Zobrazeno 1 - 10
of 433
pro vyhledávání: '"L Trache"'
Autor:
L. Ponnath, T. Aumann, C.A. Bertulani, R. Gernhäuser, M. Heil, T. Almusidi, H. Alvarez-Pol, L. Atar, L. Atkins, Y. Ayyad, J. Benlliure, K. Boretzky, M.J.G. Borge, L.T. Bott, G. Bruni, B. Brückner, P. Cabanelas, C. Caesar, E. Casarejos, J. Cederkall, A. Corsi, D. Cortina-Gil, J.A. Dueñas, M. Duer, Z. Elekes, S. Escribano Rodriguez, L. Fabbietti, A. Falduto, M. Feijoo, M. Feijoo Fontan, L.M. Fonseca, A. Frotscher, D. Galaviz, E. Galiana, G. García-Jiménez, I. Gašparic̀, E.I. Geraci, A. Gillibert, B. Gnoffo, D. González Caamaño, A. Graña González, K. Göbel, A.-L. Hartig, A. Heinz, T. Hensel, M. Holl, A. Horvat, A. Jedele, D. Jelavic̀ Malenica, T. Jenegger, H.T. Johansson, B. Jonson, N. Kalantar-Nayestanaki, A. Kelic-Heil, O.A. Kiselev, P. Klenze, D. Kresan, T. Kröll, E. Kudaibergenova, D. Kurtulgil, D. Körper, M. Labiche, C. Langer, I. Lihtar, Yu.A. Litvinov, B. Löher, J. Mayer, S. Murillo Morales, E. Nacher, T. Nilsson, A. Obertelli, V. Panin, J. Park, S. Paschalis, A. Perea, M. Petri, S. Pirrone, T. Pohl, R. Reifarth, H.-B. Rhee, J.L. Rodriguez-Sanchez, L. Rose, D.M. Rossi, P. Russotto, D. Savran, H. Scheit, H. Simon, S. Storck-Dutine, A.M. Stott, C. Sürder, R. Taniuchi, O. Tengblad, P. Teubig, L. Trache, M. Trimarchi, H.T. Törnqvist, L. Varga, V. Wagner, F. Wamers
Publikováno v:
Physics Letters B, Vol 855, Iss , Pp 138780- (2024)
The accuracy of reaction theories used to extract properties of exotic nuclei from scattering experiments is often unknown or not quantified, but of utmost importance when, e.g., constraining the equation of state of asymmetric nuclear matter from ob
Externí odkaz:
https://doaj.org/article/f1cfc1f55ff04971890ba2bd6def5fae
Autor:
Z. Elekes, V. Panin, T.R. Rodríguez, K. Sieja, D.S. Ahn, A. Al-Adili, H. Baba, A.I. Stefanescu, K.J. Cook, Cs. Dósa, N. Fukuda, J. Gao, J. Gibelin, K.I. Hahn, Z. Halász, S.W. Huang, T. Isobe, M.M. Juhász, D. Kim, T. Kobayashi, Y. Kondo, Z. Korkulu, A. Kurihara, I. Kuti, H. Miki, K. Miki, T. Motobayashi, H. Otsu, A. Saastamoinen, M. Sasano, H. Sato, T. Shimada, Y. Shimizu, L.G. Sobotka, I. Stefanescu, L. Stuhl, H. Suzuki, H. Takeda, Y. Togano, T. Tomai, L. Trache, D. Tudor, T. Uesaka, Y. Utsuki, H. Wang, A. Yasuda, K. Yoneda, Y. Yoshitome
Publikováno v:
Physics Letters B, Vol 844, Iss , Pp 138072- (2023)
The nuclear structure of 66Se, nucleus beyond the N=Z line on the proton-rich side of the valley of stability, was investigated by the neutron knock-out reaction 67Se(12C,X)66Se using a 12C target. The analysis of the singles spectrum of the γ-rays
Externí odkaz:
https://doaj.org/article/31412b4d96ae4ec0b4695e3ac72280c6
Autor:
N.T. Zhang, X.Y. Wang, D. Tudor, B. Bucher, I. Burducea, H. Chen, Z.J. Chen, D. Chesneanu, A.I. Chilug, L.R. Gasques, D.G. Ghita, C. Gomoiu, K. Hagino, S. Kubono, Y.J. Li, C.J. Lin, W.P. Lin, R. Margineanu, A. Pantelica, I.C. Stefanescu, M. Straticiuc, X.D. Tang, L. Trache, A.S. Umar, W.Y. Xin, S.W. Xu, Y. Xu
Publikováno v:
Physics Letters B, Vol 803, Iss , Pp - (2020)
Externí odkaz:
https://doaj.org/article/955ab84747bf484b82b663a108d4f21e
Autor:
N.T. Zhang, X.Y. Wang, D. Tudor, B. Bucher, I. Burducea, H. Chen, Z.J. Chen, D. Chesneanu, A.I. Chilug, L.R. Gasques, D.G. Ghita, C. Gomoiu, K. Hagino, S. Kubono, Y.J. Li, C.J. Lin, W.P. Lin, R. Margineanu, A. Pantelica, I.C. Stefanescu, M. Straticiuc, X.D. Tang, L. Trache, A.S. Umar, W.Y. Xin, S.W. Xu, Y. Xu
