The neutron-rich nucleus Pt200 is investigated via in-beam γ-ray spectroscopy to study the shape evolution in the neutron-rich platinum isotopes towards the N=126 shell closure. The two-neutron transfer reaction Pt198(Se82, Se80)Pt200 is used to populate excited states of Pt200. The Advanced Gamma Ray Tracking Array (AGATA) demonstrator coupled with the PRISMA spectrometer detects γ rays coincident with the Se80 recoils, the binary partner of Pt200. The binary partner method is applied to extract the γ-ray transitions and build the level scheme of Pt200. The level at 1884 keV reported by Yates et al. [S. W. Yates, E. M. Baum, E. A. Henry, L. G. Mann, N. Roy, A. Aprahamian, R. A. Meyer, and R. Estep, Phys. Rev. C 37, 1889 (1988)] was confirmed to be at 1882.1 keV and assigned as the (61+) state. An additional γ ray was found and it presumably deexcites the (81+) state. The results are compared with state-of-the-art beyond mean-field calculations, performed for the even-even 190-204Pt isotopes, revealing that Pt200 marks the transition from the γ-unstable behavior of lighter Pt nuclei towards a more spherical one when approaching the N=126 shell closure.

In-beam γ -ray spectroscopy of the neutron-rich platinum isotope Pt 200 toward the N=126 shell gap / P.R. John, J.J. Valiente-Dobón, D. Mengoni, V. Modamio, S. Lunardi, D. Bazzacco, A. Gadea, C. Wheldon, T.R. Rodríguez, T. Alexander, G. De Angelis, N. Ashwood, M. Barr, G. Benzoni, B. Birkenbach, P.G. Bizzeti, A.M. Bizzeti-Sona, S. Bottoni, M. Bowry, A. Bracco, F. Browne, M. Bunce, F. Camera, L. Corradi, F.C.L. Crespi, B. Melon, E. Farnea, E. Fioretto, A. Gottardo, L. Grente, H. Hess, T. Kokalova, W. Korten, A. Kuşoǧlu, S. Lenzi, S. Leoni, J. Ljungvall, R. Menegazzo, C. Michelagnoli, T. Mijatović, G. Montagnoli, D. Montanari, D.R. Napoli, Z. Podolyák, G. Pollarolo, F. Recchia, P. Reiter, O.J. Roberts, E. Şahin, M.-. Salsac, F. Scarlassara, M. Sferrazza, P.-. Söderström, A.M. Stefanini, S. Szilner, C.A. Ur, A. Vogt, J. Walshe. - In: PHYSICAL REVIEW C. - ISSN 2469-9985. - 95:6(2017 Jun).

In-beam γ -ray spectroscopy of the neutron-rich platinum isotope Pt 200 toward the N=126 shell gap

G. Benzoni;S. Bottoni;A. Bracco;F. Camera;F.C.L. Crespi;S. Leoni;D. Montanari;
2017

Abstract

The neutron-rich nucleus Pt200 is investigated via in-beam γ-ray spectroscopy to study the shape evolution in the neutron-rich platinum isotopes towards the N=126 shell closure. The two-neutron transfer reaction Pt198(Se82, Se80)Pt200 is used to populate excited states of Pt200. The Advanced Gamma Ray Tracking Array (AGATA) demonstrator coupled with the PRISMA spectrometer detects γ rays coincident with the Se80 recoils, the binary partner of Pt200. The binary partner method is applied to extract the γ-ray transitions and build the level scheme of Pt200. The level at 1884 keV reported by Yates et al. [S. W. Yates, E. M. Baum, E. A. Henry, L. G. Mann, N. Roy, A. Aprahamian, R. A. Meyer, and R. Estep, Phys. Rev. C 37, 1889 (1988)] was confirmed to be at 1882.1 keV and assigned as the (61+) state. An additional γ ray was found and it presumably deexcites the (81+) state. The results are compared with state-of-the-art beyond mean-field calculations, performed for the even-even 190-204Pt isotopes, revealing that Pt200 marks the transition from the γ-unstable behavior of lighter Pt nuclei towards a more spherical one when approaching the N=126 shell closure.
English
nuclear and high energy physics
Settore FIS/01 - Fisica Sperimentale
Articolo
Esperti anonimi
Ricerca di base
Pubblicazione scientifica
giu-2017
American Physical Society
95
6
064321
Pubblicato
Periodico con rilevanza internazionale
scopus
crossref
Aderisco
info:eu-repo/semantics/article
In-beam γ -ray spectroscopy of the neutron-rich platinum isotope Pt 200 toward the N=126 shell gap / P.R. John, J.J. Valiente-Dobón, D. Mengoni, V. Modamio, S. Lunardi, D. Bazzacco, A. Gadea, C. Wheldon, T.R. Rodríguez, T. Alexander, G. De Angelis, N. Ashwood, M. Barr, G. Benzoni, B. Birkenbach, P.G. Bizzeti, A.M. Bizzeti-Sona, S. Bottoni, M. Bowry, A. Bracco, F. Browne, M. Bunce, F. Camera, L. Corradi, F.C.L. Crespi, B. Melon, E. Farnea, E. Fioretto, A. Gottardo, L. Grente, H. Hess, T. Kokalova, W. Korten, A. Kuşoǧlu, S. Lenzi, S. Leoni, J. Ljungvall, R. Menegazzo, C. Michelagnoli, T. Mijatović, G. Montagnoli, D. Montanari, D.R. Napoli, Z. Podolyák, G. Pollarolo, F. Recchia, P. Reiter, O.J. Roberts, E. Şahin, M.-. Salsac, F. Scarlassara, M. Sferrazza, P.-. Söderström, A.M. Stefanini, S. Szilner, C.A. Ur, A. Vogt, J. Walshe. - In: PHYSICAL REVIEW C. - ISSN 2469-9985. - 95:6(2017 Jun).
open
Prodotti della ricerca::01 - Articolo su periodico
58
262
Article (author)
si
P.R. John, J.J. Valiente-Dobón, D. Mengoni, V. Modamio, S. Lunardi, D. Bazzacco, A. Gadea, C. Wheldon, T.R. Rodríguez, T. Alexander, G. De Angelis, N. Ashwood, M. Barr, G. Benzoni, B. Birkenbach, P.G. Bizzeti, A.M. Bizzeti-Sona, S. Bottoni, M. Bowry, A. Bracco, F. Browne, M. Bunce, F. Camera, L. Corradi, F.C.L. Crespi, B. Melon, E. Farnea, E. Fioretto, A. Gottardo, L. Grente, H. Hess, T. Kokalova, W. Korten, A. Kuşoǧlu, S. Lenzi, S. Leoni, J. Ljungvall, R. Menegazzo, C. Michelagnoli, T. Mijatović, G. Montagnoli, D. Montanari, D.R. Napoli, Z. Podolyák, G. Pollarolo, F. Recchia, P. Reiter, O.J. Roberts, E. Şahin, M.-. Salsac, F. Scarlassara, M. Sferrazza, P.-. Söderström, A.M. Stefanini, S. Szilner, C.A. Ur, A. Vogt, J. Walshe
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/555345
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