, Cvetinovic Alexandra, D’Agata Giuseppe, Dell’aquila Daniele, Depalo Rosanna, Gulino Marisa, Guardo Giovanni Luca, Indelicato Iolanda, Lombardo Ivano, Menegazzo Roberto, Munhoz Marcelo Gimenez, Pizzone Rosario Gianluca, Rapisarda Giuseppe Gabriele, Rigato Valentino, Romano Stefano, Sergi Maria Letizia, Souza Francisco, Sparta Roberta, Tudisco Salvo, and Tumino Aurora

Subjects
Physics, QC1-999
Abstract

The 10B(p,α)7Be reaction is the main responsible for the 10B destruction in stellar interior [1]. In such environments this p-capture process occurs at a Gamow energy of 10 keV and takes places mainly through a resonant state (Ex = 8.701 MeV) of the compound 11C nucleus. Thus a resonance right in the region of the Gamow peak is expected to significantly influence the behavior of the astrophysical S(E)-factor. The 10B(p,α)7Be reaction was studied via the Trojan Horse Method (THM) applied to the 2H(10B,α7Be)n in order to extract the astrophysical S(E)-factor in a wide energy range from 5 keV to 1.5 MeV.

Published
2017
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6. New direct measurement of the 10B(p,α)7Be reaction with the activation technique

Author

Depalo Rosanna, Caciolli Antonio, Broggini Carlo, La Cognata Marco, Lamia Livio, Menegazzo Roberto, Mou Liliana, Puglia Sebastiana Maria Regina, Rigato Valentino, Romano Stefano, Alvarez Carlos Rossi, Sergi Maria Letizia, Spitaleri Claudio, and Tumino Aurora

Subjects
Physics, QC1-999
Abstract

Boron plays an important role in astrophysics and, together with lithium and beryllium, is a probe of stellar structure during the pre-main sequence and main-sequence phases. In this context, the 10B(p,α)7 Be reaction is of particular interest. The literature data show discrepancies in the energy range between 100 keV and 2 MeV. This also poses a normalization problem for indirect data obtained with the Trojan Horse Method. A new measurement of the 10B(p,α)7 Be reaction cross section was performed at Legnaro National Laboratories (LNL). At LNL, the cross section was determined with the activation technique by measuring the activated samples at a low-background counting facility. The analysis of that experiment is now complete and the results are here presented.

Published
2017
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7. An Irradiation Test Facility at INFN-LNS: Status and Perspectives

Author

Rapisarda, Giuseppe, Bonanno, Vincenza, Catalano, Roberto, Cirrone, Giuseppe, Cosentino, Luigi, Cuttone, Giacomo, Mascali, David, Musumeci, Mario, Petringa, Giada, Puglia, Sebastiana, Rifuggiato, Danilo, and Salvatore, Tudisco

Subjects
Applications, Accelerator Physics
Abstract

In the framework of ASIF "ASI Supported Irradiation Facilities" project some beamlines available at Laboratori Nazionali del Sud-INFN (LNS) Catania have been dedicated to irradiation test. These beamlines have been recently upgraded in order to meet the ESA specifications about radiation hardness testing of devices suitable for space applications. The Superconducting Cyclotron K800 installed at LNS can provide protons up to 80 MeV for integrated dose tests and a number of heavy ion beams for Single Event Effect (SEE) studies. The beamlines are equipped with detectors that allow beam diagnostic in term of spatial uniformity, purity and energy measurement, including on-line monitoring of flux and fluence received by the device under test. Upgrades activities are now ongoing, especially to broaden up the number of available beams, both in terms of ion species and energy, to optimize the switching times from one beam to another. The paper will present an overview of the developed facility, which will take benefit of the ongoing SERSE (the superconducting ECR ion source) revamping: the new gas-box system, plasma chamber and controls system are ready to be installed within autumn 2018., Proceedings of the 23th Int. Workshop on ECR Ion Sources, ECRIS2018, Catania, Italy

Published
2019
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8. Measurement of the 10B( p,α0)7Be cross section from 5 keV to 1.5 MeV in a single experiment using the Trojan horse method

