Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Qungang Wen"'
Autor:
G.G. Rapisarda, L. Lamia, A. Caciolli, Chengbo Li, S. Degl’Innocenti, R. Depalo, S. Palmerini, R.G. Pizzone, S. Romano, C. Spitaleri, E. Tognelli, Qungang Wen
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 7 (2021)
Light elements offer a unique opportunity for studying several astrophysical scenarios from Big Bang Nucleosynthesis to stellar physics. Understanding the stellar abundances of light elements is key to obtaining information on internal stellar struct
Externí odkaz:
https://doaj.org/article/b82d8df3aff2472fa1e871fb0ada7b8b
Autor:
L. Lamia, Qungang Wen, C. Spitaleri, R. G. Pizzone, Chengbo Li, Qiuying Meng, Jing Zhou, Shuhua Zhou, A. Tumino, Yuanyong Fu
Publikováno v:
Physical Review C. 95
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fe361f5980f74a8945ed423f98442071
https://doi.org/10.1103/physrevc.95.039905
https://doi.org/10.1103/physrevc.95.039905
Autor:
Shuhua Zhou, Qiuying Meng, Jing Zhou, Claudio Spitaleri, M. Lattuada, Chengbo Li, Marco La Cognata, Qungang Wen, Livio Lamia, B. F. Irgaziev, Yuanyong Fu
Publikováno v:
Physical Review C. 93
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b14ae20d2767c3c87df38e2b11f780d5
https://doi.org/10.1103/physrevc.93.039902
https://doi.org/10.1103/physrevc.93.039902
Autor:
Chengbo Li, C. Spitaleri, Shuhua Zhou, A. Tumino, Jing Zhou, Qiuying Meng, Yuanyong Fu, R. G. Pizzone, L. Lamia, Qungang Wen
Publikováno v:
Physical Review C. 92
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:
https://explore.openaire.eu/search/publication?articleId=doi_________::4416116aa936ed2332dcc0d2aea12291
https://doi.org/10.1103/physrevc.92.025805
https://doi.org/10.1103/physrevc.92.025805
Autor:
Silvio Cherubini, Qungang Wen, J. Mrazek, Livio Lamia, H. Yamaguchi, M. Mukhamedzhanov, L. Sergi, V. Kroha, N. Carlin, Marcelo Gameiro Munhoz, C. Spitaleri, M. R. Puglia, B. F. Irgaziev, S. Romano, Sara Palmerini, G. Tabacaru, R. G. Pizzone, M. Gimenez del Santo, A. Tumino, Yusuke Wakabayashi, Marisa Gulino, V. Burjan, G. G. Rapisarda, Chengbo Li, A. Szanto de Toledo, M. La Cognata, E. Somorjai, Z. Hons, S. Zhou, F. A. Souza, V. Crucillà
The accurate knowledge of thermonuclear reaction rates is important in understanding the energy generation, the neutrinos luminosity and the synthesis of elements in stars. The physical conditions under which the majority of astrophysical reactions p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e243691f6210fc0eca0439941587b69
https://hdl.handle.net/20.500.11769/50431
https://hdl.handle.net/20.500.11769/50431
Autor:
Chengo, Li, Qungang, Wen, Yuanyong, Fu, Jing, Zhou, Shuhua, Zhou, Qiuying, Meng, Spitaleri, C., Tumino, A., Pizzone, R. G., Lamia, Livio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4731::7ad916f7187f6cb2485f36fd0d2cd53a
http://hdl.handle.net/20.500.11769/243833
http://hdl.handle.net/20.500.11769/243833
Autor:
V. Kroha, G. G. Rapisarda, Qungang Wen, A. Szanto de Toledo, R. G. Pizzone, A. M. Mukhamedzhanov, E. Somorjai, M. Gimenez del Santo, G. Tabacaru, H. Yamaguchi, S. Zhou, B. F. Irgaziev, A. Tumino, Chengbo Li, M. L. Sergi, J. Mrazek, F. A. Souza, Yusuke Wakabayashi, V. Crucillà, S. M. R. Puglia, C. Spitaleri, M. La Cognata, V. Burjan, S. Romano, Z. Hons, N. Carlin, Livio Lamia, Marcelo Gameiro Munhoz
Publikováno v:
Physical Review C. 90
The $^{10}\mathrm{B}(p,{\ensuremath{\alpha}}_{0})^{7}\mathrm{Be}$ bare nucleus astrophysical $S(E)$ factor has been measured for the first time at energies from about 100 keV down to about 5 keV by means of the Trojan Horse method (THM). In this ener
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e3793e4c7119c6c8139389dbab8ba884
https://doi.org/10.1103/physrevc.90.035801
https://doi.org/10.1103/physrevc.90.035801
Autor:
A. Szanto de Toledo, M. L. Sergi, Shigeru Kubono, Shuhua Zhou, M. La Cognata, R. G. Pizzone, M. Gimenez del Santo, Silvio Cherubini, M. Gameiro Munhoz, C. Spitaleri, Yusuke Wakabayashi, Qungang Wen, S. Romano, Livio Lamia, S. M. R. Puglia, N. Carlin, H. Yamaguchi, Chengbo Li, V. Kroha, G. G. Kiss
Publikováno v:
Nuclear Physics A. 834:655c-657c
Nuclear (p, α ) reactions destroying the so-called “light-elements” lithium, beryllium and boron have been largely studied in the past mainly because their role in understanding some astrophysical phenomena, i.e. mixing-phenomena occurring in yo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8fe48d2c98f0258d2ab22bc3b1ed3906
https://doi.org/10.1016/j.nuclphysa.2010.01.115
https://doi.org/10.1016/j.nuclphysa.2010.01.115
Autor:
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., Yamaguchi, H.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4731::7247b561cecdb11f5d5162284ff4fb8f
http://hdl.handle.net/20.500.11769/75940
http://hdl.handle.net/20.500.11769/75940
Autor:
C. Spitaleri, S. Romano, L. Lamia, S. M. R. Puglia, M. G. Del Szanto, N. Carlin, M. G. Munhoz, V. Kroha, S. Kubono, E. Somoryai, A. Szanto de Toledo, S. Cherubini, V. Crucillà, M. Gulino, G. Kiss, M. La Cognata, Chengbo Li, R. Liguori Neto, M. M. De Moura, R. G. Pizzone, G. G. Rapisarda, M. L. Sergi, F. A. Souza, A. A. P. Suaide, E. Szanto, G. Tabacaru, S. Tudisco, A. Tumino, Y. Wakabayashi, Qungang Wen, H. Yamaguchi, Sun-Chan Jeong, Yutaka Utsuno, Tohru Motobayashi, Angela Bracco
Publikováno v:
AIP Conference Proceedings.
Light elements lithium, beryllium and boron (LiBeB) were used in the last years as “possible probes” for stellar structure. They are mainly destroyed by (p,α) reactions and cross section measurements for such channels are then needed. In this wo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f085775b80965d288d9a7fbbcaf5f580
https://doi.org/10.1063/1.3141642
https://doi.org/10.1063/1.3141642