prospects for laser spectroscopy of superheavy...
TRANSCRIPT
Prospects for Laser Spectroscopy of Superheavy Elements
Hartmut Backe1, Michael Block, Mustapha Laatiaoui, Werner Lauth
1University of Mainz, Germany
International Symposium Super Heavy Nuclei 2015, Texas A&M University, College Station, Texas, USA, March 31 - April 02, 2015
Outline
1. Introduction and Motivation2. How Sensitive is Optical Spectroscopy? 3. Remarks on Laser Induced Fluorescence (LIF) Spectroscopy in a
Buffer Gas Trap4. RAdioactive Decay Detected Resonance Ionization Spectroscopy
(RADRIS)Optical Spectroscopy at Americium Fission Isomers (Z = 96)
5. Ion-Guide-Detected Resonance Ionization Spectroscopy (IGRIS)Investigation of the Atomic Level Scheme of Fermium (Z = 100)
6. RADRIS with the Ion Collection and Atom Re-Evaporation MethodStatus of Laser Spectroscopy at Nobelium (Z = 102)
7. Conclusion no le
vels
kno
wn
Met
hods
1. Introduction and Motivation
Pb83Bi
84Po
87Fr
88Ra
89Ac
35Br
53I
36Kr
54Xe
85At
86Rn
104Rf
105Du
106Sg
107Bh
108Hs
109Mt
11Na
12Mg
3Li
4Be
1H
13Al
5B
7N
14Si
6C
15P
16S
80
9F
17Cl
16Ar
10Ne
2He
58Ce
59Pr
60Nd
61Pm
62Sm
63Eu
64Gd
65Tb
66Dy
67Ho
69Tm
70Yb
71Lu
90Th
91Pa
92U
93Np
95Am
96Cm
97Bk
98Cf
99Es
101Md
102No
103Lr
110 111 112
Pu94
19K
20Ca
21Sc
22Ti
23V
24Cr
25Mn
26Fe
27Co
28Ni
29Cu
30Zn
31Ga
32Ge
33As
34Se
37Rb
38Sr
39Y
40Zr
41Nb
42Mo
43Tc
44Ru
45Rh
46Pd
47Ag
48Cd
49In
50Sn
51Sb
52Te
55Cs
56Ba
57La
72Hf
73Ta
74W
75Re
76Os
77Ir
78Pt
79Au
80Hg
81Tl
82
68Er
100Fm
6d25f 6d2 5f 6d3 5f7 5f 6d145f 6d4 5f 6d75f6 5f9 5f10 5f11 5f13 5f145f12
Ds114
Uuu Uub Uuq
Why Atomic Spectroscopy of Heavy Elements?
58Ce
59Pr
60Nd
61Pm
62Sm
63Eu
64Gd
65Tb
66Dy
67Ho
68Er
69Tm
70Yb
71Lu
90Th
91Pa
92U
93Np
94Pu
95Am
96Cm
97Bk
98Cf
99Es
100Fm
101Md
102No
103Lr
Actinides
Lanthanides
no atomic spectroscopic data available
Periodic Table
Relativistic Effects for Atomic Level Scheme of Uranium
Stabilization ofs1/2, p1/2 Orbitals
Destabilization of d, f Orbitals
finite c
Spin-OrbitCoupling
non-relativistic relativistic
-60
-50
-40
-30
-20
-10
0
6s1/2
6p1/2
6p3/2
5f5/2
5f7/2
6s
6p
5f
6d7s
{E
[eV
]6d3/2, 6d5/27p1/2, 7p3/27s1/2,
c
rela-tivistic
Z*
r /a0
P(r
)
Radial Wave Functions of Relevant Orbits in PuNon-relativistic Hartree-Fock calculations taken from E. F. Worden , Jean Blaise, and Mark Fred and N. Trautmann and J.-F. Wyart The Chemistry of the Actinide and Transactinide Elements, Third Edition (2008)
(0)I Nuclear magnetic moment
eI HAIJ
Hyperfine structure interaction1. Magnetic dipole hfs
2. Electric quadrupole hfs
(0) jjS SB Q Qe Spectroscopic quadrupole moment
3. Coupling
Nuclear spin IJ F I
Isotope shift
<r2> A,A’ change of mean square charge radius
Nuclear Ground-State Properties by Atomic Physics Techniques
Requirements for Optical Spectroscopy at Trans-Einsteinium Elements