Author

Spitaleri, C., Puglia, Sebastiana, La Cognata, M., Lamia, L., Cherubini, Silvio, Cvetinovi´c, A., D’Agata, G., Gulino, M., Guardo, G. L., Indelicato, I., Pizzone, R. G., Rapisarda, G. G., Romano, Stefano, Sergi, M. L., Spartà, R., Tudisco, S., Tumino, A., Gimenez Del Santo, M., Carlin, N., Munhoz, M. G., Souza, F. A., Szanto de Toledo, A., Mukhamedzhanov, † A., Broggini, C., Caciolli, A., Depalo, R., Menegazzo, R., Rigato, V., Lombardo, I., and Dell’Aquila, D.

Subjects
NUCLEI, REACTION-RATES, REACTION-RATES, COMPILATION, NUCLEI, COMPILATION
Published
2017

9. SiCILIA—Silicon Carbide Detectors for Intense Luminosity Investigations and Applications

Author

Tudisco, Salvatore, primary, La Via, Francesco, additional, Agodi, Clementina, additional, Altana, Carmen, additional, Borghi, Giacomo, additional, Boscardin, Maurizio, additional, Bussolino, Giancarlo, additional, Calcagno, Lucia, additional, Camarda, Massimo, additional, Cappuzzello, Francesco, additional, Carbone, Diana, additional, Cascino, Salvatore, additional, Casini, Giovanni, additional, Cavallaro, Manuela, additional, Ciampi, Caterina, additional, Cirrone, Giuseppe, additional, Cuttone, Giacomo, additional, Fazzi, Alberto, additional, Giove, Dario, additional, Gorini, Giuseppe, additional, Labate, Luca, additional, Lanzalone, Gaetano, additional, Litrico, Grazia, additional, Longo, Giuseppe, additional, Lo Presti, Domenico, additional, Mauceri, Marco, additional, Modica, Roberto, additional, Moschetti, Maurizio, additional, Muoio, Annamaria, additional, Musumeci, Franco, additional, Pasquali, Gabriele, additional, Petringa, Giada, additional, Piluso, Nicolò, additional, Poggi, Giacomo, additional, Privitera, Stefania, additional, Puglia, Sebastiana, additional, Puglisi, Valeria, additional, Rebai, Marica, additional, Ronchin, Sabina, additional, Santangelo, Antonello, additional, Stefanini, Andrea, additional, Trifirò, Antonio, additional, and Zimbone, Massimo, additional

Published
2018
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10. New direct measurement of the10B(p,α)7Be reaction with the activation technique

Author

Depalo, Rosanna, primary, Caciolli, Antonio, additional, Broggini, Carlo, additional, La Cognata, Marco, additional, Lamia, Livio, additional, Menegazzo, Roberto, additional, Mou, Liliana, additional, Puglia, Sebastiana Maria Regina, additional, Rigato, Valentino, additional, Romano, Stefano, additional, Alvarez, Carlos Rossi, additional, Sergi, Maria Letizia, additional, Spitaleri, Claudio, additional, and Tumino, Aurora, additional

Published
2017
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11. The 10B(p,α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method.

Author

La Cognata, Marco, Cvetinovic, Alexandra, Guardo, Giovanni Luca, Indelicato, Iolanda, Pizzone, Rosario Gianluca, Sergi, Maria Letizia, Regina Puglia, Sebastiana Maria, Lamia, Livio, Cherubini, Silvio, D'Agata, Giuseppe, Rapisarda, Giuseppe Gabriele, Romano, Stefano, Sparta, Roberta, Tudisco, Salvo, Spitaleri, Claudio, Gulino, Marisa, Tumino, Aurora, Rigato, Valentino, Broggini, Carlo, and Menegazzo, Roberto

Subjects
BORON isotopes, BERYLLIUM isotopes, ASTROPHYSICS, PROTON capture, CIRCUMSTELLAR matter, NUCLEAR reactions, THREE-body problem
Abstract

The 10B(p,α)7Be reaction is the main responsible for the 10B destruction in stellar interior [1]. In such environments this p-capture process occurs at a Gamow energy of 10 keV and takes places mainly through a resonant state (Ex = 8.701 MeV) of the compound 11C nucleus. Thus a resonance right in the region of the Gamow peak is expected to significantly influence the behavior of the astrophysical S(E)-factor. The 10B(p,α)7Be reaction was studied via the Trojan Horse Method (THM) applied to the 2H(10B,α7Be)n in order to extract the astrophysical S(E)-factor in a wide energy range from 5 keV to 1.5 MeV. [ABSTRACT FROM AUTHOR]

Published
2017
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12. New direct measurement of the 10B(p,α)7Be reaction with the activation technique.

