Zobrazeno 241 - 250
of 318
pro vyhledávání: '"R. G. Pizzone"'
Autor:
M. La Cognata, S. Romano, C. Spitaleri, R. Tribble, L. Trache, S. Cherubini, Changbo Fu, L. Lamia, A. Mukhamedzhanov, R. G. Pizzone, C. Rolfs, G. Tabacaru, A. Tumino
Publikováno v:
The 2nd International Conference on Nuclear Physics in Astrophysics ISBN: 9783540328421
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::082148ed393ced03a1cc432f972155b3
https://doi.org/10.1007/3-540-32843-2_39
https://doi.org/10.1007/3-540-32843-2_39
Autor:
A. M. Mukhamedzhanov, M. La Cognata, G. Tabacaru, Livio Lamia, C. Spitaleri, Changbo Fu, C. Rolfs, S. Romano, R. E. Tribble, Aurora Tumino, R. G. Pizzone, Silvio Cherubini, L. Trache
The low-energy, bare-nucleus cross section for 15N(p, α)12C is extracted by means of the Trojan-Horse Method applied to the 2H(15N, α 12C)n reaction at E beam = 60 MeV. The astrophysical S-factor is compared to the direct data in the same energy re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e163e201b0cbd9a88dcf3def1d404a40
http://hdl.handle.net/20.500.11769/11989
http://hdl.handle.net/20.500.11769/11989
Autor:
S. Fulop, Livio Lamia, J. Vincour, R. G. Pizzone, J. Novac, M. L. Sergi, V. Burjan, Salvatore Tudisco, Silvio Cherubini, C. Spitaleri, S. Romano, E. Somorjai, A. Tumino, V. Kroha, M. La Cognata
Publikováno v:
AIP Conference Proceedings.
The astrophysically relevant 7Li+p→α+α reaction was investigated via the THM by selecting the quasi‐free contribution to the measured 3He+7Li→α+α+d three‐body process. This investigation is mainly aimed at testing the validity of the pole
Autor:
C. Spitaleri, S. Romano, Aurora Tumino, R. G. Pizzone, M. La Cognata, C. Li, Silvio Cherubini, Marisa Gulino, Livio Lamia
Publikováno v:
The 2nd International Conference on Nuclear Physics in Astrophysics ISBN: 9783540328421
The Trojan Horse Method has been applied to the 2H(9Be, 6Liα)n three-body reaction in order to investigate the 9Be(p, α)6Li two-body reaction, which is involved in the study of light element abundances (lithium, beryllium and boron). A coincidence
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d3dcd857deb6a2fe107a22575861d84e
https://doi.org/10.1007/3-540-32843-2_34
https://doi.org/10.1007/3-540-32843-2_34
Autor:
L. Lamia, A. Tumino, Silvio Cherubini, C. Rolfs, A. M. Mukhamedzhanov, L. Trache, R. E. Tribble, M. La Cognata, Marisa Gulino, V. Crucillà, Stefan Typel, S. Tudisco, C. Spitaleri, S. Romano, R. G. Pizzone
Publikováno v:
ResearcherID
The Trojan Horse Method allows for the measurements of cross sections in nuclear reactions between charged particles at astrophysical energies. The basic features of the method are discussed and recent applications are presented.
Autor:
A. Tumino, C. Spitaleri, M. L. Sergi, V. Kroha, V. Burjan, S. Cherubini, Zs. Fülöp, M. La Cognata, L. Lamia, J. Novác, R. G. Pizzone, S. Romano, E. Somorjai, S. Tudisco, J. Vincour
Publikováno v:
The 2nd International Conference on Nuclear Physics in Astrophysics ISBN: 9783540328421
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9e8505f2d6fb92d14515635d071887e1
https://doi.org/10.1007/3-540-32843-2_38
https://doi.org/10.1007/3-540-32843-2_38
Publikováno v:
Journal of Physics: Conference Series. 569:012018
The bare nucleus astrophysical S(E) factor is the Nuclear Physics parameter to determine the reaction rates in stellar plasmas. Whilst not being accessed in direct measurements, it can be easily determined using the Trojan Horse Method, successful in
Autor:
D. Schürmann, Stefan Typel, Claudio Spitaleri, S. Romano, L. Lamia, R. G. Pizzone, Silvio Cherubini, Frank Strieder, M. La Cognata, C. Rolfs, A. Musumarra, Aurora Tumino, A. Rinollo
Publikováno v:
Physical Review C. 72
The $^{3}\mathrm{He}$($d,p$)$^{4}\mathrm{He}$ reaction has been studied from ${E}_{c.m.}=600$ keV down to astrophysical energies by means of the ``Trojan horse'' method using the $^{6}\mathrm{Li}$($^{3}\mathrm{He}$,$p\ensuremath{\alpha}$)$^{4}\mathrm
Publikováno v:
Recent Achievements and Perspectives in Nuclear Physics.
Reactions between nuclei in stellar environments take generally place at energies much lower than the Coulomb barrier,EcB , existing between the colliding particles. The relevant center of mass energy range is called “Garnow window” EG , and is t
Autor:
A. Musumarra, E. Casarejos, F. Rizzo, M. Papa, Wendong Tian, P. Figuera, C. Marchetta, J. Lu, F. Amorini, J. L. Sida, G. Cardella, Riccardo Raabe, Carmen Angulo, M. G. Pellegriti, A. Di Pietro, R. G. Pizzone, V. Scuderi, Silvio Cherubini
Publikováno v:
National Conference on Nuclear Physics “Frontiers in the Physics of Nucleus”
National Conference on Nuclear Physics “Frontiers in the Physics of Nucleus”, Jun 2005, St. Petersburg, Russia. pp.1366-1371, ⟨10.1134/S106377880608014X⟩
National Conference on Nuclear Physics “Frontiers in the Physics of Nucleus”, Jun 2005, St. Petersburg, Russia. pp.1366-1371, ⟨10.1134/S106377880608014X⟩
International audience; The present paper concerns the study of reactions induced by radioactive beams of halo and weakly bound nuclei at energies around and above the Coulomb barrier. The results obtained for the reaction induced by the halo nucleus
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10f8f4b7f7c6e4cffed30504364afeac
https://hal.in2p3.fr/in2p3-00097257
https://hal.in2p3.fr/in2p3-00097257