6 m 28 m
21.5 s 25.9 s 0.6 s
1.3 h3.1 m55 s
Off-line: Z 100 (Fm) breeding of material in high flux isotope reactors
Problem: Experiments at Fm with typically 1010 atoms only
On-line: Z > 100 Nuclear reactionstargets : Pb,U,Pu,Cm,Cf, Es beams : p,d,,HI (Ca)
209Bi
208Pb
No
atom
ic
spec
tros
copi
c da
ta a
re k
now
n
Problem: at σ ~ µb small production rates ~1/s 254Md253Md 255Md
252Fm25.4 h
254No 255No 256No
255Lr 256Lr 257Lr
253Fm 254Fm 255Fm
253Es
3 d 3.24 h 20.1h
252Es251Es
Ultra-sensitive Laser-Spectroscopic Methods
2. How Sensitive is Optical Spectroscopy?
How Sensitive is Optical Spectroscopy?
R.G.Voe et al., PRL 76 (1996) 2049(Toschek, Dehmelt, Neuhauser et al., 1980)
First example: Ba+ stored in an ion trap
2102
0 cm 102
)( i
kr g
g
Transition rate per atom )(1)( 00
rrik dAdP
dANdP
Power of tuneable cw dye lasers P 100 mW ... 1 W
“In principle” only 1 atom required
Flux of photons 17 18 810 ...10 / ( ) 10 / ( )2s cm s atom
ikdN PdA
Buffer Gas Trap
Radioactive Ionsfrom SeparatorT1/2 >1 ms
Buffer Gas Cell
He, Ar at 100 mbar
RIDiffusion
50 ms
1-2 cm
+
++
+ + +
+
+
+
+
+
+ ++
+
+++
+ 85% charged
15% neutral
• Laser Spectroscopy at Neutral Fraction• Ion Chemistry and Drift Time Measurements at Charged Fraction• Cooling and Bunching and Transfer to Traps for Mass Measurements
3. Remarks on Laser Induced Fluorescence (LIF) Spectroscopy
in a Buffer Gas Trap
Laser Beam
HI beam
Target
Recoil Distribution
PM
TAC
time
time
Signal
Background
LIF Signal
Laser Induced Fluorescence (LIF) Spectroscopy
G. D. Sprouse et al., Laser Spectroscopy of Light Yb Isotopes On-Line in a Cooled Gas Cell. Phys. Rev. Lett. 63 (1989) 1463Sensitivity: Target production rate about 103/s
4. RAdioactive Decay Detected Resonance Ionisation Spectroscopy
(RADRIS)Optical Spectroscopy at Americium
Fission Isomers (Z = 96)
RAdioactive Decay Detected Resonance Ionisation Spectroscopy (RADRIS)
0.9ms 1.0ms
Americium Fission Isomers
Aim: <r2>, Q20, I, gwith Optical Spectroscopy
240fAm (T1/2= 0.9 ms)242fAm (T1/2=14 ms)244fAm (T1/2=1 ms)
Dubna 1962
•conversion electron spectroscopy•lifetime measurements of excited states (charge plunger
method)•g-factor measurements• -ray spectroscopy•optical spectroscopy
d Beam 6ms on / 6ms off 12 MeV, I=3A p Beam 2ms on / 2ms off 24 MeV, I=3Ad Beam 2ms on / 2ms off 14 MeV, I=2A
242Pu (d,2n) 242fAm T1/2=14ms242Pu (p,3n) 240fAm T1/2=0.9ms244Pu (d,2n) 244fAm T1/2=1ms
0 10 20 cm
Accelerator(95 kV)
Einzel - Lens System
q~20+
5/sPu Target
60 kV 50 kV
f - Isomer Beam
=(8±3)b
f Detector
Buffer Gas Cell40 mbar Ar
Anti-CoincidenceDetector
Monitor Detector
Getter (350 °C)
Laser
H. Backe et al., PRL 80 (1998) 920
Experimental Setup
19994 20003 200040,0
0,5
1,0
1,5
RIS
-f C
ount
s [1
/mC
]C
harg
e [a
.u.]
