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An overview of the research activities and perspectives:From stable (high Intensity) to radioactive nuclear beams
Giacomo de Angelis
Gravitational wavesand General Physics
Gravitational wavesand General Physics
Interdisciplinary researchesInterdisciplinary researchesNuclear PhysicsNuclear Physics
Accelerator technologiesAccelerator technologies
Infrastructures of LNL
45004500 55005500
hourshours of of beambeam on targeton targetÞ Þ Au / from Au / from AkeVAkeV 20 20
AMeVAMeVfromfrom few few pnApnA few pfew pµµAA
10.00010.000
Interdisciplinaryactivities and applications
Nuclear Physics46% non-INFN
INFM, ENEA, ISS, Universities
CN CN ANAN--2000 2000 LinacLinac ALPIALPITandem XTUTandem XTU++
ALPI Output Energy
0
10
20
30
0 50 100 150 200 250A
E/A
[MeV
/u]
Tandem (G-F) (1-10 pnA)PIAVE+Alpi (40-200 pnA)
New Injector
Tandem
High intensity beams of stable heavy elements
LNL MAIN INSTRUMENTS
88ππLPLP
GASPGASP
PRISMAPRISMA
GarfieldGarfield
RadiobiologiaRadiobiologia
CLARACLARA
EXOTICEXOTIC
Individual users asking for accessto the Research Installations
260
100
183
135
166
168
273
277
162
305
228
356
0
100
200
300
400
500
600
1998 1999 2000 2001 2002 2003
years
Italian GuestsForeign guests
“Transnational Access to major Research Infrastuctures” Improving the Human Research Potential and Socio-economic Knowledge Base”
MAN-DAYS (2000/2003) DISTRIBUTED BY THE COUNTRY OF ORIGIN OF USERS
total amount of man-days 2981
16267
13
76
5
258
873
5
199
275
912
52 144 11 368123
247
28
BelgiumDenmarkGermanyGreeceSpainFranceItalyNetherlandsPortugalSwedenUnited KingdomBulgariaCyprusHungaryIsraelPolandRomaniaSlovakiaOther
Nuclear Structure at LNL Nuclear Structure at LNL
44,46Ar
n-rich Pd, Cd50Fe
58Cu64Ge
103Sn70,72,73Br
67Se
88Ru
66As
68,70Ni
•New symmetries at the critical point•Rotational damping
•New symmetries at the critical point•Rotational damping
156Dy
132,134Pr,139Sm133,134,135,136Nd
142,148Gd
• High spin states and superdeformation
• Chiral Symmetry in Nuclei
• High spin states and superdeformation
• Chiral Symmetry in Nuclei
• Clustering and reflection asymmetric shapes
• Collectivity and shell model • Isospin symmetries and mirror
pairs• Isospin mixing in N=Z nuclei• Spectroscopy at the dripline
• Clustering and reflection asymmetric shapes
• Collectivity and shell model • Isospin symmetries and mirror
pairs• Isospin mixing in N=Z nuclei• Spectroscopy at the dripline
• Shell stability and shell evolution • Shell stability and shell evolution
High intensity (100 pnA) beams of stable heavy ions complementary to RIBS
Transition Matrix Elements in mirror pairs
R. Du Rietz et al. PRL 93,222501 (2004)
Isospin Mixing and Mirror Simmetries
Electromagnetic spin-orbit term ?
Ekman et al.PRL 92,132502 (2004)
Quasi-molecular states in nuclei
Cou
nts
Energy (keV)
Gamma-Ray Spectrum192Hg
Thummerer et al.NPA734 (2004) 453
Critical-Point Symmetries
Observed in 134Ba
Observedin 152Sm
Extended Casten symmetry triangle
Comparison of the Excitation Energy Ratios for the N=90 Rare earth isotones
150Nd, 152Sm, 154Gd and 156Dy with the prediction of the X(5) symmetry
R. F. Casten and N. V. Zamfir, Phys. Rev. Lett. 87 (2001)052503.R. F. Casten and N. V. Zamfir, Phys. Rev. Lett. 87 (2001)052503.
