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Two-phonon octupole collectivity in the doubly-magic nucleus 146 Gd

Explore the octupole collectivity in the doubly-magic nucleus 146Gd and its significance in understanding the nuclear shell model. This study involves the investigation of two-phonon octupole states and their transitions in various stable nuclei like 208Pb, 140Nd, and 142Sm.

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Two-phonon octupole collectivity in the doubly-magic nucleus 146 Gd

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  1. Two-phonon octupole collectivity in the doubly-magic nucleus 146Gd Giacomo de Angelis INFN Laboratori Nazionali di legnaro and CERN Isolde

  2. 2.614 3- 0+ 210At 211At 212At 213At 208Pb 208Pb - central to our understanding of the nuclear shell model 210Po 211Po 212Po 208Bi 209Bi 210Bi 211Bi 209Pb 210Pb 206Pb 207Pb 208Pb 211Pb 206Tl 207Tl 208Tl 206Hg

  3. 3ћ 0,2,3,4,6+ 0,2,4,6+ E2 E3 0,2,4+ 2ћ E2 3– 2+ ћ E3 E2 0 0+ 0+ Octupole Vibration Quadrupole Vibration

  4. Octupole states 208Pb - central to our understanding of the nuclear shell model 5.241 0+ Fragmented 6+ state 2.614 3- 0+ B(E3) ≈ 34 W.u. 208Pb

  5. 1.579 3- The Doubly-magic nucleus 146Gd 0+ 146Gd Z 148Dy 149Dy 150Dy 66 149Tb 146Tb 147Tb 148Tb 65 144Gd 145Gd 146Gd 147Gd 148Gd 64 142Eu 143Eu 144Eu 145Eu 146Eu 147Eu 63 B(E3) ≈ 37(4) W.u. 62 141Sm 142Sm 143Sm 144Sm 145Sm 146Sm 140Pm 141Pm 142Pm 143Pm 144Pm 61 stable nuclei 140Nd 141Nd 142Nd 143Nd 60 N 79 80 81 82 83 84

  6. 0 -5 -10 -15 The Doubly-magic nucleus 146Gd Single-particle Energies (MeV) • 146Gd has the features of a doubly closed shell nucleus. 82 64 126 • 146Gd is the only doubly even nucleus besides 208Pb with a 3- first excited state (lowest in energy). 50 • It is accesible by low momentum transfer fusion-evaporation reactions. 82 • Expectation to observe the 3-3- double octupole. 50   S.W.Yates et al.. Z. Phys. A324 (1986) 417

  7. two-octupole phonon states in 146Gd Z 148Dy 149Dy 150Dy 66 149Tb 146Tb 147Tb 148Tb 65 144Gd 145Gd 146Gd 147Gd 148Gd 64 142Eu 143Eu 144Eu 145Eu 146Eu 147Eu 63 62 141Sm 142Sm 143Sm 144Sm 145Sm 146Sm 140Pm 141Pm 142Pm 143Pm 144Pm 61 stable nuclei 140Nd 141Nd 142Nd 143Nd 60 N 79 80 81 82 83 84

  8. 381.7 keV 502.6 KeV E1 1905.8 KeV E3 The Doubly-magic nucleus 146Gd 6+ 3484 KeV 826.7 KeV Caballero L. et al., (2010). Phys. Rev. C 81, 031301 7 - 324 KeV E1 E2 5 - 1078 KeV E2 3 - 381.7 keV gate 1579 KeV E3 0+ 146Gd

  9. Generator Coordinate Method with an axial octupole moment as generating coordinate For 146Gd EX3- ≈ 3 MeV Ex6+≈6 MeV B(E3:3- 0+)≈24 W.u. B(E3:6+3-)≈54 W.u.

  10. Coulomb Excitation of 146Gd

  11. GOSIA rate estimate Projectile and recoiling nuclei between 16 and 53 degree in the lab 146Gd E=800 MeV on 1 mg/cm2 Pb target Transition matrix elements for 3-0+, 7-5- 6+5-, 6+7- from [P. Daly et al.Z. Phys. A 298 173 (1984)] 6+3- [L. Caballero et al. PRC81,031301R (2010) ] 5-3- SM estimate I(146Gd) = 106 pps

  12. Beam Composition (146Gd) using MR-TOF Ta foil target # 565 Ion source temperature 21500 A=146 Beam purity about 3%

  13. Beam Composition (146Gd) using MR-TOF Ta foil target # 565 Ion source temperature 21500 A=162 Beam purity about 45% I146Gd=108 pps 162Dy High beam purity expected breaking the molecule in Rex-EBIS

  14. Beamtime request Requested shifts •  we expect 4 counts per day for the 1905.8 keV 6+ -> 3- and 100 counts per day for the 826.7 keV 6+ -> 5- transitions with a full statistics of 24 and 600 counts collected in 6 days of beam time (18 shifts). 6+ populated only via E3 and extracted through the 826.7 E1 strength. •  The expected statistics should be sufficient to search for other members of the double-phonon multiplet. •  Independent normalization of the B(E3, 3- -> 0+) achieved through comparison with the target excitation (94Mo) which has a well known B(E2) strength and no overlapping gamma transitions. We expetct 500 counts in two days (6 shifts) • 146Gd beam 24 shifts (18 shifts on 208Pb target and 6 shifts on 94Mo) Thanks for attention

  15. Collaboration G. de Angelis, K. Hadynska-Klek, M. Zielinska, B. Rubio, M. J. G. Borge, L. Razvan, K. Johnston, S. Lunardi, J.N. Orce, A. Algora, L. Caballero, A. Gadea, J.L. Tain, S.A.E. Orrigo, A. Morales, S. W. Yates, F. Gramegna, A. Goasduff, G. Jaworski, D.R. Napoli, G. Prete, M. Siciliano, J. Valiente Dobon, D. Bazzacco, F. Recchia, A. Boso, P.R. John, S.M. Lenzi, R. Menegazzo, D. Mengoni, D. Testov, B. Melon, A. Nannini, C. Fahlander, R. Orlandi, P. Reiter, D. Rosiak, M. Seidlitz, N. Warr, T. Kroell, T.D. Goodacre, B. Marsh, O. Sorlin, W. Gelletly, M. Rocchini, E. Sahin, E. Ganioglu, R. Julin, R. Broda, S. Leoni, G. Bocchi, G. Benzoni, D. Santonocito, U. Koester Thanks for attention

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