240fAm (x2)
242fAm
0.559(32) cm-10.250(5)cm-1
241Am 243Am
10.358(14)cm-10,0
0,5
1,0
At variance with
X240f = 26.8 (2.0) (Bemis et al.)
242Pu(d,2n)242fAm, =8 b, 12 MeV242Pu(p,3n)240fAm, =8 b, 24 MeV
500.02nm50 J/cm2
351,353nm2 mJ/cm2
48179
0
19993/ cm
-1
Laser = 1.5 GHz
242f,2
24242f
exp ,2 1
1
3 4
4
I( Am) 41.4 (8)
SIS
X
240f,2
24240f
exp ,2 1
1
3 4
4
I( Am) 39.2 (8)
SIS
X
Isotope Shift Measurement in the Second Potential Minimum
-1[cm ]
_
232 236 2405
101520253035404550 U
A
Q20
[eb]
236 240 244
Pu
240 244
Am
244 248 252
Cm
Quadrupole Moments of Fission Isomers
Charge Plunger
Axes ratio 1:1.9
5.Ion-Guide-Detected Resonance Ionization Spectroscopy (IGRIS)
Investigation of the Atomic Level Scheme
of Fermium (Z = 100)
t1/2 = 4730 a
High Flux Isotope ReactorOak Ridge National Laboratory
246Cm
249Bk
249Cf
253Es255Es
•Chemical Separation of Es,
• Waiting for 255Es 255Fm decay
• Chemical Extraction of 255Fm ( t1/2= 20.1 h )
Air Shipmentto Germany
Bake OutEvaporationTests
Electrochemical Production ofFilaments at Mainz
0.9 ng 255Fm at Oak Ridge, USA
1 2 3 4 51x1010
1x1011
1x1012
FrThWeTuMoTime [d]
LaserSpectroscopy
• Breeding of 255Es (Z = 99)n = 2.6 . 1015/cm2 . s
t = 1 a
Production of 255Fm
1/2
-
39.8 dt
tantalum filament
titanium layerelectrolyticallydepositedFm-hydroxide
QMS
ChanneltronDetector
Ion OpticsSegmentedPaul Trap
90°
Deflector
0 5cmTMP
700 l/sTMP
230 l/sTMP
360 l/sTMP
330 l/s
Buffer Gas Cell35 mbar Ar
Nozzle
Electrodes
Buffer Gas Cell35 mbar Ar
LaserBeams
Filament
Ion-Guide Detected Resonance Ionization Spectroscopy with Mass Selective Ion Detection
Detuning Laser 1
Cou
nts
h1h
h
h
h
Determinationof the IPIP
26000 28000104
105
106
107
108
109
5f127s7p
MCDF CalculationsS. Fritzsche, C.Z.Dong (5f127s7p)
5I65H5
3I53G5
3H6
A ki
[1/s
]
[cm-1]
ground state5f127s2 3He
6
12400 cm
Theoretical Level Predictions for Fermium
Optical Parametric Oscillator (OPO) :~4 cm-1 (120 GHz )
SHG THG
BBO-OPO SHG
Nd-YAG Laser50 Hz, 550 mJ
532 nm~200 mJ
355 nm50 mJ
410 ---- 1000nm~ 10 mJ
205 ---- 400 nm~1mJ
Excimer Laser500 Hz, 60 mJ/PulsLambda Physics
EMG104 MSC Dye
351 nm353 nm
Bandwidth: 0.05 cm-1 (1.5 GHz)
Excimer Laser100 Hz, 200 mJ/Puls
Lambda PhysicsLPX
308 nm
Dye Lasers, Bandwidth: 0.2 cm-1 (6 GHz)MainTrigger
Dye Dye Dye Dye
308 nm50 mJ
351 nm20 mJ
> 390 nm~ 3 mJ
> 350 nm~ 5 mJ
Laser SystemsXeF
XeCl
M. Sewtz et al., Phys. Rev. Letters 90 (2003) 163002
Excimer351/353 nm
The First Optical Transition ever Observed for Fermium (Z = 100)
