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General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

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Page 1: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB
Page 2: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

General GroupingsProton-Rich

D. Seweryniak (structure around 100Sn)CARIBU

D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands)C. Chiara (RIB + 7Li), R. Janssens (g-factor studies)N. Koller (g-factor studies), R. Casten (binding

energies)V. Werner (fast timing lifetime measurements)

Heavy ElementsW. Loveland (make them), A. Heinz (structure)T.L. Khoo (single-particle energies)

High-SpinL. Riedinger (tetrahedral), S. Tabor (island of

inversion)X. Wang (ultra high-spin)

Page 3: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

Experimental Needs for 100SnMain emphasis on excited states in 100Sn and single-

particle states and nucleon-nucleon interactions using in-beam spectroscopy

More intense beamsPush rates in GAMMASPHERE (x5)

Digital GS Beams 100-200 pnA

Channel selection – tagging with decays (, p, p, ) High granularity DSSD

Secondary fusion-evaporation reactionsIn-flight radioactive beamsBeams 10 pA

Page 4: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

CARIBU: g-factors

252Cf + GammasphereA.G. Smith et al. PLB 591, 55 (2004)

Behavior of neutron-rich g factors

An example:g factors of n-rich isotopes between Z=40 and Z=50.

Why are some g(2+) smaller than in the stable isotopes?

Use RIV on CARIBU beams to extend and improve precision of data.

** Simultaneous measurement of B(E2) and g factor **

Robert channeled A. StuchberyNoemie wants to do clean 138Xe

Page 5: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

CARIBU: Interesting stuff @ N≈90

Two regions of parabolic anomalies.

Two regions of octupole correlations

Possible signature?

Page 6: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

CARIBU: Coulex BeamsSkalski et al. find

stable γ minimumAlso see superdefJ. Hamilton et al. &

C.Y. Wu et al. pushed up around I=20

Safe Coulex to measure Q0

Unsafe Coulex to go beyond I=20

100Zr for tetrahedral shape?J. Skalski et al., NPA 617, 282 (1997)

Page 7: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

TAKE AWAY POINT:TAKE AWAY POINT:

IN ALL CASES, EBIS WILL DRAMATICALLY HELP WITH 10x MORE BEAM!!!!

Page 8: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

Heavy Elements

Page 9: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB
Page 10: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

Wish ListIntensity, intensity, intensity

Long experiments

Complicated setup → campaigns

Dedicated detection system → complete spectroscopy

Phase I will certainly help this group!

Page 11: General Groupings Proton-Rich D. Seweryniak (structure around 100 Sn) CARIBU D. Hartley (triaxial nuclei), D. Kulp (neg. parity bands) C. Chiara (RIB

High-spinTriaxial strongly

deformed bands in N ≈ 94 Er, Hf, Ta, Re, etc.

Identify wobbling bands and find linking transitions to floating bands

Island of inversion and intruder states in A ≈ 30

Tetrahedral shapes in Dy & U