Zobrazeno 1 - 10
of 393
pro vyhledávání: '"D. Pierroutsakou"'
Autor:
L. Yang, C. J. Lin, H. Yamaguchi, A. M. Moro, N. R. Ma, D. X. Wang, K. J. Cook, M. Mazzocco, P. W. Wen, S. Hayakawa, J. S. Wang, Y. Y. Yang, G. L. Zhang, Z. Huang, A. Inoue, H. M. Jia, D. Kahl, A. Kim, M. S. Kwag, M. La Commara, G. M. Gu, S. Okamoto, C. Parascandolo, D. Pierroutsakou, H. Shimizu, H. H. Sun, M. L. Wang, F. Yang, F. P. Zhong
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-8 (2022)
Halo-structured nuclei are examples of many-body open quantum system. Here the authors use a complete kinematics measurement and find an elastic breakup of proton halo nucleus 8B.
Externí odkaz:
https://doaj.org/article/ccee6a9f65054474ab440552bb27e45f
Autor:
L. Yang, C.J. Lin, H. Yamaguchi, Jin Lei, P.W. Wen, M. Mazzocco, N.R. Ma, L.J. Sun, D.X. Wang, G.X. Zhang, K. Abe, S.M. Cha, K.Y. Chae, A. Diaz-Torres, J.L. Ferreira, S. Hayakawa, H.M. Jia, D. Kahl, A. Kim, M.S. Kwag, M. La Commara, R. Navarro Pérez, C. Parascandolo, D. Pierroutsakou, J. Rangel, Y. Sakaguchi, C. Signorini, E. Strano, X.X. Xu, F. Yang, Y.Y. Yang, G.L. Zhang, F.P. Zhong, J. Lubian
Publikováno v:
Physics Letters B, Vol 813, Iss , Pp 136045- (2021)
The mechanism of reactions with weakly-bound proton-rich nuclei at energies near the Coulomb barrier is a long-standing open question owing to the paucity of experimental data. In this study, a complete kinematics measurement was performed for the pr
Externí odkaz:
https://doaj.org/article/8e78059dd2d845d2ab4b074fbe7f9db3
Autor:
A. A. Oliva, A. Tumino, N. Soic, P. M. Prajapati, L. Acosta, R. Alba, F. Barba, S. Cherubini, G. D’Agata, D. Dell’Aquila, A. Di Pietro, J.P. Fernandez, P. Figuera, D. Galaviz Redondo, L. Guardo, M. Gulino, F. Hammache, D. Jelavic Malenica, A.I. Kiliç, M. La Cognata, M. La Commara, L. Lamia, D. Lattuada, C. Maiolino, G. Manicò, M. Mazzocco, M. Milin, Ma Nanru, A. Nurmukhanbetova, D. Nurkic, S. Palmerini, T. Parascandolo, D. Pierroutsakou, R.G. Pizzone, R. Popocovski, G.G. Rapisarda, S. Romano, D. Santonocito, M.L. Sergi, A. Shotter, R. Spartà, A. Spiridon, L. Trache, N. Vukman, H. Yamaguchi
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 depleted and its abundance is lower than 16O, the 12C +16 O fusion can also become relevant. Mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d6ccaa6cadc3b0aabcc2a45eff433f6
https://hdl.handle.net/20.500.11769/558663
https://hdl.handle.net/20.500.11769/558663
Autor:
H. Yamaguchi, S. Hayakawa, N.R. Ma, H. Shimizu, K. Okawa, Q. Zhang, L. Yang, D. Kahl, M. La Cognata, L. Lamia, K. Abe, 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, Y.H. Lam, A. Heger, A.M. Jacobs, S.W. Xu, S.B. Ma, L.H. Ru, E.Q. Liu, T. Liu, C.B. Hamill, A. St J. Murphy, J. Su, X. Fang, M.S. Kwag, N.N. Duy, N.K. Uyen, D.H. Kim, J. Liang, A. Psaltis, M. Sferrazza, Z. Johnston, Y.Y. Li
Astrophysical reactions involving radioactive isotopes (RI) often play an important role in high-temperature stellar environments. The experimental studies on the reaction rates for those are still limited mainly due to the technical difficulties in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a57900e370742a76d423f6cf84bdac3d
https://hdl.handle.net/20.500.11769/558667
https://hdl.handle.net/20.500.11769/558667
Autor:
A.A. Oliva, A. Tumino, N. Soic, M.P. Prajapati, L. Acosta, R. Alba, F. Barba, S. Cherubini, G. D’Agata, D. Dell’Aquila, A. Di Pietro, P.J. Fernandez, P. Figuera, D. Galaviz Redondo, L. Guardo, M. Gulino, F. Hammache, D. Jelavic Malenica, A.I. Kiliç, M. La Cognata, M. La Commara, L. Lamia, D. Lattuada, C. Maiolino, G. Manicò, M. Mazzocco, M. Milin, Ma Nanru, A. Nurmukhanbetova, D. Nurkic, S. Palmerini, T. Parascandolo, D. Pierroutsakou, R.G. Pizzone, R. Popocovski, G.G. Rapisarda, S. Romano, D. Santonocito, M.L. Sergi, A. Shotter, R. Spartà, A. Spiridon, L. Trache, N. Vukman, H. Yamaguchi
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 of 16O produced during the later stages of the heliumburning,the 12C+16O fusion can also be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::30ec1accd2af6e1d0672088ddc277306
https://hdl.handle.net/20.500.11769/558666
https://hdl.handle.net/20.500.11769/558666
Autor:
C. Parascandolo, D. Pierroutsakou, R. Alba, A. Del Zoppo, C. Maiolino, D. Santonocito, C. Agodi, V. Baran, A. Boiano, M. Colonna, R. Coniglione, E. De Filippo, A. Di Nitto, U. Emanuele, F. Farinon, A. Guglielmetti, G. Inglima, M. La Commara, G. La Rana, B. Martin, C. Mazzocchi, M. Mazzocco, C. Rizzo, M. Romoli, M. Sandoli, C. Signorini, R. Silvestri, F. Soramel, A. Trifirò, M. Trimarchi, E. Vardaci
Publikováno v:
Physical Review C. 105
Akademický článek
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Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
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Autor:
H. Yamaguchi, S. Hayakawa, N.R. Ma, H. Shimizu, K. Okawa, L. Yang, D. Kahl, M. La Cognata, L. Lamia, K. Abe, 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, Y.H. Lam, A. Heger, A.M. Jacobs, S.W. Xu, S.B. Ma, L.H. Ru, E.Q. Liu, T. Liu, C.B. Hamill, A. St J. Murphy, J. Su, X. Fang, M.S. Kwag, N.N. Duy, N.K. Uyen, D.H. Kim, J Liang, A. Psaltis, M. Sferrazza, Z. Johnston, Y.Y. Li
Experimental studies on astrophysical reactions involving radioactive isotopes (RI) often accompany technical challenges. Studies on such nuclear reactions have been conducted at the low-energy RI beam separator CRIB, operated by Center for Nuclear S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0419ef379b9a9e507c736707744899fb
https://hdl.handle.net/20.500.11769/558670
https://hdl.handle.net/20.500.11769/558670
Publikováno v:
Handbook of Nuclear Physics ISBN: 9789811588181
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ec1ae122f2a881ad41807588c1bbb84b
https://doi.org/10.1007/978-981-15-8818-1_67-1
https://doi.org/10.1007/978-981-15-8818-1_67-1