Author

Depalo, Rosanna, Caciolli, Antonio, Broggini, Carlo, Menegazzo, Roberto, La Cognata, Marco, Regina Puglia, Sebastiana Maria, Sergi, Maria Letizia, Romano, Stefano, Spitaleri, Claudio, Tumino, Aurora, Lamia, Livio, Mou, Liliana, Rigato, Valentino, and Alvarez, Carlos Rossi

Subjects
BORON isotopes, NUCLEAR reactions, ACTIVATION cross sections, STELLAR structure, STELLAR mass
Abstract

Boron plays an important role in astrophysics and, together with lithium and beryllium, is a probe of stellar structure during the pre-main sequence and main-sequence phases. In this context, the 10B(p,α)7 Be reaction is of particular interest. The literature data show discrepancies in the energy range between 100 keV and 2 MeV. This also poses a normalization problem for indirect data obtained with the Trojan Horse Method. A new measurement of the 10B(p,α)7 Be reaction cross section was performed at Legnaro National Laboratories (LNL). At LNL, the cross section was determined with the activation technique by measuring the activated samples at a low-background counting facility. The analysis of that experiment is now complete and the results are here presented [ABSTRACT FROM AUTHOR]

Published
2017
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14. Experimental study of the O-18(d, p)O-19 reaction and the ANC Method

Author

Burjan, V, Hons, Z, Kroha, V, Mrazek, J, Piskor, S, Mukhamedzhanov, Am, Trache, L, Tribble, Re, La Cognata, M, Gulino, M, Lamia, Livio, Pizzone, Gr, Puglia, Sebastiana, Rapisarda, G, Romano, Stefano, Sergi, Ml, Sparta, R, Spitaleri, C, and Tumino, A.

Published
2013

15. New measurement of the B-11(p,alpha(0))Be-8 bare-nucleus S(E) factor via the Trojan horse method

Author

Lamia, Livio, Spitaleri, C., Burjan, V., Carlin, N., Cherubini, Silvio, Crucilla, V., Gameiro Munhoz, M., Gimenez Del Santo, M., Gulino, M., Hons, Z., Kiss, G. G., Kroha, V., Kubono, S., La Cognata, M., Li, C., Mrazek, J., Mukhamedzhanov, A., Pizzone, R. G., Puglia, Sebastiana, Wen, Q., Rapisarda, G. G., Rolfs, C., Romano, Stefano, Sergi, M. L., Somorjai, E., Souza, F. A., Szanto de Toledo, A., Tabacaru, G., Tumino, A., Wakabayashi, Y., Yamaguchi, H., and Zhou, S. H.

Published
2012

16. The resonant cross sections of 10,11B(p,a) reactions at astrophysical energies: indirect measurements via the THM

Author

Puglia, Sebastiana Maria Regina

Subjects
NATURAL SCIENCES::Physics::Astronomy and astrophysics::Formation and development of stars [Research Subject Categories], NATURAL SCIENCES::Physics::Nuclear physics::Low energy physics [Research Subject Categories]
Abstract

