Zobrazeno 1 - 10
of 39
pro vyhledávání: '"G F Ciani"'
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 7 (2021)
The chemical evolution of the Universe and several phases of stellar life are regulated by minute nuclear reactions. The key point for each of these reactions is the value of cross-sections at the energies at which they take place in stellar environm
Externí odkaz:
https://doaj.org/article/07031d2a0327400394e5a46ec4d5b9ef
Autor:
J Skowronski, R M Gesuè, A Boeltzig, G F Ciani, D Piatti, D Rapagnani, M Aliotta, C Ananna, F Barile, D Bemmerer, A Best, C Broggini, C G Bruno, A Caciolli, M Campostrini, F Cavanna, P Colombetti, A Compagnucci, P Corvisiero, L Csedreki, T Davinson, R Depalo, A Di Leva, Z Elekes, F Ferraro, A Formicola, Zs Fülöp, G Gervino, A Guglielmetti, C Gustavino, Gy Gyürky, G Imbriani, M Junker, M Lugaro, P Marigo, E Masha, R Menegazzo, V Paticchio, R Perrino, P Prati, V Rigato, L Schiavulli, R S Sidhu, O Straniero, T Szücs, S Zavatarelli
Publikováno v:
Journal of Physics G-Nuclear and Particle Physics 50(2023), 045201
Aliotta, M, Bruno, C G & Davinson, T & Sidhu, R S 2023, ' Advances in radiative capture studies at LUNA with a segmented BGO detector ', Journal of Physics G: Nuclear and Particle Physics, vol. 50, no. 4, 045201, pp. 1-20 . https://doi.org/10.1088/1361-6471/acb961
Aliotta, M, Bruno, C G & Davinson, T & Sidhu, R S 2023, ' Advances in radiative capture studies at LUNA with a segmented BGO detector ', Journal of Physics G: Nuclear and Particle Physics, vol. 50, no. 4, 045201, pp. 1-20 . https://doi.org/10.1088/1361-6471/acb961
Studies of charged-particle reactions for low-energy nuclear astrophysics require high sensitivity, which can be achieved by means of detection setups with high efficiency and low backgrounds, to obtain precise measurements in the energy region of in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64ed856596c5b0b307bc1b63a16188d8
https://www.hzdr.de/publications/Publ-36575-1
https://www.hzdr.de/publications/Publ-36575-1
Autor:
A. Badalà, M. La Cognata, R. Nania, M. Osipenko, S. Piantelli, R. Turrisi, L. Barion, S. Capra, D. Carbone, F. Carnesecchi, E. A. R. Casula, C. Chatterjee, G. F. Ciani, R. Depalo, A. Di Nitto, A. Fantini, A. Goasduff, G. L. Guardo, A. C. Kraan, A. Manna, L. Marsicano, N. S. Martorana, L. Morales-Gallegos, E. Naselli, A. Scordo, S. Valdré, G. Volpe
Publikováno v:
La Rivista del Nuovo Cimento. 45:277-279
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 7 (2021)
The chemical evolution of the Universe and several phases of the stellar life are regulated by minute nuclear reactions. The key point for each of these reactions is the value of cross sections at the energies at which they take place in stellar envi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79c54f2e58cca1e9e3d7d1414bf0559e
http://arxiv.org/abs/2208.09283
http://arxiv.org/abs/2208.09283
Autor:
