Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Nyhus HT"'
Autor:
Kheswa, BV, Wiedeking, M, Brown, JA, Larsen, AC, Goriely, S, Guttormsen, M, Garrote, FL Bello, Bernstein, LA, Bleuel, DL, Eriksen, TK, Giacoppo, F, Görgen, A, Goldblum, BL, Hagen, TW, Koehler, PE, Klintefjord, M, Malatji, KL, Midtbø, JE, Nyhus, HT, Papka, P, Renstrøm, T, Rose, SJ, Sahin, E, Siem, S, Tornyi, TG
Publikováno v:
Kheswa, BV; Wiedeking, M; Brown, JA; Larsen, AC; Goriely, S; Guttormsen, M; et al.(2017). La 137,138,139 (n,γ) cross sections constrained with statistical decay properties of la 138,139,140 nuclei. Physical Review C, 95(4). doi: 10.1103/PhysRevC.95.045805. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/3fb9h275
Physical Review C, vol 95, iss 4
Physical Review C, vol 95, iss 4
© 2017 American Physical Society. The nuclear level densities and γ-ray strength functions of La138,139,140 were measured using the La139(He3,α), La139(He3,He3′), and La139(d,p) reactions. The particle-γ coincidences were recorded with the sili
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::583bd86721a21f1154971b9b10483e79
http://www.escholarship.org/uc/item/3fb9h275
http://www.escholarship.org/uc/item/3fb9h275
Autor:
Tveten, GM, Spyrou, A, Schwengner, R, Naqvi, F, Larsen, AC, Eriksen, TK, Garrote, FLB, Bernstein, LA, Bleuel, DL, Campo, LC, Guttormsen, M, Giacoppo, F, Gorgen, A, Hagen, TW, Hadynska-Klek, K, Klintefjord, M, Meyer, BS, Nyhus, HT, Renstrom, T, Rose, SJ, Sahin, E, Siem, S, Tornyi, TG
Publikováno v:
Physical Review C, vol 94, iss 2
Tveten, GM; Spyrou, A; Schwengner, R; Naqvi, F; Larsen, AC; Eriksen, TK; et al.(2016). Completing the nuclear reaction puzzle of the nucleosynthesis of Mo-92. PHYSICAL REVIEW C, 94(2). doi: 10.1103/PhysRevC.94.025804. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/1wg7b53t
Tveten, GM; Spyrou, A; Schwengner, R; Naqvi, F; Larsen, AC; Eriksen, TK; et al.(2016). Completing the nuclear reaction puzzle of the nucleosynthesis of Mo-92. PHYSICAL REVIEW C, 94(2). doi: 10.1103/PhysRevC.94.025804. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/1wg7b53t
One of the greatest questions for modern physics to address is how elements heavier than iron are created in extreme astrophysical environments. A particularly challenging part of that question is the creation of the so-called p-nuclei, which are bel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::cbedfb6e821ec6d98d4953b59b327283
https://escholarship.org/uc/item/1wg7b53t
https://escholarship.org/uc/item/1wg7b53t
Autor:
Renstrøm, T, Nyhus, HT, Utsunomiya, H, Schwengner, R, Goriely, S, Larsen, AC, Filipescu, DM, Gheorghe, I, Bernstein, LA, Bleuel, DL, Glodariu, T, Görgen, A, Guttormsen, M, Hagen, TW, Kheswa, BV, Lui, YW, Negi, D, Ruud, IE, Shima, T, Siem, S, Takahisa, K, Tesileanu, O, Tornyi, TG, Tveten, GM, Wiedeking, M
Publikováno v:
Physical Review C, vol 93, iss 6
The γ-ray strength functions and level densities of Ge73,74 have been extracted up to the neutron-separation energy Sn from particle-γ coincidence data using the Oslo method. Moreover, the γ-ray strength function of Ge74 above Sn has been determin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::835161f5a4c3d979144a039855f367fa
https://escholarship.org/uc/item/9bj1r8fv
https://escholarship.org/uc/item/9bj1r8fv
Autor:
Görgen, A, Siem, S, Korten, W, Obertelli, A, Sulignano, B, Theisen, Ch, Bürger, A, Guttormsen, M, Hagen, TW, Larsen, AC, Nyhus, HT, Renstrøm, T, Syed, NUH, Toft, HK, Tveten, GM, Wikan, K, Delaroche, JP, Girod, M, Cederkäll, J, Van de Walle, J, Clément, E, De France, G, Ljungvall, J, Butler, PA, Scheck, M, Jenkins, DG, Freeman, S, Reiter, P, Seidlitz, M, Wendt, A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________65::5893bd21697511dfb35533562ad2b594
http://cds.cern.ch/record/1156116
http://cds.cern.ch/record/1156116
Autor:
Kibédi T; Department of Nuclear Physics, Research School of Physics, The Australian National University, Canberra, Australian Capital Territory 2601, Australia., Alshahrani B; Department of Nuclear Physics, Research School of Physics, The Australian National University, Canberra, Australian Capital Territory 2601, Australia.; Department of Physics, Faculty of Science, King Khalid University, Abha 61413, Saudi Arabia., Stuchbery AE; Department of Nuclear Physics, Research School of Physics, The Australian National University, Canberra, Australian Capital Territory 2601, Australia., Larsen AC; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Görgen A; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Siem S; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Guttormsen M; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Giacoppo F; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Morales AI; Dipartimento di Fisica dell'Universitá degli Studi di Milano and INFN-Milano, 20133 Milano, Italy., Sahin E; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Tveten GM; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Garrote FLB; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Campo LC; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Eriksen TK; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Klintefjord M; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Maharramova S; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Nyhus HT; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Tornyi TG; Department of Physics, University of Oslo, N-0316 Oslo, Norway.; Institute of Nuclear Research, MTA ATOMKI, Debrecen H-4026, Hungary., Renstrøm T; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Paulsen W; Department of Physics, University of Oslo, N-0316 Oslo, Norway.
Publikováno v:
Physical review letters [Phys Rev Lett] 2020 Oct 30; Vol. 125 (18), pp. 182701.
Autor:
Larsen AC; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Blasi N; INFN, Sezione di Milano, I-20133 Milano, Italy., Bracco A; INFN, Sezione di Milano, I-20133 Milano, Italy and Dipartimento di Fisica, University of Milano, I-20122 Milano, Italy., Camera F; INFN, Sezione di Milano, I-20133 Milano, Italy and Dipartimento di Fisica, University of Milano, I-20122 Milano, Italy., Eriksen TK; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Görgen A; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Guttormsen M; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Hagen TW; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Leoni S; INFN, Sezione di Milano, I-20133 Milano, Italy and Dipartimento di Fisica, University of Milano, I-20122 Milano, Italy., Million B; INFN, Sezione di Milano, I-20133 Milano, Italy., Nyhus HT; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Renstrøm T; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Rose SJ; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Ruud IE; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Siem S; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Tornyi T; Department of Physics, University of Oslo, N-0316 Oslo, Norway and Institute of Nuclear Research, MTA ATOMKI, H-4026 Debrecen, Hungary., Tveten GM; Department of Physics, University of Oslo, N-0316 Oslo, Norway., Voinov AV; Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA., Wiedeking M; iThemba LABS, Post Office Box 722, 7129 Somerset West, South Africa.
Publikováno v:
Physical review letters [Phys Rev Lett] 2013 Dec 13; Vol. 111 (24), pp. 242504. Date of Electronic Publication: 2013 Dec 11.