Zobrazeno 1 - 10
of 5 626
pro vyhledávání: '"Lattuada"'
Autor:
Palada Luka, Soić Neven, Acosta Louis, Bailey Sam, Dell’Aquila Daniele, Duenas Jose Antonio, Fernandez-Garcia Juan Pablo, Figuera Pierpaolo, Fioretto Enrico, Fisichella Maria, Grassi Laura, Kirsebom Oliver, Kokalova Wheldon Tzany, Lattuada Marcello, Marquinez-Duran Gloria, Martel Ismael, Mijatović Tea, Prepolec Lovro, Skukan Natko, Smith Robin, Szilner Suzana, Tokić Vedrana, Uroić Milivoj, Vukman Nikola, Walshe Joe, Wheldon Carl
Publikováno v:
EPJ Web of Conferences, Vol 311, p 00025 (2024)
Measurement was conducted at the INFN-LNL, employing a Tandem accelerator to achieve a 95 MeV 14N beam focused on 10B target (201 µg/cm²) with the aim to explore the cluster structures of light carbon isotopes. The main focus of this report will be
Externí odkaz:
https://doaj.org/article/41dbf370386244b39aeb4751a61de12b
Autor:
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., Rapisarda G.G., Romano S., Santonocito D., Spartà R., Sergi M.L., Tumino A., Ventura P.
Publikováno v:
EPJ Web of Conferences, Vol 306, p 01010 (2024)
In astrophysics, the abundance of 26Al is essential for understanding nucleosynthesis in the Milky Way and Galactic core-collapse supernovae rates. Detection methods involve γ-ray lines and comparing 26Mg overabundance with the common Mg isotope in
Externí odkaz:
https://doaj.org/article/3d9845f862ff458183f7582742da937b
Autor:
Scisciò, M., Petringa, G., Zhu, Z., Rodrigues, M. R. D., Alonzo, M., Andreoli, P. L., Filippi, F., Consoli, Fe., Huault, M., Raffestin, D., Molloy, D., Larreur, H., Singappuli, D., Carriere, T., Verona, C., Nicolai, P., McNamee, A., Ehret, M., Filippov, E., Lera, R., Pérez-Hernández, J. A., Agarwal, S., Krupka, M., Singh, S., Istokskaia, V., Lattuada, D., La Cognata, M., Guardo, G. L., Palmerini, S., Rapisarda, G., Batani, K., Cipriani, M., Cristofari, G., Di Ferdinando, E., Di Giorgio, G., De Angelis, R., Giulietti, D., Xu, J., Volpe, L., Rodríguez-Frías, M. D., Giuffrida, L., Margarone, D., Batani, D., Cirrone, G. A. P., Bonasera, A., Consoli, Fa.
Driving the nuclear fusion reaction p+11B -> 3 alpha + 8.7 MeV in laboratory conditions, by interaction between high-power laser pulses and matter, has become a popular field of research, due to numerous applications that it can potentially allow: an
Externí odkaz:
http://arxiv.org/abs/2411.04577
Autor:
Sergi Maria Letizia, Lamia Livio, Cherubini Silvio, D’Agata Giuseppe, Di Pietro Alessia, Fernandez-Garcia Juan Pablo, Figuera Pierpaolo, Guardo Giovanni Luca, Gulino Marisa, Hayakawa Seiya, Indelicato Iolanda, La Cognata Marco, La Commara Marco, Lattuada Dario, Lattuada Marcello, Mazzocco Marco, Oliva Alessandro Alberto, Palmerini Sara, Pizzone Rosario Gianluca, Rapisarda Giuseppe Gabriele, Romano Stefano, Spartà Roberta, Spitaleri Claudio, Torresi Domenico, Tumino Aurora
Publikováno v:
EPJ Web of Conferences, Vol 290, p 03002 (2023)
Neutron induced reactions on stable and unstable nuclei play a significant role in the nucleosynthesis of the elements in the cosmos. In the last years, several efforts have been made to investigate the possibility of applying the Trojan Horse Method
Externí odkaz:
https://doaj.org/article/9a9a09e3f10b4f3ba0fcf2320d1f0b47
Autor:
Manzoni G, Oltolini A, Perra S, Muraca E, Ciardullo S, Pizzi M, Castoldi G, Lattuada G, Pizzi P, Perseghin G
Publikováno v:
Diabetes, Metabolic Syndrome and Obesity, Vol Volume 13, Pp 489-497 (2020)
Giuseppina Manzoni,1 Alice Oltolini,1 Silvia Perra,1 Emanuele Muraca,1 Stefano Ciardullo,1,2 Mattia Pizzi,3 Giovanna Castoldi,2 Guido Lattuada,1 Pietro Pizzi,3 Gianluca Perseghin1,2 1Department of Medicine and Rehabilitation, Policlinico di Monza, Mo
Externí odkaz:
https://doaj.org/article/bf5067564fbc414fb0d70ffbffb85da1
Autor:
La Cognata M., Kiss G. G., Yarmukhamedov R., Tursunmakhatov K. I., 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., Spitaleri C., Trippella O., Tumino A., Anastasiou M., Kuvin S. A., Rijal N., Schmidt B., Igamov S. B., Sakuta S. B., Fülöp Zs., Gyürky Gy., Szücs T., Halász Z., Somorjai E., Hons Z., Mrázek J., Tribble R. E., Mukhamedzhanov A. M.
