Zobrazeno 1 - 10
of 161
pro vyhledávání: '"Guardo L."'
Autor:
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.
Publikováno v:
EPJ Web of Conferences, Vol 279, p 11015 (2023)
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://doaj.org/article/5b9ac92064e548e5934bc79d9585bcb4
Autor:
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.
Publikováno v:
EPJ Web of Conferences, Vol 275, p 02010 (2023)
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://doaj.org/article/fb801b18186444e28ca2d5221be2d83c
Autor:
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.
Publikováno v:
EPJ Web of Conferences, Vol 184, p 02012 (2018)
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 Treiman-Yang (TY) Criterion is a model-independent experimental test for the dominance of th
Externí odkaz:
https://doaj.org/article/62acf7d6879c43c1ba3bfd4737e4acb6
Autor:
Tumino A., Spitaleri C., Cherubini S., Guardo L., Gulino M., Indelicato I., La Cognata M., Lamia L., Pizzone R.G., Puglia S.M.R., Rapisarda G.G., Romano S., Sergi M.L., Spartá R.
Publikováno v:
EPJ Web of Conferences, Vol 117, p 09004 (2016)
A measurement of the 12C(14N,α20Ne)2H and 12C(14N,p23Na)2Hreactions has been performed at a 14N beam energy of 30.0 MeV. The experiment aims to explore the extent to which contributing 24Mg excited states can be populated in the quasi-free reaction
Externí odkaz:
https://doaj.org/article/c303374783df43aaaee61f27f1119deb
Akademický článek
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Akademický článek
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Autor:
D'Agata, G, Kilic, Ai, Burjan, V, Mrazek, J, Glagolev, V, Kroha, V, Cassisa, A, Guardo, L, La Cognata, M, Lamia, L, Palmerini, S, Pizzone, Rg, Rapisarda, Gg, Romano, S, Sergi, Ml, Sparta, R, Spitaleri, C, Tumino, A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3982::d32e11406c7a0da64020749b76847ba4
https://hdl.handle.net/11391/1553501
https://hdl.handle.net/11391/1553501
Autor:
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., Redondo, D. G., Guardo, L., Gulino, M., Hammache, F., Malenica, D. J., Kilic, A. I., La Cognata, M., La Commara, M., Lamia, L., Lattuada, D., Maiolino, C., Manico, G., Mazzocco, M., Milin, M., Nanru, M., 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., Sparta, R., Spiridon, A., Trache, L., Vukan, N., Yamaguchi, H.
The 12C + 16O fusion reaction plays a role in the later stages of carbon burning, influencing the evolution of both massive stars and Type Ia Supernovae: when most of the carbon is depleted, by the main fusion reaction 12C + 12C, the abundance of 16O
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::ba7a47b5f060e5879305f7729351b900
https://hdl.handle.net/11391/1544496
https://hdl.handle.net/11391/1544496
Autor:
Filippi, F., Serra, N., Vigano, P., Boeri, L., Cimminiello, C., Di Guardo, L., Somigliana, E., Del Vecchio, M.
Publikováno v:
Melanoma research. 32(5)
The advent of immunotherapy and targeted therapy has outstandingly improved the prognosis in subjects with melanoma. Their use is now advocated also in earlier stages as an adjuvant therapy, and some neoadjuvant clinical trials are ongoing. Consequen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4cffada8ff07e45208df3e4baed649bb
https://pubmed.ncbi.nlm.nih.gov/35855660
https://pubmed.ncbi.nlm.nih.gov/35855660
Autor:
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.
Publikováno v:
EPJ Web of Conferences; 3/22/2023, Vol. 279, p1-4, 4p