Zobrazeno 1 - 10
of 27
pro vyhledávání: '"SPITALERI, C."'
Autor:
Tognelli, E., Degl'Innocenti, S., Moroni, P. G. Prada, Lamia, L., Pizzone, R. G., Tumino, A., Spitaleri, C., Chiavassa, A.
Publikováno v:
published in Front. Astron. Space Sci., 13 May 2021, 8, 22
Theoretical prediction of surface stellar abundances of light elements -- lithium, beryllium, and boron -- represents one of the most interesting open problems in astrophysics. As well known, several measurements of 7-Li abundances in stellar atmosph
Externí odkaz:
http://arxiv.org/abs/2107.02518
Autor:
Lan, H. Y., Xu, Y., Luo, W., Balabanski, D. L., Goriely, S., La Cognata, M., Matei, C., Anzalone, A., Chesnevskaya, S., Guardo, G. L., Lattuada, D., Pizzone, R. G., Romano, S., Spitaleri, C., Taffara, A., Tumino, A., Zhu, Z. C.
Photodisintegration reaction rates involving charged particles are of relevance to the p-process nucleosynthesis that aims at explaining the production of the stable neutron-deficient nuclides heavier than iron. In this study, the cross sections and
Externí odkaz:
http://arxiv.org/abs/1810.04958
Autor:
Tumino, A., Spitaleri, C., La Cognata, M., Cherubini, S., Guardo, G. L., Gulino, M., Hayakawa, S., Indelicato, I., Lamia, L., Petrascu, H., Pizzone, R. G., Puglia, S. M. R., Rapisarda, G. G., Romano, S., Sergi, M. L., Spartá, R., Trache, L.
The goal of this reply is to draw attention of the readers that the major problems rose in the short Comment authored by A.M. Mukhamedzhanov, X. Tang and D.Y. Pang (arXiv:1806.05921) are totally groundless.
Comment: 4 pages, 2 figures
Comment: 4 pages, 2 figures
Externí odkaz:
http://arxiv.org/abs/1807.06148
Autor:
Bertulani, C. A., Spitaleri, C.
Electron screening changes appreciably the magnitude of astrophysical nuclear reactions within stars. This effect is also observed in laboratory experiments on Earth, where atomic electrons are present in the nuclear targets. Theoretical models were
Externí odkaz:
http://arxiv.org/abs/1710.03388
Autor:
Dell'Aquila, D., Lombardo, I., Verde, G., Vigilante, M., Acosta, L., Agodi, C., Cappuzzello, F., Carbone, D., Cavallaro, M., Cherubini, S., Cvetinovic, A., D'Agata, G., Francalanza, L., Guardo, G. L., Gulino, M., Indelicato, I., La Cognata, M., Lamia, L., Ordine, A., Pizzone, R. G., Puglia, S. M. R., Rapisarda, G. G., Romano, S., Santagati, G., Spartà, R., Spadaccini, G., Spitaleri, C., Tumino, A.
Publikováno v:
Phys. Rev. Lett. 119, 132501 (2017)
The decay path of the Hoyle state in $^{12}$C ($E_x=7.654\textrm{MeV}$) has been studied with the $^{14}\textrm{N}(\textrm{d},\alpha_2)^{12}\textrm{C}(7.654)$ reaction induced at $10.5\textrm{MeV}$. High resolution invariant mass spectroscopy techniq
Externí odkaz:
http://arxiv.org/abs/1705.09196
Autor:
Li, Chengbo, Wen, Qungang, Fu, Yuanyong, Zhou, Jing, Zhou, Shuhua, Meng, Qiuying, Spitaleri, C., Tumino, A., Pizzone, R. G., Lamia, L.
Publikováno v:
Phys. Rev. C 95, 035804 (2017)
The $\mathrm{^2H}(d,p)\mathrm{^3H}$ bare nucleus astrophysical S(E) factor has been measured indirectly at energies from about 500 keV down to several keV by means of the Trojan-horse method applied to the quasi-free process $\mathrm{^2H({}^6Li},pt)\
Externí odkaz:
http://arxiv.org/abs/1607.00899
Autor:
Caciolli, A., Depalo, R., Broggini, C., La Cognata, M., Lamia, L., Menegazzo, R., Mou, L., Puglia, S. M. R., Rigato, V., Romano, S., Alvarez, C. Rossi, Sergi, M. L., Spitaleri, C., Tumino, A.
The $^{10}$B(p,$\alpha$)$^{7}$Be reaction is of great interest since it has many applications in different fields of research such as nuclear astrophysics, nuclear physics, and models of new reactors for clean energy generation. This reaction has bee
Externí odkaz:
http://arxiv.org/abs/1604.04456
Autor:
Cherubini, S., Gulino, M., Spitaleri, C., Rapisarda, G. G., La Cognata, M., Lamia, L., Pizzone, R. G., Romano, S., Kubono, S., Yamaguchi, H., Hayakawa, S., Wakabayashi, Y., Iwasa, N., Kato, S., Komatsubara, T., Teranishi, T., Coc, A., de Séréville, N., Hammache, F., Kiss, G., Bishop, S., Binh, D. N.
Measurement of nuclear cross sections at astrophysical energies involving unstable species is one of the most challenging tasks in experimental nuclear physics. The use of indirect methods is often unavoidable in this scenario. In this paper the Troj
Externí odkaz:
http://arxiv.org/abs/1505.00593
Autor:
Li, Chengbo, Wen, Qungang, Fu, Yuanyong, Zhou, Jing, Zhou, Shuhua, Meng, Qiuying, Spitaleri, C., Tumino, A., Pizzone, R. G., Lamia, L.
Publikováno v:
Phys. Rev. C 92, 025805 (2015)
The study of d(d,p)t reaction is very important for the nucleosynthesis in both standard Big Bang and stellar evolution, as well as for the future fusion reactors planning of energy production. The d(d,p)t bare nucleus astrophysical S(E) factor has b
Externí odkaz:
http://arxiv.org/abs/1503.08672
Accurate measurements of nuclear reactions of astrophysical interest within, or close to, the Gamow peak, show evidence of an unexpected effect attributed to the presence of atomic electrons in the target. The experiments need to include an effective
Externí odkaz:
http://arxiv.org/abs/1503.05266