IP
25100
52400
0
2
_
1
_
[cm-1]_
351/353 nm
10.3 cm
2
mJ2cm
(352 – 380) nm
27385 27390 273950
5
10
15
20
27465 274700
10
20
30
40
50
28185 281900
50
100
150
200
28375 283800
1020304050607080
28385 28390 283950
20
40
60
80
100
120
25000 26000 27000 280000
50
100
150
200
R6 R7R5R4R3
Cou
nts
[cm-1] [cm-1] [cm-1] [cm-1]
Cou
nts
[cm-1]
Cou
nts
Cou
nts
Cou
nts
Scan RegionScan Region
C
ount
s
[cm-1]
Summary of Level Search
Aki ≥ 1.5 ּ◌107Aki ≥ 5.2 ּ◌106
6. RADRIS with theIon Collection and Atom Re-
Evaporation Method Status of Laser Spectroscopy
at Nobelium (Z = 102)
Experimental Setup208Pb (48Ca,2n) 254No (t1/2=55 s, a decay)
3.4 b: 5 Ions/s
The Ion Collection and Atom Re-Evaporation Method (ICARE)
Heavy ion beam(highly charged,40-90 MeV)
Buffer Gas CellAr at 50-100 mbar
Method take advantage of the85 % charged fraction
15 % neutrals
85 % charged
The Ion Collection and Atom Re-Evaporation Method (ICARE)
Heavy ion beam(highly charged,40-90 MeV)
Buffer Gas CellAr at 50-100 mbar
Method take advantage of the85 % charged fraction
15 % neutrals
85 % charged
The Ion Collection and Atom Re-Evaporation Method (ICARE)
Heavy ion beam(highly charged,40-90 MeV)
Buffer Gas CellAr at 50-100 mbar
Method take advantage of the85 % charged fraction
15 % neutrals
85 % charged
Radioactive Decay Detected Resonance Ionization with the ICARE Method
0 1 2 3 4 5 6
Collecting on DetectorCollecting on FilamentBeam offBeam on
Time [s]
Heat Pulse
Lasers
10 cm
-
Detector
Filament(Tantal)
+
++
RecoilBeam
LaserBeams
BufferGas
Pulsed
0
10000
20000
30000
40000
50000
60000
0.0
1.2
2.5
3.7
5.0
6.2
7.4
Exci
mer
lase
r 350
nm
MC
DF
calc
. S.F
ritzs
che
This
pro
ject
is s
aved
to
C:\U
sers
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ocum
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\Kon
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-Pap
ers\
2006
-Fra
uenw
oerth
\No-
leve
ls-L
aser
s
Nd
YAG
355
nm
OPO
-SH
G
Cou
pele
d C
lust
or, K
aldo
r
5f147s7p 1P1
5f147s7p 3P1
IP 50443 cm-1IP 53600 cm-1
870 ns
5,2 ns
14,6 ns
70 ns14 ns
4f146s6p 3P1
4f146s6p 1P1
E /
eV
4f135d6s2
4f135d6s2
4f146s7p
Theo
rie
Dye
lase
rs
[Rn]5f147s2 1S0
[Xe]4f146s2 1S0
Z=102Z=70
NoYb
/ cm
-1
TheoreticalPredictions
IP 53600 cm-1
Nobelium as Chemical Homolog of Ytterbium
4.0 4.5 5.0 5.50
200
400
600 Laser off
-Energie [MeV]
154Tm 154Yb155Yb152Er
156Yb
151Ho151Ho
150Dy
0
200
400
600 Laser on
Even
ts
154Yb
155Yb