The study of the nucleosynthesis of the light elements, Lithium, Beryllium and Boron, plays a key role in understanding of several astrophysical problems related to cosmology as well as to stellar structure and evolution. Moreover, the knowledge of their abundances can be a precious tool for the investigation of the inner stellar structure, especially to understand the mixing processes in stellar plasma. These elements, LiBeB, are mainly destroyed in stellar interior through (p,alpha) reactions induced at temperature of the order of 106 K, corresponding to the Gamow energy EG of a few keV's. In this energy region the direct determination of the cross section for charged particle induced reactions is affected by the presence of the Coulomb barrier between the interacting nuclei, and by the electron screening effect. Thus, precise measurements of the cross section for such processes are very complex and sometimes not possible. In the thesis, is presented the study of the 10B(p,alpha)7Be and 11B(p,alpha)8Be reactions which are the main responsible for the Boron destruction in stellar environments. The study of these reactions has been performed by means of the indirect Trojan Horse Method, that allows to overcome the effects due to the presence of the Coulomb barrier and electron screening. The method provides the bare nucleus two-body astrophysical-factor in the energy region of interest for astrophysics, from the quasi-free (QF) contribution of a suitable three-body reaction. The approach allows to avoid the extrapolation, usually made on the direct measurements. The experimental procedure and the results regarding the extracted Sb(E)-factor are reported in the thesis, as well as the electron screening potential Ue determined by means of the comparison with direct data. Lo studio della nucleo sintesi degli elementi leggeri, Litio, Berillio e Boro, svolge un ruolo fondamentale nella comprensione di alcuni problemi astrofisici legati sia alla cosmologia, che alla comprensione della struttura e dell'evoluzione stellare. Inoltre la conoscenza delle abbondanze di tali elementi puo' costituire un prezioso strumento nell'indagine della struttura interna stellare , in particolare nella comprensione dei processi di mixing che avvengono nel plasma stellare. Nelle stelle in fase quiescente, questi elementi,LiBeB, vengono distrutti principalmente attraverso reazioni (p, alpha) indotte alla temperatura dell'ordine di 106 K, corrispondente all'energia di Gamow EG di qualche keV. In questa regione energetica la determinazione diretta della sezione d'urto per reazioni indotte da particelle cariche influenzata dalla presenza della barriera Coulombiana tra i nuclei interagenti, e dall'effetto di screening elettronico. Pertanto per questi processi le misure della sezione d'urto sono molto complesse e a volte non realizzabili. Nella tesi,e' riportato lo studio delle reazioni 10B (p,alpha) 7Be e 11B(p,alpha)8BE che sono le principali reazioni nucleari responsabili della distruzione di Boro in ambiente stellare. Lo studio di queste reazioni e' stato eseguito attraverso il metodo indiretto del Trojan Horse (THM), che permette di superare gli effetti dovuti alla presenza della barriera colombiana e di screening elettronico. Tale metodo fornisce il fattore astrofisico di nucleo nudo Sb(E) nella regione energetica di interesse per l'astrofisica, dalla selezione del contributo quasi-libero (QF) di una opportuna reazione a tre corpi. L' approccio consente di evitare l'estrapolazioni, che di norma vengono usate nelle misure dirette. Nella tesi viene riportata in dettaglio, per entrambe le reazioni suddette, la procedura sperimentale e vengono inoltre mostrati i risultati ottenuti, sia del fattore astrofisico S b(E) che del potenziale di screening elettronico Ue.

Published
2011

24. Indurect measurement of 17 O(p,a)14N cfoss section at ultra-low energy

Author

Sergi, M. L., Spitaleri, C, Coc, A., Mukhamedzhanov, A., Burjan, V., Cherubini, Silvio, Crucillá, V., Gulino, M., Hammache, F., Hons, V. Z., Irgaziev, B., Kiss, G., Kroha, V., LA COGNATA, M., Lamia, L., Pizzone, R. G., Puglia, Sebastiana, Rapisarda, G. G., Romano, S., DE SÉRÉVILLE, N., Somorjai, E., and Tumino, S. TUDISCO AND A.

Published
2010

26. FIRST EXPERIMENTAL MEASURENT OF THE 18O(P,A)15N REACTION AT ASTROPHYSICAL ENERGIES

Author

LA COGNATA, M., Spitaleri, C, Mukhamedzhanov, A., AL ABDDULLAH, T., Banu, A., Cherubini, Silvio, Coc, A., Crucilla, V., Gulino, M., Irgaziev, B., Kiss, G. G., Lamia, L., Mrazek, J., Pizzone, R. G., Puglia, Sebastiana, Rapisarda, GIUSEPPE GABRIELE, Romano, S., Sergi, M. L., Tabacaru, G., Trache, L., Tribble, R. E., Trzaska, W., Tudisco, S., and Tumino, A.