Publikováno v:
EPJ Web of Conferences, Vol 279, p 11001 (2023)
The p - p-chain reaction 3He(α, γ)7Be can sensitively influence the prediction of the 7Be and 8B neutrino fluxes. Despite its importance, the knowledge of its reaction cross section at energies of the core of the Sun (15 keV 30 keV) is limited and
Externí odkaz:
https://doaj.org/article/35441615cd0c4307a522d4b4a7dbca39
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:
Yamaguchi H., Hayakawa S., Ma N.R., Shimizu H., Okawa K., Zhang Q., Yang L., Kahl D., La Cognata M., Lamia L., Abe K., Beliuskina O., Cha S.M., Chae K.Y., Cherubini S., Figuera P., Ge Z., Gulino M., Hu J., Inoue A., Iwasa N., Kim A., Kim D., Kiss G., Kubono S., La Commara M., Lattuada M., Lee E.J., Moon J.Y., Palmerini S., Parascandolo C., Park S.Y., Phong V.H., Pierroutsakou D., Pizzone R.G., Rapisarda G.G., Romano S., Spitaleri C., Tang X.D., Trippella O., Tumino A., Zhang N.T., Lam Y.H., Heger A., Jacobs A.M., Xu S.W., Ma S.B., Ru L.H., Liu E.Q., Liu T., Hamill C.B., Murphy A. St J., Su J., Fang X., Kwag M.S., Duy N.N., Uyen N.K., Kim D.H., Liang J., Psaltis A., Sferrazza M., Johnston Z., Li Y.Y.
Publikováno v:
EPJ Web of Conferences, Vol 275, p 01015 (2023)
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://doaj.org/article/bddb2deee4b24a159b646a7fe3f55ce2
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:
Yamaguchi H., Hayakawa S., Ma N.R., Shimizu H., Okawa K., Yang L., Kahl D., La Cognata M., Lamia L., Abe K., Beliuskina O., Cha S.M., Chae K.Y., Cherubini S., Figuera P., Ge Z., Gulino M., Hu J., Inoue A., Iwasa N., Kim A., Kim D., Kiss G., Kubono S., La Commara M., Lattuada M., Lee E.J., Moon J.Y., Palmerini S., Parascandolo C., Park S.Y., Phong V. H., Pierroutsakou D., Pizzone R.G., Rapisarda G.G., Romano S., Spitaleri C., Tang X.D., Trippella O., Tumino A., Zhang N.T., Lam Y.H., Heger A., Jacobs A.M., Xu S.W., Ma S.B., Ru L.H., Liu E.Q., Liu T., Hamill C.B., St J. Murphy A., Su J., Fang X., Kwag M.S., Duy N.N., Uyen N.K., Kim D.H., Liang J, Psaltis A., Sferrazza M., Johnston Z., Li Y.Y.
Publikováno v:
EPJ Web of Conferences, Vol 260, p 03003 (2022)
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://doaj.org/article/b0873e80403540bca7a4d103f879a4d0