Rosanna Depalo, A. Best, D. Piatti, G. Gervino, G. F. Ciani, T. Chillery, P. Colombetti, F. Ferraro, E. Masha, Luigi Schiavulli, A. Boeltzig, R. Menegazzo, Tamás Szücs, Z. Elekes, Oscar Straniero, Gianluca Imbriani, K. Stöckel, Marialuisa Aliotta, A. Guglielmetti, Filippo Terrasi, R. Perrino, A. Di Leva, J. Balibrea-Correa, László Csedreki, T. Davinson, Sandra Zavatarelli, Paolo Prati, Gy. Gyürky, F. Cavanna, P. Corvisiero, C. Gustavino, E. M. Fiore, Zs. Fülöp, V. Mossa, M. P. Takács, Paola Marigo, Carlo Bruno, Maria Lugaro, Antonio Caciolli, V. Paticchio, A. Formicola, Francesco Barile, F. R. Pantaleo, Diego Vescovi, M. Junker, Carlo Broggini, Sergio Cristallo, D. Rapagnani, Daniel Bemmerer
Publikováno v:
Physical Review Letters. 127
One of the main neutron sources for the astrophysical s process is the reaction ^{13}C(α,n)^{16}O, taking place in thermally pulsing asymptotic giant branch stars at temperatures around 90 MK. To model the nucleosynthesis during this process the rea
Autor:
Rosanna Depalo, A. Best, Antonio Caciolli, K. Stöckel, I. Kochanek, Davide Trezzi, Gianluca Imbriani, R. Perrino, E. Masha, Luigi Schiavulli, F. R. Ferraro, M. P. Takács, V. Paticchio, A. Formicola, F. R. Pantaleo, Francesco Barile, T. Chillery, T. Davinson, Daniel Bemmerer, G. F. Ciani, Tamás Szücs, A. Guglielmetti, László Csedreki, D. Rapagnani, Oscar Straniero, A. Di Leva, Sandra Zavatarelli, Gy. Gyürky, Michael Wiescher, G. Gervino, A. Boeltzig, Zs. Fülöp, V. Mossa, Marialuisa Aliotta, J. Balibrea-Correa, Carlo Bruno, E. M. Fiore, M. Junker, C. Gustavino, G. D'Erasmo, F. Cavanna, Paolo Prati, Carlo Broggini, M. Lugaro, Raffaele Buompane, Richard deBoer, R. Menegazzo, D. Piatti, Z. Elekes, P. Corvisiero
Publikováno v:
Physical Review C. 104
Background: Shell hydrogen burning during the asymptotic giant branch (AGB) phase through the oxygen isotopes has been indicated as a key process that is needed to understand the observed O 18 / O 16 relative abundance in presolar grains and in stell
Autor:
Roberto Menegazzo, Pierre Descouvemont, Z. Elekes, M. P. Takács, Thomas Davinson, C. G. Bruno, P. Corvisiero, Oscar Straniero, Gianluca Imbriani, A. Guglielmetti, Marialuisa Aliotta, Antonio Caciolli, V. Mossa, D. Piatti, A. Boeltzig, Tamás Szücs, Davide Trezzi, A. Di Leva, Paolo Prati, G. F. Ciani, Zs. Fülöp, Maria Lugaro, Paola Marigo, F. Cavanna, K. Stöckel, A. Best, C. Gustavino, D. Bemmerer, Frank Strieder, T. Chillery, C. Broggini, M. Junker, F. R. Pantaleo, R. Depalo, A. Formicola, Gy. Gyürky, G. Gervino, F. Ferraro
Publikováno v:
Physics Letters B, Vol 790, Iss, Pp 237-242 (2019)
Bruno, C, Aliotta, M, Descouvemont, P, Best, A, Davinson, T, Bemmerer, D, Boeltzig, A, Broggini, C, Caciolli, A, Cavanna, F, Chillery, T, Ciani, G F, Corvisiero, P, Depalo, R, Antonino, D L, Elekes, Z, Ferraro, F, Formicola, A, Fülöp, Z, Gervino, G, Guglielmetti, A, Gustavino, C, Gyürky, G, Imbriani, G, Junker, M, Lugaro, M, Marigo, P, Menegazzo, R, Mossa, V, Pantaleo, F R, Piatti, D, Prati, P, Stöckel, K, Straniero, O, Strieder, F, Szucs, T, Takács, M P & Trezzi, D 2019, ' Improved astrophysical rate for the 18O(p,α)15N reaction by underground measurements ', Physics Letters B, vol. 790, pp. 237-242 . https://doi.org/10.1016/j.physletb.2019.01.017