R0/2=E(02+)/E(22
+)
R4/2=E(41+)/E(21
+)
D. Tonev et. al., Phys. Rev. C 69 (2004) 034334.D. Tonev et. al., Phys. Rev. C 69 (2004) 034334.
R42/22=E(42+)-E(02
+)/E(22+)-E(02
+)
Transition Matrix elements and X(5) symmetry
Comparison of the experimental level scheme of 154Gd with the X(5) predictions.The E(21
+) value (in keV) and the B(E2; 21+ 01
+) value (in W.u.) are normalizedto the experimental data.
F. Iachello, Phys. Rev. Lett. 87 (2001) 052502.F. Iachello, Phys. Rev. Lett. 87 (2001) 052502.
D. Tonev et. al., Phys. Rev. C 69 (2004) 034334.D. Tonev et. al., Phys. Rev. C 69 (2004) 034334.
Does Chiral symmetry exists in nuclei ?
“I call any geometrical figure, or group of points, chiral, and say it has chirality, if its image in a plane mirror, ideally realized, cannot be brought to coincide with itself.” - Lord Kelvin 1904
Examples of chiral systems are found in :Chemistry: molecules
with opposite handedness react differently in similar environments
Biology: DNA has right and left-handed “screws”
Particle Physics
Nuclear Physics: Current distributions in nuclei
Triaxial odd-odd nuclei result in 3 perpendicular angular momenta for p-h configurations built on high-j orbitals
The energies of the excited states for the left-handed and right-handed systems should be identical
The energies of the excited states for the left-handed and right-handed systems should be identical
V. I. Dimitrov et al, PRL 84 (2000) 5732V. I. Dimitrov et al, PRL 84 (2000) 5732
Does Chiral symmetry exists in nuclei ?Planar to a-planar phase transition ?
D. Tonev et al.
IBFFM
S. Brant et al, PRC 69 (2004) 017304S. Brant et al, PRC 69 (2004) 017304
High Intensity Stable Beams and Neutron Rich Nuclei
Stable nuclei: N/Z ≈ 1 - 1.5, Sp ≈ Sn ≈ 6 - 8 MeV
Homogeneously mixed protons and neutronsGood mean-field descriptionGood “single-particle” picture (magic numbers)Large gaps between major shellsEmpirical shell-model interactions
Very neutron-rich nuclei: N/Z ≈ 2 - 2.5, Sn << 1 MeV
Diffuseness of neutron distribution (neutron skins & halos)More states near the Fermi surfaceBreakdown of the single-particle descriptionRedefinition or disappearance of magic numbersUnknown shell-model interactions
Reduction of spin-orbit potential
Phys. Lett. B 418, 7 (98) D.VretenarN
neutronsprotons
The Properties of Nuclei with Extreme N/Z-Ratios
Disappearance of ShellStructure?
• Basic nuclear properties of rare isotopes (e.g., masses, half-lives, …) determine element formation in the cosmos
Element formation in r-process: quenching of shell-structure?Pfeiffer et al., Z. Phys. A357 (1997) 235
Cautions in jumping to conclusions about shell modificationsrelated to diffuse density distribution:
“Single particle” orbitals are dressed even in semi-magic nuclei
• Effective single-particle energy (ESPE)
ESPE : Total effect on single-
particle energies due to interaction with other valence nucleons
Monopole interaction, vm
ESPE is changed by N vm
N particles
T. Otsuka et al. Zakopane 2004
