laser spectroscopy on bunched radioactive ion...
TRANSCRIPT
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Laser Spectroscopy on BunchedRadioactive Ion Beams
Jon BillowesUniversity of Manchester
Balkan School on Nuclear Physics, Bodrum 2004
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Balkan School on Nuclear Physics, 2004
Lecture 1.
Lecture 2.
1.1 Nuclear moments
1.2 Hyperfine interaction in free atoms
1.3 Lasers and laser spectroscopy
1.4 Collinear-beams laser spectroscopy
2.1 Ion beam cooling and bunching
2.2 Experiments with bunched beams
2.3 Laser ionization techniques
www.man.ac.uk/dalton/files
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Summary of Isotope Shift and Hyperfine Structure
Isotope shift ofatomic transition
176Hf 178Hf
Analysis yields thechange in nuclearmean square chargeradius
Nuclear size, static anddynamic deformations
Hyperfine structureof atomic transition
177Hf
Nuclear spin I
Magnetic moment µ
Quadrupole moment Qs
ppm shift
(Isotope shift foundusing centroids ofhyperfine multiplet)
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+40 kV
Ion beamcooler
Light collection region(Laser resonance fluorescence)
Reduces energy-spread of ion beam
Improves emittance of ion beam
Trap and accumulates ions – typically for 300 ms
Releases ions in a 15 µs bunch
2.1 Ion beam cooling and bunching
Fast ion beam
Ions accelerated while still in low-pressurehelium acquire a large energy spread – thecollinear-beams method loses both resolutionand sensitivity.
Solution: an ion beam “cooler”
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The JYFL cooler/buncher
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Principle of RFQ trap
Time-averaged force towards central axis
Damping of motion provided by low-pressure helium gas at room temperature
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Bunching ions in the RFQ cooler
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+40 kV
Ion beamcooler
Light collection region(Laser resonance fluorescence)
Reduces energy-spread of ion beam
Improves emittance of ion beam
Trap and accumulates ions – typically for 300 ms
Releases ions in a 15 µs bunch
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Background reduction by signal gating
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Sensitivity gains using the RFQ ion-cooler
8000 ions/sec
5.3 hours
2000 ions/sec
48 minutes
Photons from laser-excitation of radioactive 88ZrLaser frequency
200
100
30
0
BEFORE
AFTER
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2.2 Experiments with bunched beams
1. Zr isotopes – shape changes near N=50 shell
2. Ce isotopes – shape transition at N=60
3. Neutron-deficient Ti – proton skins?
4. High spin isomers – effect of pairing reduction?
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Fission product yields at IGISOL (25 MeV p + 238U)Neutron number
Prot
on n
umbe
r
Zr
V. Rubchenya
Fission fragment spectroscopy
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Charge radii of Zr isotopes
40Zr
mea
n sq
uare
cha
rge
radi
us
Deformed nucleus
Spherical nucleus
Spherical droplet modelMyers & Schmidt, Nucl. Phys. A410 (1983) 61.
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Radii predictions for 40Zr from B(E2) values
40Zr
(Very similar to 38Sr behaviour)
Shaded areas: only B(E2) to thefirst 2+ state used.
Should also include higher statesand B(E3) strenghts.
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Isotope shifts of neutron-rich Ce
331 nm (Ce+)
Mea
n sq
uare
cha
rge
radi
i
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Brix-Kopfermann plot
(differential changes in mean square charge radii)
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Light Ti isotopesIs 44Ti an α-cluster nucleus?
orOff-set centre
of mass
In fact: almost no differencein predicted rms radius!
Neutron number
40Ca40Ca
Produced by 45Sc (p, xn) 46-xTi
Does 42Ti have a proton skin?