Publikováno v:
Physics Letters B, Vol 801, Iss , Pp - (2020)
We use an underground counting lab with an extremely low background to perform an activity measurement for the C12+13C system with energies down to Ec.m.=2.323 MeV, at which the 12C(13C,p)24Na cross section is found to be 0.22(7) nb. The C12+13C fusi
Externí odkaz:
https://doaj.org/article/2bbd59efa55644a483573b279d105aa1
Autor:
B. Fernández-Domínguez, B. Pietras, W.N. Catford, N.A. Orr, M. Petri, M. Chartier, S. Paschalis, N. Patterson, J.S. Thomas, M. Caamaño, T. Otsuka, A. Poves, N. Tsunoda, N.L. Achouri, J.-C. Angélique, N.I. Ashwood, A. Banu, B. Bastin, R. Borcea, J. Brown, F. Delaunay, S. Franchoo, M. Freer, L. Gaudefroy, S. Heil, M. Labiche, B. Laurent, R.C. Lemmon, A.O. Macchiavelli, F. Negoita, E.S. Paul, C. Rodríguez-Tajes, P. Roussel-Chomaz, M. Staniou, M.J. Taylor, L. Trache, G.L. Wilson
Publikováno v:
Physics Letters B, Vol 779, Iss , Pp 124-129 (2018)
Intermediate energy single-neutron removal from 31Mg has been employed to investigate the transition into the N=20 island of inversion. Levels up to 5 MeV excitation energy in 30Mg were populated and spin-parity assignments were inferred from the cor
Externí odkaz:
https://doaj.org/article/f2e8857fd2b444aebd72eb2795dab20f
Akademický článek
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Autor:
A. A. Oliva, A. Tumino, N. Soic, P. M. Prajapati, L. Acosta, R. Alba, F. Barba, S. Cherubini, G. D’Agata, D. Dell’Aquila, A. Di Pietro, J.P. Fernandez, P. Figuera, D. Galaviz Redondo, L. Guardo, M. Gulino, F. Hammache, D. Jelavic Malenica, A.I. Kiliç, M. La Cognata, M. La Commara, L. Lamia, D. Lattuada, C. Maiolino, G. Manicò, M. Mazzocco, M. Milin, Ma Nanru, A. Nurmukhanbetova, D. Nurkic, S. Palmerini, T. Parascandolo, D. Pierroutsakou, R.G. Pizzone, R. Popocovski, G.G. Rapisarda, S. Romano, D. Santonocito, M.L. Sergi, A. Shotter, R. Spartà, A. Spiridon, L. Trache, N. Vukman, H. Yamaguchi
12C +12 C is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than 109K when most of the carbon is depleted and its abundance is lower than 16O, the 12C +16 O fusion can also become relevant. Mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d6ccaa6cadc3b0aabcc2a45eff433f6
https://hdl.handle.net/20.500.11769/558663
https://hdl.handle.net/20.500.11769/558663
Autor:
A.A. Oliva, A. Tumino, N. Soic, M.P. Prajapati, L. Acosta, R. Alba, F. Barba, S. Cherubini, G. D’Agata, D. Dell’Aquila, A. Di Pietro, P.J. Fernandez, P. Figuera, D. Galaviz Redondo, L. Guardo, M. Gulino, F. Hammache, D. Jelavic Malenica, A.I. Kiliç, M. La Cognata, M. La Commara, L. Lamia, D. Lattuada, C. Maiolino, G. Manicò, M. Mazzocco, M. Milin, Ma Nanru, A. Nurmukhanbetova, D. Nurkic, S. Palmerini, T. Parascandolo, D. Pierroutsakou, R.G. Pizzone, R. Popocovski, G.G. Rapisarda, S. Romano, D. Santonocito, M.L. Sergi, A. Shotter, R. Spartà, A. Spiridon, L. Trache, N. Vukman, H. Yamaguchi
The carbon-burning process in massive stars mainly occurs via the 12C +12 C. However, at temperatures higher than 109K and considering the increased abundance of 16O produced during the later stages of the heliumburning,the 12C+16O fusion can also be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::30ec1accd2af6e1d0672088ddc277306
https://hdl.handle.net/20.500.11769/558666
https://hdl.handle.net/20.500.11769/558666
Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
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