Detecting γ-ray emittedat rest: no Doppler correction!Sensitive to the decay of levels which live longer then the stopping time
( )
( )CCMMAX
MAXTB
TLF
VERL
LAA
L
−=
⎟⎟⎠
⎞⎜⎜⎝
⎛
+=
2
2
31
2
11
72
:limit Rolling
h
µ
Populate high spin states
higher selectivity stronglyneeded
angular acceptances ∆θ~12o ∆φ~22o
solid angle ∆Ω ~ 80 msrd. target-focal plane 7 menergy acceptance ± 20%max rigidity 70 MeV amudispersion ~ 4 cm/%mass resolution ~ 1/300 FWHM B. Fornal
Clover Ge detectors from EUROBALL
82Se+238U E=505 MeV 64deg
∆ E
proton stripping channels
proton pick-up channels
fission eventsZ=50
Z=34
First experimental campaign just started
E LNL – APRIL 2004
γ-spectroscopy of neutron rich nuclei Mass distribution of 505 MeV 82Se + 238U
Se
As
Br
Kr
Ge
Ga
Zn
Cu
Ni
82
838481
80
77
76
89
8182
7978
7980
8176
75
69
7778
7473
7475
73
7170
6768 72
6564 7170
69
8685
87
81
84 8883
A
Preli
mina
ry
87Rb
84Se
667
1455
455 keV 23/2(+)→21/2(+)
82Se + 238U E=505 MeV
+3p+2n
+2n
PRC70, 024301 (2004)
Shell model in 37P and 39PBreaking of a semi-magic shell
closure far from stability
82Se+238U
36S+208Pb15
2032S+58Ni
Mirror pair 31S and 31P
Spectroscopy of 54Co Isospin non conservingpart of the effective
interaction
64Ni+238UShell model A~60
Shell closure evolution at Shell closure evolution at the magic number N=50the magic number N=50
50
32
Multi-nucleon transfer
Resonances in 24Mg+24Mg and molecular states in 48Cr
27
2840Ca+208Pb
Pairing-vibration states in 42Ca
90Zr+208Pb
24Mg+24Mg
Large-angle scattering
58Ni+60Ni
54Fe+50Cr
43% of the 43% of the TandemTandem--ALPI beam ALPI beam
time time
Research activities of Prisma-Clara in 2004
Heavy ion beams from PIAVE-ALPI strongly needed
64Ni 400MeV + 238U
Preliminary
EXP. LSSM
FPD6
LSSM
KB3G
0+2+
(4+)(6+)
(8+)
(10+)
58Cr
E4+/E2+ = 2.20E4+/E2+ = 2.20
E6+/E2+ = 3.65E6+/E2+ = 3.65
vibrator to γ-unstable rotor
E(5) critical point symmetry
B. Fornal, R. Broda et al.
Identification of new statesbased on γ-coincidences (cross-coincidences) between the two binary products
Neutron rich heavy projectiles allow to use transfer reactions as a ∆N-∆Z filter for driving the multi-nucleon transfer flux to exotic regions
beams of heavy ions or neutron-rich radioactive beams
Transfer induced by Neutron Rich (radioactive) Beams
Driving the multi-nucleon transfer flux to very exotic regions
p-rich
n-rich
Coupled channel calculations (Grazing).G. Pollarolo RIB n-rich
Understand the relative weight of the sequential transfer of single nucleons, of pair transfer or the more complex transfer of clusters.
Enhancement of the pair-transfer mode due to the dropping of the two-neutron separation energy as a function of the neutron excess
Gamma Arrays based on ComptonSuppressed Spectrometers
ε ∼ 10 — 5 %( Mγ=1 — Mγ=30)
GAMMASPHEREEUROBALL
Gamma Arrays based on ComptonSuppressed Spectrometers
ε ∼ 10 — 5 %( Mγ=1 — Mγ=30)
GAMMASPHEREEUROBALL
Tracking Arrays based onPosition Sensitive Ge Detectors
ε ∼ 40 — 20 %( Mγ=1 — Mγ=30)
GRETAAGATA
Intermediate step Exogam, Miniball, SeGa : optimized for Doppler correction at low γ-multiplicitiy