152Er156Yb
151Ho151Ho150Dy
Test of the Method at 155Yb (Z=70)
λ2 = 399.6 nm
Laser 1
Laser 2
λ1 = 398.9 nm
SignalBackground
301=
107Ag(52Cr, p3n)155Yb (t1/2=1.75 s, - decay); = 15 mb, d = 0.455 mg/cm2, 4·104 Ions/s
Efficiency
Target
RI
Yb
S2Yb
NN 0.8 10
0.5 0.7 0.85 0.8 0.59 0.16 1 0.36
2SHIP Cell Ion Collect Decay Evap RIS Transp. Det0.8 10
Predictions for the 1P1 – level[1,2] (MCDF) S. Fritzsche, Eur. Phys. J. D 33, 15 (2005)
[3] (IHFSCC) A. Borschevsky et al., Phys. Rev. A 75, 042514 (2007)
[5] (MCDF) Y. Liu, R. Hutton, Y. Zou, Phys. Rev. A 76, 062503 (2007)
[6] (MCDF) P. Indelicato et al., Eur. Phys. J. D45, 155 (2007)
[4] (RCC) V.A. Dzuba et al., Phys. Rev. A 90 (2014) 012504
[7] (Extrapolation) J.Sugar, J. Chem. Phys. 60 (1974) 4103
Multi-Configuration Dirac Fock (MCDF)Intermediate Hamiltonian Fock-space coupled-cluster (IHFSCC)Relativistic coupled cluster (RCC)
Search for an Atomic Level
7. Conclusions• Resonance Ionization Spectroscopy (RIS) in gas cells is a
powerful laser spectroscopic method at samples in the order of only 1010 atoms or production rates as low as 1/s.
• 240-244fAm 0.9–14 ms on-line 106 - 107 RADRIS• 255Fm 20.1 h off-line few 1010 IGRIS
Prospects• 254No 55 s on-line 106 - 107 RADRIS• Method has been tested with an on-line laser spectroscopy
experiment at the chemical homologue 155Yb. An overall efficiency of ~ 1% has been measured.
• The experiment at 254No at GSI for an atomic level search is well prepared but is difficult and requires a lot of beam time.
• Activities are also underway at KU Leuven (Belgium) within the Heavy Element Laser Ionization Project (HELIOS) to be performed at the SPIRAL-2 facility at GANIL (France).
no a
tom
ic n
leve
ls k
now
n
H. BackeM. DahlingerA. DretzkeM. HiesT. KolbH. KunzP. KunzW. LauthP. SchwambM. Sewtz
K. EberhardtC. GrüningP. ThörleN. TrautmannJ.V. Kratz
Institut fürKernchemie
Universität MainzGermany
Institut fürKernphysik
Universität MainzGermany
Institut fürPhysik
Universität MainzGermany
ORNLOak Ridge
USA
Max-Planck-Institutfür Kernphysik
HeidelbergGermany
R.G. Haire
G. GwinnerR. RepnowD. Schwalm
G. HuberJ. LassenG. Passler
D. AckermannM. BlockF.-P. HeßbergerS. HofmannH.-J. KlugeM. Laatiaoui
GSI Helmholtzzentrum für
SchwerionenforschungGermany
Institut für Angewandte Physik
Technische UniversitätDarmstadt, Germany
F. LautenschlägerTh. WaltherHelmholtz-Institut
Mainz, Germany
M. BlockM. Laatiaoui
TRIUMFVancouver, Canada
P. Kunz