Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Pierpaolo Figuera"'
Autor:
Giovanni L. Guardo, Giuseppe G. Rapisarda, Dimiter L. Balabanski, Giuseppe D’Agata, Alessia Di Pietro, Pierpaolo Figuera, Marco La Cognata, Marco La Commara, Livio Lamia, Dario Lattuada, Catalin Matei, Marco Mazzocco, Alessandro A. Oliva, Sara Palmerini, Teodora Petruse, Rosario G. Pizzone, Stefano Romano, Maria Letizia Sergi, Roberta Spartá, Xuedou Su, Aurora Tumino, Nikola Vukman
Publikováno v:
Universe, Vol 10, Iss 7, p 304 (2024)
Fluorine is one of the most interesting elements in nuclear astrophysics. Its abundance can provide important hints to constrain the stellar models since fluorine production and destruction are strictly connected to the physical conditions inside the
Externí odkaz:
https://doaj.org/article/d0007945529f4f299719a3f42f91049d
Autor:
Pierpaolo Figuera
Publikováno v:
International Journal of Modern Physics E. 20:923-928
The peculiar structure of the halo nuclei is expected to strongly influence the reaction dynamics at energies around the Coulomb barrier . In this paper we will summarize the main experimental results obtained by different authors on the above topic.
Autor:
Pierpaolo Figuera
Publikováno v:
Proceedings of 10th Latin American Symposium on Nuclear Physics and Applications — PoS(X LASNPA).
Autor:
Pierpaolo Figuera
Publikováno v:
AIP Conference Proceedings.
The study of collisions around the Coulomb barrier induced by halo and/or weakly bound nuclei has been the object of many publications in the last years. In this paper we will summarize some recent results on the above topic obtained by our group at
Autor:
Pierpaolo Figuera
Publikováno v:
AIP Conference Proceedings.
The study of collisions around the Coulomb barrier induced by halo and/or weakly bound nuclei has been the object of many publications in the last years, since the peculiar structure of such nuclei can strongly affect the reaction dynamics. In this p
Autor:
L. Achouri, Paul Mumby-Croft, I. Stefan, P. Leleux, Kelly Vaughan, Douglas Robertson, Nicolas de Séréville, Jürgen Kiener, Pierre Descouvemont, E. Casarejos, N. A. Orr, A. Coc, F. Hammache, Vincent Tatischeff, T. Davinson, A. Lefebvre-Schuhl, Alison Laird, S. P. Fox, Pierpaolo Figuera, C. Angulo
Publikováno v:
International Symposium on Nuclear Astrophysics--Nuclei in the Cosmos--IX
International Symposium on Nuclear Astrophysics--Nuclei in the Cosmos--IX, Jun 2006, Genève, Switzerland
HAL
International Symposium on Nuclear Astrophysics--Nuclei in the Cosmos--IX, Jun 2006, Genève, Switzerland
HAL
International audience; The 18F nucleus is one of the radioactive isotopes produced during nova explosions. It is of particular interest since it is mainly responsible for the 511 keV gamma-ray emission of novae that could be detected with the INTEGR