The race for 100 Sn – History and status of experimental and shell model approach Topics: • History: the past 50 years • Experimental approach • Spin gap isomerism and seniority in the g 9/2 hole space • Excitation of the 100 Sn core and large scale shell model • Super Gamow-Teller decay of 100 Sn • Z=N=50 shell gaps • The doubly-magic neighbours 56 Ni, 78 Ni and H. Grawe, M. Górska, T. Faestermann SMUV Strasbourg 8. – 10. 10. 2012 (cf. FGG, Progr. in Part. Nucl. Phys., in print)
31
Embed
The race for 100 Sn – History and status of experimental and shell model approach Topics: History: the past 50 years Experimental approach Spin gap isomerism.
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
The race for 100Sn – History and status of experimental and shell model approach
Topics:
• History: the past 50 years
• Experimental approach
• Spin gap isomerism and seniority in the g9/2 hole space
• Excitation of the 100Sn core and large scale shell model
• Super Gamow-Teller decay of 100Sn
• Z=N=50 shell gaps
• The doubly-magic neighbours 56Ni, 78Ni and 132Sn
• The future has started !
H. Grawe, M. Górska, T. Faestermann SMUV Strasbourg 8. – 10. 10. 2012
(cf. FGG, Progr. in Part. Nucl. Phys., in print)
2d5/2,1g7/2,3s1/2,1h11/2,2d3/2
2d5/2,3s1/2,2d3/2,1g7/2,1h11/2
1f5/2,2p3/2,2p1/2,1g9/2
On the road to 100Sn
88Sr,89Y, 90Zr, 92Mo
"classical" and "new‘‘
doubly-magic and
"almost" magic nuclei
The Start !
The race for 100Sn – landmarks part I – the start 1958 90Zr up to (0-8)+ N.H. Lazar et al., PR 110, 513(58)
A. De Shalit, I. Talmi, Nuclear Shell Theory, Academic Press, New York, 1963R.F.Casten, Nuclear Structure from a Simple Perspective, Oxford University Press, 2000H. G., The Euroschool Lectures on Physics with Exotic Beams, Vol. I, Lect. Notes Phys.
651, 33 (2004)A. Amusa, R.D. Lawson, ZPA 307, 333 (1982)H. Grawe et al., EPJA 27, s01, 257 (2006)H. Mach et al., Proc. Int. Symposium A New Era of Nuclear Structure Physics, Niigata, Japan 2003, World Scientific, Singapore, 2004, p.277F. Nowacki, priv. comm. A. Escuderos, L. Zamick, PRC73, 044302 (2006) P. Van Isacker, Int. J. Mod. Phys. E20, 191 (2011)
}95Rh
96Pd94Ru
Z=28
N=50
Valence mirror g9/2n nuclei in Z=28 isotopes
and
N=50 isotones The 8+ isomers disappear in mid-shell Ni isotopes due to stronger I= 2+ two-body matrix element (Ex(2+)
~1.0 vs. 1.5 MeV), which shifts the seniority v=4, 6+ state (*) below the v=2, 8+ enabling a strong v=2 B(E2)H.G. et al., NPA 704, 211c (2002)
A. Lisetskiy et al., PRC 70, 044314 (2004)
8+ isomers !
No 8+ isomers !
A. Blazhev et al., PRC 69, 064304
preliminary !
100Sn core excitation
•LSSM smoothly converged at t=5 (F. Nowacki, E. Caurier)
• 100Sn neutron shell gap N=50 inferred 6.46 (15) MeV• remaining E2,E4 deficiency is due to interaction and/or proton gap Z=50• effective E2 charge will not help !
