Search: onr:"swepub:oai:DiVA.org:kth-153388" > Shape evolution in ...
Fältnamn | Indikatorer | Metadata |
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000 | 05050naa a2201285 4500 | |
001 | oai:DiVA.org:kth-153388 | |
003 | SwePub | |
008 | 141003s2014 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:uu-233099 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1533882 URI |
024 | 7 | a https://doi.org/10.1103/PhysRevC.90.0213012 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-2330992 URI |
040 | a (SwePub)kthd (SwePub)uu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a John, P. R.4 aut |
245 | 1 0 | a Shape evolution in the neutron-rich osmium isotopes :b Prompt gamma-ray spectroscopy of Os-196 |
264 | 1 | c 2014 |
338 | a print2 rdacarrier | |
500 | a QC 20141010 | |
520 | a The shape transition in the neutron-rich Os isotopes is studied by investigating the neutron-rich Os-196 nucleus through in-beam gamma-ray spectroscopy using a two-proton transfer reaction from a Pt-198 target to a Se-82 beam. The beam-like recoils were detected and identified with the large-acceptance magnetic spectrometer PRISMA, and the coincident gamma rays were measured with the advanced gamma tracking array (AGATA) demonstrator. The de-excitation of the low-lying levels of the yrast-band of Os-196 were identified for the first time. The results are compared with state-of-the-art beyond-mean-field calculations, performed for the even-even Os188-198 isotopes. The new results suggest a smooth transition in the Os isotopes from a more axial rotational behavior towards predominately vibrational nuclei through triaxial configurations. An almost perfect gamma-unstable/triaxial rotor yrast band is predicted for Os-196 which is in agreement with the experimentally measured excited states. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a atomic-nuclei | |
653 | a transition | |
653 | a coexistence | |
653 | a isomers | |
653 | a os | |
700 | 1 | a Modamio, V.4 aut |
700 | 1 | a Valiente-Dobon, J. J.4 aut |
700 | 1 | a Mengoni, D.4 aut |
700 | 1 | a Lunardi, S.4 aut |
700 | 1 | a Rodriguez, T. R.4 aut |
700 | 1 | a Bazzacco, D.4 aut |
700 | 1 | a Gadea, A.4 aut |
700 | 1 | a Wheldon, C.4 aut |
700 | 1 | a Alexander, T.4 aut |
700 | 1 | a de Angelis, G.4 aut |
700 | 1 | a Ashwood, N.4 aut |
700 | 1 | a Barr, M.4 aut |
700 | 1 | a Benzoni, G.4 aut |
700 | 1 | a Birkenbach, B.4 aut |
700 | 1 | a Bizzeti, P. G.4 aut |
700 | 1 | a Bizzeti-Sona, A. M.4 aut |
700 | 1 | a Bottoni, S.4 aut |
700 | 1 | a Bowry, M.4 aut |
700 | 1 | a Bracco, A.4 aut |
700 | 1 | a Browne, F.4 aut |
700 | 1 | a Bunce, M.4 aut |
700 | 1 | a Camera, F.4 aut |
700 | 1 | a Cederwall, Bou KTH,Kärnfysik4 aut0 (Swepub:kth)u15ywilj |
700 | 1 | a Corradi, L.4 aut |
700 | 1 | a Crespi, F. C. L.4 aut |
700 | 1 | a Desesquelles, P.4 aut |
700 | 1 | a Eberth, J.4 aut |
700 | 1 | a Farnea, E.4 aut |
700 | 1 | a Fioretto, E.4 aut |
700 | 1 | a Goergen, A.4 aut |
700 | 1 | a Gottardo, A.4 aut |
700 | 1 | a Grebosz, J.4 aut |
700 | 1 | a Grente, L.4 aut |
700 | 1 | a Hess, H.4 aut |
700 | 1 | a Jungclaus, A.4 aut |
700 | 1 | a Kokalova, Tz.4 aut |
700 | 1 | a Korichi, A.4 aut |
700 | 1 | a Korten, W.4 aut |
700 | 1 | a Kusoglu, A.4 aut |
700 | 1 | a Lenzi, S.4 aut |
700 | 1 | a Leoni, S.4 aut |
700 | 1 | a Ljungvall, J.4 aut |
700 | 1 | a Maron, G.4 aut |
700 | 1 | a Meczynski, W.4 aut |
700 | 1 | a Melon, B.4 aut |
700 | 1 | a Menegazzo, R.4 aut |
700 | 1 | a Michelagnoli, C.4 aut |
700 | 1 | a Mijatovic, T.4 aut |
700 | 1 | a Million, B.4 aut |
700 | 1 | a Molini, P.4 aut |
700 | 1 | a Montagnoli, G.4 aut |
700 | 1 | a Montanari, D.4 aut |
700 | 1 | a Napoli, D. R.4 aut |
700 | 1 | a Nolan, P.4 aut |
700 | 1 | a Oziol, Ch.4 aut |
700 | 1 | a Podolyak, Zs.4 aut |
700 | 1 | a Pollarolo, G.4 aut |
700 | 1 | a Pullia, A.u Uppsala universitet,Institutionen för fysik och astronomi4 aut |
700 | 1 | a Quintana, B.4 aut |
700 | 1 | a Recchia, F.4 aut |
700 | 1 | a Reiter, P.4 aut |
700 | 1 | a Roberts, O. J.4 aut |
700 | 1 | a Rosso, D.4 aut |
700 | 1 | a Sahin, E.4 aut |
700 | 1 | a Salsac, M. -D4 aut |
700 | 1 | a Scarlassara, F.4 aut |
700 | 1 | a Sferrazza, M.4 aut |
700 | 1 | a Simpson, J.4 aut |
700 | 1 | a Soderstrom, P. -A4 aut |
700 | 1 | a Stefanini, A. M.4 aut |
700 | 1 | a Stezowski, O.4 aut |
700 | 1 | a Szilner, S.4 aut |
700 | 1 | a Theisen, Ch.4 aut |
700 | 1 | a Ur, C. A.4 aut |
700 | 1 | a Walshe, J.4 aut |
710 | 2 | a KTHb Kärnfysik4 org |
773 | 0 | t Physical Review C. Nuclear Physicsg 90:2, s. 021301-q 90:2<021301-x 0556-2813x 1089-490X |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-153388 |
856 | 4 8 | u https://doi.org/10.1103/PhysRevC.90.021301 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-233099 |
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