Ingredients of Gamma Tracking
Pulse Shape Analysisto decompose
recorded waves
Highly segmented HPGe detectors
··
Identified interaction
points
(x,y,z,E,t)iReconstruction of tracks evaluating permutations of interaction points
EγEγ1
Eγ2
e2
e3
1
3
θ1
θ2
e1
0 2
Digital electronicsto record and
process segment signals
1
2
3
4
Reconstructedgamma-rays
AGATA/GRETA Prototypes 2
May, 2004 April, 2004
Courtesy J.Eberth, IKP Cologne Courtesy I-Yang Lee, LBNL
Solid Angle = 80 msr Energy accept. 20%∆m/m = 1/300 ∆E/E=1/1000
64Ni (390 MeV) + 238U
54535251504948474645
With the PIAVE Xe beams
With present ALPI beam
First phase of AGATA15 clusters (1π)4 x efficiency
larger selectivity
Reaction Mechanisms at LNLReaction Mechanisms at LNL
p(17O, 17F )n 105
pps
Break-up ofExotic light nuclei
Break-up ofExotic light nuclei
Fission dynamicsSymmetry energy and stellar collapse
Fission dynamicsSymmetry energy and stellar collapse
Multifragmentation at low excitation energyMultifragmentation at low excitation energy
132Ce
N/Z=1 N/Z=1.38
+
N/Z=1.25 N/Z=1.29
Z
N Z
N/Z=1.28
N/Z=1.28
N
+
γ γ
γ
γγ
γ
132Ce
96Mo
100Mo32S
36S
γγ
D(t=0)=18.2 fm
D(t=0)=1.7 fm
GDR response probing shapesand non uniform charge and mass distributions in nuclei
GDR response probing shapesand non uniform charge and mass distributions in nuclei
PISOLORMSPRISMA8πLPGARFIELD
Deformed protonemitters
Deformed protonemitters
Sub-barrier fusion: Fusion dynamics and nuclear structure
Sub-barrier fusion: Fusion dynamics and nuclear structure
z
A40Ca
Fission dynamics in the super-heavy mass region
E (a.u.)
TOF
(a.u
.)
Influence of Q.F. on fusion process
Scattered beam
Fusion
A - TOF CORSET
Fission dynamics in Super-Heavy region80Se + 208Pb 470 MeV
Fission dynamics in Super-Heavy region80Se + 208Pb 470 MeV
Neutrons12 scintillators 2m from the targetFission Fragment PPAC 5 x 4 cm2 for TOF, 2 MWPC 13 x 13 cm2
No evidence for symmetricsplitting events, corresponding to
Fusion-Fission reactionsNevertheless:
Pre-scissioncomponent
Evidence of a longtransient delayin asymmetric
splitting (DIC-like) suggesting the formation of a
composite Super-heavy system
SHE - InstrumentationCompetition between the
Quasi-Fission e Fusion-Fission mechanismsCompetition between the
Quasi-Fission e Fusion-Fission mechanisms
DEMON: Détecteur Modulaire de Neutrons(belgian-french collaboration: ULB, UCL, LPC, IReS + LNL)
DEMON
40 NE513 + FF + BaF2
Fission dynamics in the super-heavy mass region340 MeV 28Si + 232Th: PRC 65 (2002) 646 and NPA to be published
Multi-source fit to the experimentalneutron and a energy spectra
pre- and post-scission multiplicities
Fission Fission delaydelay timetime ttDD
Elab (MeV)
α = 35.4°β = 25.9°
α = 24.9°β = 36.1°
α = 9.2°β = 42.1°
α = 335.1°β = 36.1°
α = 324.6°β = 25.9°
α = 318.9°β = 13.5°
α = 41.1°β = 13.5°
α = 350.8°β = 42.1°
d2 M/d
ΩαdE
α(s
ter-1
MeV
-1)
Comparing neutron prescission multiplicities with Statistical Model a tD~5x10-20 s is obtained.
GasLiquid
Density ρ/ρ0
Big Bang
Neutron Stars
Tem
pera
ture
20
200
MeV
1 5?