Valence statesg9/2
-2
ph statesg9/2
-2g9/2-t (d5/2,g7/2)t
pairing
• Valence excitation energy increases with t• ph excitation energy decreases with t• Exception t=2 : pairing overbinds valence states
E2
E2
E4
98Cd
A. Blazhev et al., PRC 69, 064304 (04)
96Pd
First core excited odd-parity isomer in N=50 96Pd
• = + states well reproduced in LSSM @t=5 in gds space
• = - states calculated @ t=1 for neutrons in fpgd5/2
M. Palacz et al., PRC 86, 014318 (2012)
valence
corex
96Ag
Valence and core excited isomers in N=49
96Ag
P. Boutachkov et al., PRC 84, 044311 (2011) see A. Blazhev !
valence isomers
core excited isomer
SMf5/2,p,g9/2
LSSM gds
100Sn excited states predictions from shell model and mean field
100Sn Super Gamow-Teller decay (II)Ch. Hinke et al., Nature 486, 341 (2012)
QEC = 4.35(-17 +19) MeVT1/2 = 1.09 (18) s
LSSM 100In EXP
g9/2-1 g7/2) 1+ log(ft) = 2.62(+0.13
-0.11) record low !
B(GT) = 9.3 (+2.3-3.0)
record high ! Single 1+ feeding
+
Ch. Hinke et al., Nature 486, 341 (2012)
100Sn
LSSM in gdsK. Sieja, F. Nowacki
LSSM guided correction:3 more 1+ states fed with B(GT)>0.1
B(GT) = 9.9 (+2.8-3.2)
B(GT;1+1) = 7.6 (+2.2 -2.5)
LSSM value 5.7 robust shell gaps >6 MeV q~0.75 quenching of GT operator confirmed
Why “Super“ ?
B(GT) =160/9 × 1 × 1for g9/2 → g7/2 spin-flip transition Unique in the Segrè chart !
100Sn Super Gamow-Teller decay (III)
Monopole driven shell structureSingle particle/hole energies (SPE/SHE) and shell gaps from extrapolation of experimental data from known CS´to next CS
e.g. N=50
99,100,101Sn99In
90,91,92Nb89,90,91Zr
92Mo
Two-body matrix elements (TBME) and monopoles from binding energies (BE),SPE/SHE () and excitation energies (Ex)within each multiplet j´j for particle-particle andj´k for particle-hole
See FGG !
Exp. gaps from separation energies S1n,S2n
ESPE from exp. multipletscorrected for occupation
theoretical monopoleT. Otsuka et al., PRL104,012501 (10)
SM in valence space, no corex
100Sn : 6.35(13) MeV for d5/2 g.s.3.9(5)/3.0(3) MeV for d5/2/g7/2 g.s.O. Sorlin, M.-G. Porquet, PPNP 61, 602 (08)
robust shell gaps !
78Ni : 4.05(18) MeV for d5/2 g.s.3.4 MeV for d5/2 g.s.M.-G. Porquet, O. Sorlin,PRC 85, 014307(12)
4.7 from LSSM and d5/2 g.s.K. Sieja, F. Nowacki, PRC 85,051301(R) (12)
Shell gap along N=50
100Sn and 56Ni SPE/SHE and g7/2 monopole migration
d5/2, g7/2 problem in 101SnAnalogy of N=3, 4 HO shells andintruders from N=4, 5100Sn gaps: 5.96(20) () and 6.35(13) () MeV
D. Seweryniak et al., PRL 99, 022504(07) (ANL)I.G. Darby et al.,PRL105, 162502(10) (ORNL)
Extrapolation “safe“ for g9/2d5/2 multiplet (92Nb)g9/2g7/2 monopole from G-matrix (MHJ)modified to fit N=51 single particle states (MHJm)
100Sn extrapolated SPE vs. SM and global predictions (just a selection from many)
“EX“: extrapolated H.G.SKX : Skyrme B.A. Brown PRC 58,220(98)
PL40: RMF K. Rutz et al., NPA 634,67 (98)DZ: SM based global monopole scalingJ. Duflo, A.P Zuker, PRC 59, R2347(99)
100Sn and its magic neighbours 56,78Ni and 132Sn
f5/2(p) − g9/2: gap increase from 56Ni to 78Ni /100Sn and decrease from 100Sn to 132Sn due to strong monopole; Z=40 subshell at N=82?f5/2(p)g9/2 – g7/2(ds)h11/2: N=4 intruder g9/2 well separated N=40 subshell in Ni´s N=5 intruder h11/2 embedded in s1/2,d3/2 orbits no subshells in Sn´s
56Ni vs. 100Sn – fp vs. gds structure analogies - Why and why not?