Physics letters. Section B, 790
Bruno, C G, Aliotta, M, Descouvemont, P, Best, A, Davinson, T, Bemmerer, D, Boeltzig, A, Broggini, C, Caciolli, A, Cavanna, F, Chillery, T, Ciani, G F, Corvisiero, P, Depalo, R, Di Leva, A, Elekes, Z, Ferraro, F, Formicola, A, Fülöp, Z, Gervino, G, Guglielmetti, A, Gustavino, C, Gyürky, G, Imbriani, G, Junker, M, Lugaro, M, Marigo, P, Menegazzo, R, Mossa, V, Pantaleo, F R, Piatti, D, Prati, P, Stöckel, K, Straniero, O, Strieder, F, Szücs, T, Takács, M P & Trezzi, D 2019, ' Improved astrophysical rate for the 18O(p,α)15N reaction by underground measurements ' vol. 790, pp. 237-242 . DOI: 10.1016/j.physletb.2019.01.017
Physics Letters B 790(2019), 237-242
Bruno, C, Aliotta, M, Descouvemont, P, Best, A, Davinson, T, Bemmerer, D, Boeltzig, A, Broggini, C, Caciolli, A, Cavanna, F, Chillery, T, Ciani, G F, Corvisiero, P, Depalo, R, Antonino, D L, Elekes, Z, Ferraro, F, Formicola, A, Fülöp, Z, Gervino, G, Guglielmetti, A, Gustavino, C, Gyürky, G, Imbriani, G, Junker, M, Lugaro, M, Marigo, P, Menegazzo, R, Mossa, V, Pantaleo, F R, Piatti, D, Prati, P, Stöckel, K, Straniero, O, Strieder, F, Szucs, T, Takács, M P & Trezzi, D 2019, ' Improved astrophysical rate for the 18O(p,α)15N reaction by underground measurements ', Physics Letters B, vol. 790, pp. 237-242 . https://doi.org/10.1016/j.physletb.2019.01.017
Physics letters. Section B, 790
Bruno, C G, Aliotta, M, Descouvemont, P, Best, A, Davinson, T, Bemmerer, D, Boeltzig, A, Broggini, C, Caciolli, A, Cavanna, F, Chillery, T, Ciani, G F, Corvisiero, P, Depalo, R, Di Leva, A, Elekes, Z, Ferraro, F, Formicola, A, Fülöp, Z, Gervino, G, Guglielmetti, A, Gustavino, C, Gyürky, G, Imbriani, G, Junker, M, Lugaro, M, Marigo, P, Menegazzo, R, Mossa, V, Pantaleo, F R, Piatti, D, Prati, P, Stöckel, K, Straniero, O, Strieder, F, Szücs, T, Takács, M P & Trezzi, D 2019, ' Improved astrophysical rate for the 18O(p,α)15N reaction by underground measurements ' vol. 790, pp. 237-242 . DOI: 10.1016/j.physletb.2019.01.017
Physics Letters B 790(2019), 237-242
The 18O(p,α)15N reaction affects the synthesis of 15N, 18O and 19F isotopes, whose abundances can be used to probe the nucleosynthesis and mixing processes occurring deep inside asymptotic giant branch (AGB) stars. We performed a low-background dire
Autor:
Gianluca Imbriani, A. Boeltzig, A. Gnech, V. Mossa, T. Davinson, Carlo Bruno, R. Menegazzo, Laura Elisa Marcucci, G. F. Ciani, M. P. Takács, Antonio Caciolli, Oscar Straniero, F. Cavanna, Gy. Gyürky, M. Junker, Marialuisa Aliotta, Rosanna Depalo, A. Best, T. Chillery, Z. Elekes, C. Gustavino, E. Masha, A. Di Leva, Luigi Schiavulli, G. Gervino, P. Corvisiero, V. Paticchio, A. Formicola, Zs. Fülöp, K. Stöckel, Paolo Prati, M. Lugaro, D. Piatti, A. Guglielmetti, László Csedreki, F. R. Pantaleo, Carlo Broggini, I. Kochanek, Sandra Zavatarelli, Paola Marigo, Daniel Bemmerer, R. Perrino, F. R. Ferraro, Tamás Szücs, E. M. Fiore
