Astrophysical S-factor of 14N (p, γ) 15O A Formicola, G Imbriani, H Costantini, C Angulo, D Bemmerer, R Bonetti, ... Physics Letters B 591 (1-2), 61-68, 2004 | 431 | 2004 |
S-factor of 14N(p,γ)15O at astrophysical energies⋆ G Imbriani, H Costantini, A Formicola, A Vomiero, C Angulo, D Bemmerer, ... The European Physical Journal A-Hadrons and Nuclei 25, 455-466, 2005 | 303 | 2005 |
Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data T Rauscher, N Dauphas, I Dillmann, C Fröhlich, Z Fülöp, G Gyürky Reports on Progress in Physics 76 (6), 066201, 2013 | 288 | 2013 |
First measurement of the d (p, γ) 3He cross section down to the solar Gamow peak C Casella, H Costantini, A Lemut, B Limata, R Bonetti, C Broggini, ... Nuclear Physics A 706 (1-2), 203-216, 2002 | 240 | 2002 |
Astrophysical factor of the () reaction measured at low energy via detection of prompt and delayed γ rays F Confortola, D Bemmerer, H Costantini, A Formicola, G Gyürky, P Bezzon, ... Physical Review C—Nuclear Physics 75 (6), 065803, 2007 | 222 | 2007 |
The bottleneck of CNO burning and the age of Globular Clusters G Imbriani, H Costantini, A Formicola, D Bemmerer, R Bonetti, C Broggini, ... Astronomy & Astrophysics 420 (2), 625-629, 2004 | 211 | 2004 |
Activation Measurement of the Cross Section at Low Energy D Bemmerer, F Confortola, H Costantini, A Formicola, G Gyürky, R Bonetti, ... Physical review letters 97 (12), 122502, 2006 | 210 | 2006 |
Enhanced electron screening in d (d, p) t for deuterated metals F Raiola, L Gang, C Bonomo, G Gyürky, M Aliotta, HW Becker, R Bonetti, ... The European Physical Journal A-Hadrons and Nuclei 19, 283-287, 2004 | 194 | 2004 |
First measurement of the 14N (p, γ) 15O cross section down to 70 keV A Lemut, D Bemmerer, F Confortola, R Bonetti, C Broggini, P Corvisiero, ... Physics Letters B 634 (5-6), 483-487, 2006 | 180 | 2006 |
Enhanced electron screening in d (d, p) t for deuterated Ta F Raiola, P Migliardi, G Gyürky, M Aliotta, A Formicola, R Bonetti, ... The European Physical Journal A-Hadrons and Nuclei 13, 377-382, 2002 | 176 | 2002 |
The baryon density of the Universe from an improved rate of deuterium burning V Mossa, K Stöckel, F Cavanna, F Ferraro, M Aliotta, F Barile, ... Nature 587 (7833), 210-213, 2020 | 175 | 2020 |
Three New Low-Energy Resonances in the Reaction F Cavanna, R Depalo, M Aliotta, M Anders, D Bemmerer, A Best, ... Physical Review Letters 115 (25), 252501, 2015 | 166* | 2015 |
Electron screening in d (d, p) t for deuterated metals and the periodic table F Raiola, P Migliardi, L Gang, C Bonomo, G Gyürky, R Bonetti, C Broggini, ... Physics Letters B 547 (3-4), 193-199, 2002 | 163 | 2002 |
Stellar and Primordial Nucleosynthesis of : Measurement of A Di Leva, L Gialanella, R Kunz, D Rogalla, D Schürmann, F Strieder, ... Physical review letters 102 (23), 232502, 2009 | 152 | 2009 |
() cross section at low energies G Gyürky, F Confortola, H Costantini, A Formicola, D Bemmerer, R Bonetti, ... Physical Review C—Nuclear Physics 75 (3), 035805, 2007 | 142 | 2007 |
First Direct Measurement of the Cross Section at Big Bang Energies and the Primordial Lithium Problem M Anders, D Trezzi, R Menegazzo, M Aliotta, A Bellini, D Bemmerer, ... Physical Review Letters 113 (4), 042501, 2014 | 140 | 2014 |
Electron screening effect in the reactions 3He (d, p) 4He and d (3He, p) 4He M Aliotta, F Raiola, G Gyürky, A Formicola, R Bonetti, C Broggini, ... Nuclear Physics A 690 (4), 790-800, 2001 | 137 | 2001 |
Precision study of ground state capture in the reaction M Marta, A Formicola, G Gyürky, D Bemmerer, C Broggini, A Caciolli, ... Physical Review C—Nuclear Physics 78 (2), 022802, 2008 | 126 | 2008 |
Absolute cross section of 7Be (p, γ) 8B F Strieder, L Gialanella, G Gyürky, F Schümann, R Bonetti, C Broggini, ... Nuclear Physics A 696 (1-2), 219-230, 2001 | 106 | 2001 |
Electron screening in 7Li (p, α) α and 6Li (p, α) 3He for different environments J Cruz, Z Fülöp, G Gyürky, F Raiola, A Di Leva, B Limata, M Fonseca, ... Physics Letters B 624 (3-4), 181-185, 2005 | 102 | 2005 |