(a)valence states Imax = 6+ vs. 8+
B(E2) = 3.3 vs. 1.2 W.u.
core excited isomers I= 10+ vs. 12+ = Imax + 4 B(E2) = 1.7 vs. 2.2 W.u.B(E4) = 0.8 vs. 3.0 W.u.
correspondence principle ! (Jan Blomqvist)(b)valence statesImax = 11+ vs. 15+ Imax-2 = 9+ (!) vs. 13+
Isomer destroyed !9+2 needs p3/2 !No core excited isomers due to proximity to proton mid-shell
LSSM80Zr
Z=50 shell gap for 100-132Sn and B(E2;0+→2+)
SM 100Sn core onlyLSSM 80/90Zr core A. Banu et al., PRC 72,
061305 (2005)
RQRPAA. Ansari et al., PLB 623, 37
(2005)EXP: ENSDF
AMDC sys
Extrapolated• B(E2) enhanced below A~114• correlation with reduced Z=50 shell gap and g9/2
E(2+) and B(E2;2+ 0+) in semi-magicvalence mirrors fpg and gdsh nuclei Experiment and shell model (SM/LSSM)
Moderate N=40 and Z=(38),40 gaps No N=64,66 nor 70 gapsbetween p1/2 and g9/2 orbits due to closely packed g7/2dsh11/2 orbits SM: A. Lisetskiy et al., PRC 70, 044314 (04) SM and
LSSM: O. Kenn et al., PRC 63,064306(01) LSSM: A. Banu et al., PRC 72 ,061305(05) O. Sorlin et al., PRL 88,092501(02) S. Lenzi et al., PRC 82,054301(10)
Z=28 N=50 Z=50
p,f5/2 g9/2p,f5/2 g9/2 s,d,g7/2 h11/2
No gap !
Apparent scaling of effective g9/22 two-body matrix
elements
S S S
• S = E(8+)-E(2+) ~ A-1 ?
• valence space pf5/2g9/2 ~ A-1/3
• Coulomb and pairing negligible
• Cross shell excitation different N=3, N=4, N=5 HO shells !
• Quadrupole interaction scales as EQ = O(D-1 A-1/3) , Degeneracy D M. Dufour and A. P.
Zuker, PRC54, 1641 (1996)
• Normalise to 98Cd LSSM in gds Frederic Nowacki, priv. comm.
Normalised to 2+ to minimise effect of
p1/2, Coulomb and pairing
9848Cd50
LSSM EXP
t=0 1 2 3 4 5
EX D A-1 A-1/3
76Ni 1428 1353 1336 1128
98Cd 1036 1036 1036 1036 (reference)
130Cd 803 785 781 943
Summary of status and outlook
• g9/2 isomerism, interaction, seniority scheme and distortions • core excitation across Z,N=50 and E2/E4 isomerism and strength• super Gamow-Teller decay and implication for shell structure• verification of general GT quenching factor ~0.75 for N=4 HO shell• robustness of Z=N=50 shells 3 MeV from the proton dripline • monopole driven evolution of single particle energies • shell structure evolution towards HO shell neighbours• A-1 scaling of empirical TBME• masses and half lives along the rp path• super-allowed decay close to N=Z
• experimental verification 100Sn gaps and single particle/hole energies• excited states and mirror symmetry in, below and beyond 100Sn• precision masses and GT strength along the rp path• precision studies of super-allowed Fermi decay and CVC hypothesis• proton emission below Z=50• super-allowed -decay at N=Z• realistic interaction beyond 0 ħ• consistent LSSM description of excitation and masses
Done:
To do:
Collaborations
EUROBALL I-IV, the home of European Gamma Arrays
RISING Rare ISotope INvestigation at GSI
EURICA EUroball Riken Cluster Array
PreSPEC Pre- (HI-DE-SPEC) campaign @GSI plus
AGATA Advanced Gamma Tracking Array
SM2 Strasbourg-Madrid Shell Model
Special thanks go to: A. Blazhev, P. Boutachkov, B.A. Brown, E. Caurier, T. Faestermann, M. Górska, Ch. Hinke, M. Hjorth-Jensen, G. Martinez-Pinedo, B.S. Nara Singh, F. Nowacki, T.