Published
2009

27. Reaction rate of the 18O(p,!)15N reaction at astrophysical temperatures

Author

Lacognata, M., Spitaleri, C, Mukhamedzhanov, A., Tribble, R. E., AL ABDULLAH, T., Banu, A., Cherubini, Silvio, Coc, A., Crucillà, V., Goldberg, V., Gulino, M., Irgaziev, B., Kiss, G. G., Lamia, L., Mrazek, J., Pizzone, R. G., Puglia, Sebastiana, Rapisarda, G., Romano, Stefano, Sergi, M. L., Tabacaru, G., Trache, L., Trzaska, W., Tudisco, S., and Tumino, A.

Published
2009

28. Improvements on the study of 17O(p,!)14N reaction via the Trojan Horse Method at astrophysical energies

Author

Sergi, M. L., Spitaleri, C, Coc, A., Mukhamedzhanov, A., Tang, X., Brian, S., Bucher, B., Burian, Cherubini, Silvio, Couder, M., Crucilla', V., Davies, P., Deboer, R., Gulino, M., Hammache, F., Hons, V. Z., Irgaziev, B., Kiss, G., Kroha, V., Lacognata, M., Lamia, L., Lamm, L., Ma, C., Mrazek, J., Notani, M., Pizzone, R. G., Puglia, Sebastiana, Rapisarda, G. G., Roberson, D., Romano, Stefano, Desereville, N., Somorjai, E., Tan, W., Tudisco, S., and Tumino, A.

Published
2009

29. Nuclear Proton-proton Elastic Scattering via the Trojan Horse Method

Author

Tumino, A., Spitaleri, C, Mukhamedzhanov, A. ), Rapisarda, Gg, Campajola, L, Cherubini, S., Crucilla, V, Elekes, Z, Fulop, Z, Gialanella, L, Gulino, M. ., Gyurky, G., Kiss, Gg, Cognata, La, Lamia, M., Ordine, L, Pizzone, A., R. G., Puglia, Sebastiana, Romano, S, Sergi, Ml, and Somorjai, E.

Published
2009

32. 10B(p, alpha)7Be reaction S(E)-factor at the Gamow energy extracted via the THM

Author

Puglia, Sebastiana, Romano, S., Delsanto, M. G., Lamia, L., Spitaleri, C, Carlin, N., Cherubini, Silvio, Gulino, M., Kroha, V., Kubono, S., Lacognata, M., Li, C., Pizzone, R. G., Munhoz, M. G., Qungang, W., Rapisarda, G. G., Sergi, M. L., Somorjai, E., Souza, F., SZANTO DE TOLEDO, A., Tudisco, S., Tumino, A., Wakabayashi, Y., and Yamaguchi, H.

Published
2009

33. IMPROVED RESULTS ON THE EZTRACTION OF 11B8P,A)8BE AND 10B(P,A)7BE S(E)-FACTOR THROUGH THE INDIRECT TROJAN HORSE METHOD

Author

Lamia, L., Spitaleri, C, Romano, Stefano, Puglia, Sebastiana, GIMENEZ DEL SANTO, M., Carlin, N., Cherubini, Silvio, Crucilla', V., GAMEIRO MUNHOZ, M., Gulino, M., Kiss, G., Kroha, V., Kubono, S., LA COGNATA, M., Li, C., Mukhamedzhanov, A., Pizzone, R. G., Qungang, Wen, Rapisarda, G. G., Sergi, M. L., Somorjai, E., Souza, F. A., SZANTO DE TOLEDO, A., Tabacaru, G., Tudisco, S., Tumino, A., Wakabayashi, Y., and Yamaguchi, H.

