Title: Isomer Spectroscopy of the Heaviest Elements
1Isomer Spectroscopy of the Heaviest Elements
Rod Clark (Lawrence Berkeley National Laboratory)
2Outline
- Motivation for studying structure of heaviest
nuclei - K-isomers in Z100 region
- The Berkeley Gas-Filled Separator (BGS)
- Recent results
- 50Ti208Pb?256Rf2n (s20nb)
- 48Ca209Bi?255Lr2n (s300nb)
- Heavy element spectroscopy with GRETINABGS
- Summary
3Motivation
- Single-particle levels ? shell structure
- Next major spherical gaps
- Deformed gaps
-
- Deformation and collectivity
- K-isomerism
- Rotational structures
- Low-lying vibrations
- Pairing properties
- Multi-quasiparticle states
- Effects on rotation
- Effects on alpha decay
- Effects fission decay
4K-Isomers in Z100 Nuclei
RITU at JYFL
FMA at ANL
5Conversion Electron and Gamma Spectroscopy
S.K.Tandel et al., PRL 97 082502 (2006)
6Berkeley Gas-filled Separator
- ? Large acceptance 45 msr ( 9 vertical, 4.5
horizontal) - ? Highest transmission ( NiPb
70 CaPb 60 MgU 18 ) - ? Large bend angle 70
- ? Lowest background rates ( 40Hz/pmA 20Hz/pmA 10
0Hz/pmA )
7Focal Plane Detectors
1616 strip DSSD 1mm thick, 5cm by 5cm
1) Recoil implanted in pixel of DSSD 2) Burst of
conversion electrons in same pixel from isomer
decay 3) Gamma-rays in coincidence with electron
burst 4) Recoil decays in same pixel by
alpha/fission
Key idea was to tag on isomer by searching for
burst of conversion electrons and using a single
pixel as a calorimeter.
G.D. Jones (Liverpool), NIM A 488 471 (2002).
8256Rf Z104, N152
50Ti208Pb?256Rf2n at 243 MeV (s20nb), 200pnA,
6 days
Electrons
Gamma Rays
r-e-e-f
r-e-e-f
9H. B. Jeppesen et al., Submitted to PRL
10255Lr Z103, N152
48Ca209Bi?255Lr2n at 222 MeV (s300nb), 300pnA,
4 days
11247Es Z99, N148
g-spectroscopy following a-decay of
255Lr?251Md?247Es
12Eisteinium (Z99) Systematics Re-examined
251Md
251Md
a1
a2
a
g294
g243
g243
g294
0x
247Es
247Es
F.P.Hessberger et al., EPJ A 26 233 (2005) A.
Chatillon et al., EPJ A 30 397 (2006)
13Eisteinium (Z99) Systematics Re-examined
251Md
251Md
?
a1
a2
a
g294
g243
g243
g294
0x
247Es
247Es
F.P.Hessberger et al., EPJ A 26 233 (2005) A.
Chatillon et al., EPJ A 30 397 (2006)
14Transfermium Spectroscopy with GRETINABGS
The best heavy element separator with the best
g-ray detector system
Assumptions for simulation sTOT 1 barn Target
0.5 mg/cm2 Beam Current 50 pnA eg / crystal
0.0067 Mg 10 ? 30.3 kHz/crystal
Energy (keV)
15Summary
- New generation of spectroscopy experiments on
heaviest elements - RITU at JYFL, FMA at ANL, BGS at LBNL,
- GABRIELLA at Dubna, SHIP at GSI, VAMOS at
GANIL - Decay spectroscopy at BGS able to reach Sg
(Z106) - - single-particle states
- - K-isomerism
- - low-lying rotational and vibrational modes
- Prompt spectroscopy with GRETINA at BGS able to
reach Rf (Z104) - - rotation versus fission
- - moments of inertia, alignments
- - configuration assignments
- Can modern microscopic theories reproduce
experiment?
16Thanks!