Zobrazeno 1 - 10
of 378
pro vyhledávání: '"Palmerini, S"'
Autor:
Rodrigues, M. R. D., Bonasera, A., Scisciò, M., Pérez-Hernández, J. A., Ehret, M., Filippi, F., Andreoli, P. L., Huault, M., Larreur, H., Singappuli, D., Molloy, D., Raffestin, D., Alonzo, M., Rapisarda, G. G., Lattuada, D., Guardo, G. L., Verona, C., Consoli, Fe., Petringa, G., McNamee, A., La Cognata, M., Palmerini, S., Carriere, T., Cipriani, M., Di Giorgio, G., Cristofari, G., De Angelis, R., Cirrone, G. A. P., Margarone, D., Giuffrida, L., Batani, D., Nicolai, P., Batani, K., Lera, R., Volpe, L., Giulietti, D., Agarwal, S., Krupka, M., Singh, S., Consoli, Fa.
Laser technologies improved after the understanding of the Chirped Pulse Amplification (CPA) which allows energetic laser beams to be compressed to tens of femtosecond (fs) pulse durations and focused to few $\mu$m. Protons of tens of MeV can be acce
Externí odkaz:
http://arxiv.org/abs/2312.09145
Autor:
Carrasco-Rojas, D. P., Williams, M., Adsley, P., Lamia, L., Bastin, B., Faestermann, T., Fougeres, C., Hammache, F., Harrouz, D. S., Hertenberger, R., La Cognata, M., Meyer, A., Santos, F. de Oliveira, Palmerini, S., Pizzone, R. G., Romano, S., de Sereville, N., Tumino, A., Wirth, H. -F.
Background: Globular clusters show strong correlations between different elements, such as the well-known sodium-oxygen anticorrelation. One of the main sources of uncertainty in this anticorrelation is the $^{22}$Ne($p,\gamma$)$^{23}$Na reaction rat
Externí odkaz:
http://arxiv.org/abs/2302.12939
Autor:
Adsley, P, Williams, M, Harrouz, D S, Carrasco-Rojas, D P, de Séréville, N, Hammache, F, Longland, R, Bastin, B, Davids, B, Faestermann, T, Fougères, C, Greife, U, Hertenberger, R, Hutcheon, D, La Cognata, M, Laird, AM, Lamia, L, Lennarz, A, Meyer, A, Santos, F d'Oliveira, Palmerini, S, Psaltis, A, Pizzone, R G, Romano, S, Ruiz, C, Tumino, A, Wirth, H-F
Globular clusters contain multiple stellar populations, with some previous generation of stars polluting the current stars with heavier elements. Understanding the history of globular clusters is helpful in understanding how galaxies merged and evolv
Externí odkaz:
http://arxiv.org/abs/2212.03648
Autor:
Harrouz, D. S., de Séréville, N., Adsley, P., Hammache, F., Longland, R., Bastin, B., Faestermann, T., Hertenberger, R., La Cognata, M., Lamia, L., Meyer, A., Palmerini, S., Pizzone, R. G., Romano, S., Tumino, A., Wirth, H. -F.
[Background] Abundance anomalies in some globular clusters, such as the enhancement of potassium and the depletion of magnesium, can be explained in terms of an earlier generation of stars polluting the presently observed ones. It was shown that the
Externí odkaz:
http://arxiv.org/abs/2201.03411
Publikováno v:
ApJ 933, 158 (2022)
We analyze the $^{134}_{55}$Cs$\rightarrow^{134}_{56}$Ba and $^{135}_{55}$Cs$\rightarrow^{135}_{56}$Ba $\beta^-$ decays, which are crucial production channels for Ba isotopes in Asymptotic Giant Branch (AGB) stars. We reckon, from relativistic quantu
Externí odkaz:
http://arxiv.org/abs/2109.14230
Publikováno v:
A&A 652, A100 (2021)
Asymptotic giant branch (AGB) stars are considered to be among the most significant contributors to the fluorine budget in our Galaxy. While at close-to-solar metallicity observations and theory agree, at lower metallicities stellar models overestima
Externí odkaz:
http://arxiv.org/abs/2106.08241
Autor:
Broggini, C., Straniero, O., Taiuti, M. G. F., de Angelis, G., Benzoni, G., Bruno, G. E., Bufalino, S., Cardella, G., Colonna, N., Contalbrigo, M., Cosentino, G., Cristallo, S., Curceanu, C., De Filippo, E., Depalo, R., Di Leva, A., Feliciello, A., Gammino, S., Galatà, A., La Cognata, M., Lea, R., Leoni, S., Lombardo, I., Manzari, V., Mascali, D., Massimi, C., Mengoni, A., Mengoni, D., Napoli, D. R., Palmerini, S., Piano, S., Pirrone, S., Pizzone, R. G., Politi, G., Prati, P., Prete, G., Russotto, P., Tagliente, G., Urciuoli, G. M.
Publikováno v:
Rivista del Nuovo Cimento 42, 3 (2019) pp. 103-152
Nuclear astrophysics, the union of nuclear physics and astronomy, went through an impressive expansion during the last twenty years. This could be achieved thanks to milestone improvements in astronomical observations, cross section measurements, pow
Externí odkaz:
http://arxiv.org/abs/1902.05262
Autor:
Vescovi, D., Piersanti, L., Cristallo, S., Busso, M., Vissani, F., Palmerini, S., Simonucci, S., Taioli, S.
Publikováno v:
A&A 623, A126 (2019)
The electron-capture rate on $^7$Be is the main production channel for $^7$Li in several astrophysical environments. Theoretical evaluations have to account for not only the nuclear interaction, but also the processes in the plasma where $^7$Be ions
Externí odkaz:
http://arxiv.org/abs/1902.01826
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.