Title: Spectroscopy of the heaviest Nuclei
1Spectroscopy of the heaviest Nuclei
2Overview
- Transfermium Nuclei
- Internal Conversion
- In-beam g and CE spectroscopy
- 253No
- The SAGE Spectrometer
3Shell Positions for 298114
From M. Bender et al., PRC 60 (1999) 034304
R-D Herzberg
4Deformed orbitals
Problems No gap at Z100 or 102 No gap at
N152 Trace to position of high-j Orbitals? p
i13/2 n j15/2
M Bender, e.g. in A. Chatillon et al, EPJA30,
06, 397
R-D Herzberg
5Different Skyrme Forces
- Nuclear EOS from 18 different Skyrme
parametrisations - All agree around nuclear density
S. Typel, B.A. Brown, PRC 64 027302.
r0 0.16 fm-3
Neutron density
R-D Herzberg
6Today
RDH PTG, Prog Part Nucl Phys 61 (2008) 674
7Experimental Tools
- Decay spectroscopy
- In-beam spectroscopy
- c.f. Eddie Parr talk today
- Gamma Rays
- Conversion Electrons
R-D Herzberg
8Systematics Z99 Es
F.P. Hessberger et al., EPJA 26 (2005) 233
9Single particle Z99
7/2 ? 3/2- ?
10Neutrons e.g. N149
c.f. TASIspec Poster LL Andersson
11Experimental Tools
- Decay spectroscopy
- In-beam spectroscopy
- c.f. Eddie Parr talk today
- Gamma Rays
- Conversion Electrons
12Internal Conversion
13Spectrum
14Conversion Coefficients
103 102 10 1 0.1 10-2
Z100
M1 K E2 K
e- dominate
alpha
a 1
g dominate
100 200 300
400 500
15Conversion Coefficients
Absolute
Normalised
E 200 keV Z 102 BrICC (T. Kibédi et
al., NIMA 589 (2008) 202)
16Advantages of ICE
- Multipolarity and Parity directly observable from
subshell ratios - Mixing ratios directly accessible
- Low energy transitions observable
17253No 151 neutrons
- Ground state 9/2-
- Excited state 7/2
-
- Rotational band observed at Gammasphere,
assigned 7/2
9/2-734 7/2624
R. Chasman et al, Rev Mod Phys 49 (1977) 833.
18253No Gammasphere
P. Reiter, PRL 95 (05) 032501
19253No Jurogam
11400 Recoils
20Levelscheme
S. Moon, PhD thesis
EPJA submitted
21SACRED Data
T. Page, PhD thesis
1840(40) Recoils
22Moment of Inertia
M. Bender et al., Skyrme-HFB priv. comm.
23Conclusions
- Observed band is built on g.s. 9/2-734
- Branching ratios were key
- Electron Spectroscopy is possible
- No band built on 7/2 observed (yet)
24SAGE
25SAGE and JUROGAM II
26SAGE
Ge opening angles
Beam
27Shielding
BT
- Photomultiplier tubes are sensitive to magnetic
fields - Shields Weaken
- redirect stray magnetic field
28Capability
- 106 Chn Ge _at_ 30-50 kHz
- 90 Chn Si _at_ 30-50 kHz
- Triggerless TDR DAQ
- no common dead time!
- No bottlenecks
29Digital Electronics
50 kHz
40 kHz
30 kHz
20 kHz
10 kHz
Early implementation still needs pileup and
Compton Suppression
30Experiments
- SHE
- 253No, 251Md, 255Lr,
- 254No, 256Rf,
- Shape Coexistence
- 184-190Pb, 180-188Hg, light Po,Bi etc
- E0 from multiphonon states
- Etc
31SAGE
Status April 2nd
Philippos Juha Janne
32Summary
- Combined Electron and Gamma Ray spectroscopy is a
very powerful tool - The SAGE Spectrometer will be commissioned in the
summer - Experiments welcome in the September PAC!
33SAGE Collaboration
- University of Liverpool, UK
- R.-D. Herzberg, J. Pakarinen, P. Papadakis,
- L.L. Andersson, P.A. Butler, R.D. Page,
- J.R. Cresswell, D.A. Seddon, J. Thornhill,
- D. Wells
- University of Jyväskylä, Finland
- P.T. Greenlees, P. Jones, R. Julin,
- P. Rahkila, J. Sorri
- STFC Daresbury Laboratory, UK
- J. Simpson, P.J. Coleman-Smith,
- I.H. Lazarus, S.C. Letts, V.F.E. Pucknell