(the laser measurement would bevery sensitive to this)
T1/2 = 200 ms
42Ti
44Ti
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Comparison with RMF (G. A. Lalazissis etal., Nucl. Phys. A628 (1998) 221
Comparison withneighbouring chains
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The K=8 isomers in 130Ba and 176Yb
Structure of 2-neutron 8-
state in 176Yb
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The 176Yb K=8 isomer
Production: (d,pn) at 13 MeV, 5.5 µA
Flux: 200 isomers/sec (total flux at A=176: 8,400 ions/sec)
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16+
8-
23/2-
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Calculation by Bordeaux Group(Quentin, Pillet, Libert)
Without pairing effects,Isomer shift = +0.092 fm2
Including pairingIsomer shift = -0.086 fm2
(Experiment: -0.076(12) fm2)
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• Similar features now found in 4isomers: smaller radius than groundstate, but not due to reduction indeformation.
• Effect greatest for 4qp state.• Effect for 2qp isomer is about twice
the normal odd-even staggering (a1qp effect?).
Explaining 178Hf (16+) isomer shift
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New development: Laser ion source FURIOS(using laser resonance ionization)Powerful pulsed lasers can be tuned to ionizeneutral atoms of a selected element with highefficiency
2-laser scheme 3-laser scheme
Applications:
Laser ion sources – beams selected by mass and atomic number
Ultra-high sensitivity laser spectroscopy – collinear beams RIS
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The CRIS method
5 µs 10 ns50 Hz
repetitionrate lasers
Atom bunch
50 Hz delivery rate,synchronized with
laser pulse
All atoms from the ion sourcehave a chance to be ionized
Resonance located by ioncounting (not photon counting)
Doppler-broadening free
Ionizationlimit
308 nm
532 nm
Off-linetests with
27Al
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Collinear resonance ionizationspectroscopy
Chargeexchange cell
Ionizationregion
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Laser fluorescencespectra – 27Al
Detection efficiency:1 photon detected per50,000 atoms in beam
308.2 nm
309.3 nm
309.2 nm
1.5 GHz
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Comparison with low-fluxbunched beams
1.5 GHz
Photon counting (12 minutes)
Ion counting (4 minutes)
Sensitivity:1 resonance ion per 30 atoms
within 1 µs time window
(compared with 1 photon per50,000 atoms)
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Laser transportation and atom beam overlap
Laser beams
Ti:Sa 1
Ti:Sa 2
Ti:Sa 3
Nd:YAG
Ion beam toexperiments
Cyclotron beam
~ 10cm
Dye 1
Dye 2
CVL
Ion guide
RF multipole
Mass separator
Laser system
Gas inlet
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(Fast Universal Resonant laser IOn Source)
Penning TrapMassspectroscopy RFQ cooler
Collinearlaserspectroscopy
Ti:Sapphire lasers
Nd:YAG pumplaser
Ion GuideDecayspectroscopy
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1H 2He
3Li 4Be 5B 6C 7N 8O 9F 10Ne
11Na 12Mg 13Al 14SI 15P 16S 17Cl 18Ar
19K 20Ca 21Sc 22Ti 23V 24Cr 25Mn 26Fe 27Co 28Ni 29Cu 30Zn 31Ga 32Ge 33As 34Se 35Br 36Kr
37Rb 38Sr 39Y 40Zr 41Nb 42Mo 43Tc 44Ru 45Rh 46Pd 47Ag 48Cd 49In 50Sn 51Sb 52Te 53I 54Xe
55Cs 56Ba 57La 72Hf 73Ta 74W 75Re 76Os 77Ir 78Pt 79Au 80Hg 81Tl 82Pb 83Bi 84Po 85At 86Rn
87Fr 88Ra 89Ac 104Rf 105Ha 106 107 108 109 110 111 112 113
58Ce 95Pr 60Nd 61Pm 62Sm 63Eu 64Gd 65Tb 66Dy 67Ho 68Er 69Tm 70Yb 71Lu
90Th 91Pa 92U 93Np 94Pu 95Am 96Cm 97Bk 98Fc 99Es 100Fm 101Md 102No 103Lr
V. Fedoseyev, ISAC-TRIUMFLIS Workshop, 2000
Accessibility of elements using lasers
Elements studied with dye laser RIS
Dye laser RIS possible
Ti:Sapphire laser RIS demonstrated
Ti:Sapphire laser RIS possible
NIPNET meeting, NIPNET meeting, SaariselkaSaariselka, April 2004, April 2004
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End of Lecture 2
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