Completing the nuclear reaction puzzle of the nucleosynthesis of Mo92

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

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

Radiative Width of the Hoyle State from γ-Ray Spectroscopy.

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.

Thermal properties of 97Mo and 90Y nuclei using temperature dependent level density parameter.

Autor: Benam, Kh.¹ (AUTHOR) kh.benam@sku.ac.ir, Dehghani, V.² (AUTHOR), Alavi, S. A.² (AUTHOR)

Publikováno v: European Physical Journal A -- Hadrons & Nuclei. Oct2023, Vol. 59 Issue 10, p1-8. 8p.

Evidence for the dipole nature of the low-energy γ enhancement in 56Fe.

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.

Constraining the nuclear spin distribution using improved 197Au neutron resonance parameters.

Autor: Koehler, P. E.¹ (AUTHOR) koehler@lanl.gov, Ullmann, J. L.¹ (AUTHOR), Couture, A. J.¹ (AUTHOR), Mosby, S. M.¹ (AUTHOR)

Publikováno v: European Physical Journal A -- Hadrons & Nuclei. Oct2022, Vol. 58 Issue 10, p1-7. 7p.