Published
2009

34. Improved results on extraction of 11B(p,α0)8Be S(E)-factor through the indirect Trojan Horse Method

Author

Lamia, L., Spitaleri, C, Romano, Stefano, Carlin, N., Cherubini, Silvio, Crucillà, V., DEL SANTO, M. G., Gulino, M., Kiss, G. G., Kroha, V., Kubono, S., LA COGNATA, M., Li, C., Munho, M. G., Pizzone, R. G., Puglia, Sebastiana, Wend, Q., Rapisarda, G. G., Sergi, M. L., Somoryai, E., Souza, F., SZANTO DE TOLEDO, A., Tabacaru, G., Tudisco, S., Tumino, A., Wakabayashi, Y., and Yamaguchi, H.

Published
2009

35. State of the art for the 11B(p,!)8Be reaction studied through the Trojan Horse Method: recent results

Author

Lamia, L., Romano, Stefano, Puglia, Sebastiana, Delsanto, M. G., Spitaleri, C, Carlin, N., Cherubini, Silvio, Crucillà, V., Kiss, M. GULINO G., Kroha, V., Kubono, S., Lacognata, M., CHENG BO LI, Mukhamedzhanov, A., Pizzone, R. G., QUN GANG WEN, Rapisarda, G. G., Sergi, M. L., Somorjai, E., Souza, F., Szantodetoledo, A., Tabacaru, G., Tudisco, S., Tumino, A., Wakabayashi, Y., Yamaguchi, H., and Shu, Huazhou

Published
2009

36. Status of the 18F+p and 18F+d experiment at CRIB

Author

Cherubini, Silvio, Spitaleri, C, Crucilla', V., Gulino, M., Lacognata, M., Lamia, L., Pizzone, R. G., Puglia, Sebastiana, Rapisarda, G. G., Romano, S., Sergi, M. L., Tudisco, S., Tumino, A., Kubono, S., Yamaguchi, H., Wakabayashi, Y., Hayakawa, S., Iwasa, N., Kato, S., Komatsubara, H., Teranishi, T., Coc, A., Hammache, F., and Desereville

Published
2009

40. Recent astrophysical application of the trojanhorse method to nuclear astrophysics

Author

Spitaleri, C, Cherubini, Silvio, Crucilla, V., LA COGNATA, M., Lamia, L., Pizzone, R. G., Puglia, Sebastiana, Rapisarda, G. G., Romano, S., Tumino, M. L. SERGI A., Tribble, R., Banu, A., AL ABULLAH, T., Fu, C., Goldberg, V., MUCHAMED ZHANOV, A., Tabacaru, G., Trache, L., Zhai, Y., Kroha, V., Burjan, V., Homs, Z., Mrazek, J., Somoryai, E., Kiss, G., and Li, C.

Published
2008

43. Electron Screening in fusion reactions

Author

Pizzone, R. G., Spitaleri, C, Cherubini, Silvio, Crucilla', V., Gulino, M., LA COGNATA, M., Lamia, Livio, Puglia, Sebastiana, Rapisarda, G. G., Rolfs, C., Romano, Stefano, Sergi, M. L., and Tumino, A.

Published
2008

46. Measurement of the 18F(p,alpha)15O reaction in nova conditions

Author

Cherubini, Silvio, Spitaleri, C., Crucilla', V., Gulino, M., LA COGNATA, M., Lamia, Livio, Pizzone, R. G., Puglia, Sebastiana, Rapisarda, G. G., Romano, Stefano, Sergi, M. L., Tumino, A., Kubono, S., Yamaguchi, H., Wakabayashi, Y., Hayakawa, S., Amadio, G., Iwasa, N., Kato, S., Komatsubara, Y., Nishimura, S., Teranishi, T., Coc, A., and DE SEREVILLE, N.

Published
2008

50. Light elements depletion: indirect measurement of the Boron depleting reactions

Author

Romano, S, Spitaleri, C, Cherubini, Silvio, Crucilla', V, LA COGNATA, M, Lamia, Livio, Pizzone, R. G., Puglia, Sebastiana, Rapisarda, G. G., Sergi, M. L., Tudisco, S, Tumino, A, Goldberg, V. Z., Mukhamedzhanov, A, Tribble, R, Trache, L, Kroha, V, Somorjai, E, ZSANTO DE TOLEDO, A, Zhou, S, and Kubono, S.

Published
2008

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