Zobrazeno 1 - 10
of 36
pro vyhledávání: '"C. G. Bruno"'
Autor:
L. Morales-Gallegos, M. Aliotta, L. Gialanella, A. Best, C. G. Bruno, R. Buompane, T. Davinson, M. De Cesare, A. Di Leva, A. D’Onofrio, J. G. Duarte, L. R. Gasques, G. Imbriani, G. Porzio, D. Rapagnani, M. Romoli, F. Terrasi
Publikováno v:
The European Physical Journal A. 59
Autor:
R. Garg, S. Dellmann, C. Lederer-Woods, C. G. Bruno, K. Eberhardt, C. Geppert, T. Heftrich, I. Kajan, F. Käppeler, B. Phoenix, R. Reifarth, D. Schumann, M. Weigand, C. Wheldon
Publikováno v:
Physical Review C. 107
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:
J. Wu, S. Nishimura, P.-A. Söderström, A. Algora, J. J. Liu, V. H. Phong, Y. Q. Wu, F. R. Xu, J. Agramunt, D. S. Ahn, T. A. Berry, C. G. Bruno, J. J. Bundgaard, R. Caballero-Folch, A. C. Dai, T. Davinson, I. Dillmann, A. Estrade, A. Fijałkowska, N. Fukuda, S. Go, R. K. Grzywacz, T. Isobe, S. Kubono, G. Lorusso, K. Matsui, A. I. Morales, N. Nepal, S. E. A. Orrigo, B. C. Rasco, K. P. Rykaczewski, H. Sakurai, Y. Shimizu, D. W. Stracener, T. Sumikama, H. Suzuki, J. L. Tain, H. Takeda, A. Tarifeño-Saldivia, A. Tolosa-Delgado, M. Wolińska-Cichocka, R. Yokoyama
Publikováno v:
Physical Review C. 106
Autor:
V. H. Phong, S. Nishimura, G. Lorusso, T. Davinson, A. Estrade, O. Hall, T. Kawano, J. Liu, F. Montes, N. Nishimura, R. Grzywacz, K. P. Rykaczewski, J. Agramunt, D. S. Ahn, A. Algora, J. M. Allmond, H. Baba, S. Bae, N. T. Brewer, C. G. Bruno, R. Caballero-Folch, F. Calviño, P. J. Coleman-Smith, G. Cortes, I. Dillmann, C. Domingo-Pardo, A. Fijalkowska, N. Fukuda, S. Go, C. J. Griffin, J. Ha, L. J. Harkness-Brennan, T. Isobe, D. Kahl, L. H. Khiem, G. G. Kiss, A. Korgul, S. Kubono, M. Labiche, I. Lazarus, J. Liang, Z. Liu, K. Matsui, K. Miernik, B. Moon, A. I. Morales, P. Morrall, N. Nepal, R. D. Page, M. Piersa-Siłkowska, V. F. E. Pucknell, B. C. Rasco, B. Rubio, H. Sakurai, Y. Shimizu, D. W. Stracener, T. Sumikama, H. Suzuki, J. L. Tain, H. Takeda, A. Tarifeño-Saldivia, A. Tolosa-Delgado, M. Wolińska-Cichocka, P. J. Woods, R. Yokoyama
Publikováno v:
Physical Review Letters. 129
Autor:
V H, Phong, S, Nishimura, G, Lorusso, T, Davinson, A, Estrade, O, Hall, T, Kawano, J, Liu, F, Montes, N, Nishimura, R, Grzywacz, K P, Rykaczewski, J, Agramunt, D S, Ahn, A, Algora, J M, Allmond, H, Baba, S, Bae, N T, Brewer, C G, Bruno, R, Caballero-Folch, F, Calviño, P J, Coleman-Smith, G, Cortes, I, Dillmann, C, Domingo-Pardo, A, Fijalkowska, N, Fukuda, S, Go, C J, Griffin, J, Ha, L J, Harkness-Brennan, T, Isobe, D, Kahl, L H, Khiem, G G, Kiss, A, Korgul, S, Kubono, M, Labiche, I, Lazarus, J, Liang, Z, Liu, K, Matsui, K, Miernik, B, Moon, A I, Morales, P, Morrall, N, Nepal, R D, Page, M, Piersa-Siłkowska, V F E, Pucknell, B C, Rasco, B, Rubio, H, Sakurai, Y, Shimizu, D W, Stracener, T, Sumikama, H, Suzuki, J L, Tain, H, Takeda, A, Tarifeño-Saldivia, A, Tolosa-Delgado, M, Wolińska-Cichocka, P J, Woods, R, Yokoyama
Publikováno v:
Physical review letters. 129(17)
The β-delayed one- and two-neutron emission probabilities (P_{1n} and P_{2n}) of 20 neutron-rich nuclei with N≥82 have been measured at the RIBF facility of the RIKEN Nishina Center. P_{1n} of ^{130,131}Ag, ^{133,134}Cd, ^{135,136}In, and ^{138,13
Autor:
L. Morales-Gallegos, M. Aliotta, L. Gialanella, A. Best, C. G. Bruno, R. Buompane, T. Davinson, M. De Cesare, A. Di Leva, A. D’Onofrio, J. G. Duarte, L. R. Gasques, G. Imbriani, G. Porzio, D. Rapagnani, M. Romoli, F. Terrasi
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Carbon fusion reactions $$^{12}$$ 12 C($$^{12}$$ 12 C,p)$$^{23}$$ 23 Na and $$^{12}$$ 12 C($$^{12}$$ 12 C,$$\alpha $$ α )$$^{20}$$ 20 Ne play a key role in the evolution of massive stars and in explosive scenarios such as type-Ia supernovae and supe
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, 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
Autor:
G. Cortes, L. J. Harkness-Brennan, X. X. Xu, Robert Grzywacz, K. Matsui, G. G. Kiss, A. Algora, C. Domingo-Pardo, H. Takeda, D. S. Ahn, K. P. Rykaczewski, Mustafa Rajabali, J. Simpson, C. J. Griffin, M. Singh, Y. Saito, K. Miernik, P. J. Woods, Shigeru Kubono, Le Hong Khiem, D. W. Stracener, Jun Liang, M. Karny, N. Nepal, A. Korgul, R. Caballero-Folch, T. Isobe, M. Wolińska-Cichocka, Hiroyoshi Sakurai, P. J. Coleman-Smith, H. Baba, V. H. Phong, A. I. Morales, T. T. King, S.L. Thomas, Toshiyuki Sumikama, Fernando Montes, Joseph Heideman, Ariel Tarifeño-Saldivia, M. Prydderch, I.H. Lazarus, J. Ha, A. Estrade, H. Suzuki, M. Piersa, N. Fukuda, F. Calviño, Jorge Agramunt, R. Yokoyama, B. C. Rasco, Shintaro Go, J. M. Allmond, J. L. Tain, Rebecca Surman, Giuseppe Lorusso, S. Bae, D. Kahl, Berta Rubio, O. Hall, M. Madurga, Toshihiko Kawano, P. Morrall, N. T. Brewer, R. D. Page, M. Labiche, JJ Liu, V. F. E. Pucknell, A. Tolosa-Delgado, Y. Shimizu, Shunji Nishimura, Iris Dillmann, T. Davinson, C. G. Bruno
Publikováno v:
Physical Review C. 100
Aquesta es una copia de la versio author’s final draft d'un article publicat a la revista [Physical Review C ]. URL d'aquest document a UPCommons E-prints: http://hdl.handle.net/2117/174873