Publikováno v:
Physical Review C. 102
Autor:
Davide Trezzi, L. Di Paolo, I. Kochanek, V. Mossa, F. Ferraro, P. Colombetti, Carlo Bruno, K. Stöckel, Paolo Prati, Sandra Zavatarelli, F. R. Pantaleo, M. Junker, J. Balibrea-Correa, E. M. Fiore, A. Formicola, Gyuri Gyürky, F. Barile, G. Gervino, T. Chillery, G. F. Ciani, R. Depalo, A. Di Leva, Z. Elekes, M. P. Takács, R. Perrino, A. Best, Oscar Straniero, Marialuisa Aliotta, Filippo Terrasi, A. Guglielmetti, László Csedreki, A. Boeltzig, P. Corvisiero, C. Gustavino, F. Cavanna, Antonio Caciolli, Zs. Fülöp, Gianluca Imbriani, Carlo Broggini, M. Lugaro, E. Masha, Luigi Schiavulli, Daniel Bemmerer, Paola Marigo, D. Piatti, Roberto Menegazzo, Tamás Szücs, V. Paticchio, Thomas Davinson
Publikováno v:
The European Physical Journal A. 56
Direct measurements of reaction cross-sections at astrophysical energies often require the use of solid targets able to withstand high ion beam currents for extended periods of time. Thus, monitoring target thickness, isotopic composition, and target
Autor:
Gianluca Imbriani, Gianpiero Mangano, F. Ferraro, K. Stöckel, Thomas Davinson, F. R. Pantaleo, F. Cavanna, R. Menegazzo, E. M. Fiore, E. Masha, Luigi Schiavulli, A. Best, M. Junker, M. P. Takács, Oscar Straniero, I. Kochanek, Daniel Bemmerer, Gyuri Gyürky, A. Guglielmetti, László Csedreki, D. Piatti, Ofelia Pisanti, Marialuisa Aliotta, Tamás Szücs, G. Gervino, Michele Viviani, A. Di Leva, R. Perrino, Laura Elisa Marcucci, Carlo Broggini, Sandra Zavatarelli, Paola Marigo, Davide Trezzi, Maria Lugaro, G. F. Ciani, V. Paticchio, A. Formicola, A. Boeltzig, Alejandro Kievsky, Zs. Fülöp, C. Gustavino, Rosanna Depalo, C. G. Bruno, Z. Elekes, Paolo Prati, Antonio Caciolli, Francesco Barile, V. Mossa, P. Corvisiero, T. Chillery
Publikováno v:
Nature 587(2020), 210-213
Aliotta, M, Bruno, C G & Chillery, T & Davinson, T 2020, ' The baryon density of the Universe from an improved rate of deuterium burning ', Nature, vol. 587, pp. 210-213 . https://doi.org/10.1038/s41586-020-2878-4
Aliotta, M, Bruno, C G & Chillery, T & Davinson, T 2020, ' The baryon density of the Universe from an improved rate of deuterium burning ', Nature, vol. 587, pp. 210-213 . https://doi.org/10.1038/s41586-020-2878-4
Light elements were produced in the first few minutes of the Universe through a sequence of nuclear reactions known as Big Bang nucleosynthesis (BBN)1,2. Among the light elements produced during BBN1,2, deuterium is an excellent indicator of cosmolog
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::acc7c9771ebf8cadc24dc4679504e934
http://hdl.handle.net/11588/827426
http://hdl.handle.net/11588/827426