Plasma of Quarks and
Gluons
Nucleus
Dense matter EOS
Crab nebula
July 5, 1054
Collisions
HeavyIons
32S + 58Ni (grey), + 64Ni (hatched)
0
0.2
0.4
0 1 2 3 4
Z=1
0
0.2
2 3 4 5 6
Z=2
0
0.05
0.1
5 6 7 8 9
P(A
)
Z=3
0
0.05
0.1
6 7 8 9 10 11
Z=4
0
0.05
9 10 11 12 13A
Z=5
0
0.05
10 11 12 13 14 15A
Z=6
80% of Zp+ZT
Evaporation residues and fragments measurement: from fusion to multifragmentation
With the last upgradealso Isotope
identification:
• 3rd coordinate in thephase space
•Temperature informationof the emitting source
To be checked : • same charge of the emitting systems formedthrough the differententrance channels through comparison to models(charge correlations,charge distributions
etc.)• same temperature of the emitting sources• same volume (through correlation functions)
Signals already at lower energy11AMeV
InterdisciplinaryResearches
SPATIAL RESOLUTION < 100 µm
Images of seven holes 300 µm in diameter and 100 µm spaced
Vdrift= 50 V 100 V 200 V 500 V
Zoom effect as function of the drift voltage
LM
a
High reflectance mirrors for solar coronaHigh reflectance mirrors for solar coronaMOT trapsMOT traps
Detection ofexplosives
Detection ofexplosives
Detector technologyDetector technology
Surface analysisSurface analysis
Tissue equivalent proportional counters
Tissue equivalent proportional counters
Radiation biologyRadiation biologyNb sputtering into Cu cavities
Tests of the Standard Model - Atomic Parity violation
Precision tests of CP, P violation and unitarity of CKM matrix; physics beyond VA; and measurements of sin2ΘW at low q
215Fr: CN* formed in 18O+197Au
TRAPPING OF 85RB
Interdisciplinary & Biomedical Physics FacilitiesNan
odos
imet
ric
stru
ctur
eof
had
ron
trac
ks DNA
Ionization events
Biological sample holder
Beam extraction window
Beam-pipe
Cooled-CCD
Microbeam facility for single cell irradiation
Tissue
equiv
alent
propor
tional
count
ers Radiation biology
Radiobiological studies:Radiobiological studies:
• Light ion broad-beam irradiation facility at the 7MV Van de Graaff CN electrostatic accelerator (protons, deuterons, helium-3 and helium-4 ions; E: 0.8-12 MeV)
• Heavy ion broad-beam facility at the Tandem-ALPI accelerator complex (A>4; E: 5-26 MeV/amu)
• Light single-ion microbeam facility for single-cell irradiation at the 7MV Van de Graaff CN electrostatic accelerator (protons, deuterons, helium-3 and helium-4 ions; E: 0.8-12 MeV)
• Fully equipped biology Laboratory
2
Main Activities at LNLMain Activities at LNL
• Cell inactivation
• Gene mutation
• Mutation characterization
• Chromosome aberration
• influence of chromosome architecture in aberration formation
• Protein expression in normal and tumoral cells.
…Particular emphasis on the low-dose and low-dose rate effects……bystander effects and cell-to-cell communication.
Mainly performed in the framework of INFN and EU Contract projects.
INFN-LNL Radiobiology Laboratory
Relative Biological Effectiveness (RBE) Relative Biological Effectiveness (RBE) vsvs Linear Energy Linear Energy Transfer (LET) of light ions for cell inactivation in V79 cellsTransfer (LET) of light ions for cell inactivation in V79 cells
5
• ADVANCED THIN FILM MATERIALSSynthesis and Process Development
• Plasma Sputtering Deposition
• Plasma Diagnostics
• Ion Implantation
• Low Friction, High Hardness NanoscaledMaterials and Multilayers
• Extreme UV and soft X-rayoptics development
• Insulating Oxides and High Performance Plastics
Characterization of Physical Properties• ADVANCED THIN FILM MATERIALS
Composition
• Ion Beam Analysis (RBS, NRA, ERDA, PIXE)
• Microbeam (Micro-PIXE 2-D trace element analysis)
Mechanical Characterization• Nano Hardness / Stress• Adhesion (Micro Scratch)• Atomic Force Microscopy
Nuclear Physics Perspectives at LNLNuclear Physics Perspectives at LNLtime
Tandem+Alpi High intensity stable beams from SPES to Eurisol
Moderately neutron rich nuclei by means of high intensity stable beams
Multi-nucleon transfer and deep-inelastic collisions as a way to access n-rich nuclei: The Clover array + PRISMA
Medium size next generation RIB facility, away to Eurisol
Advanced Gamma-rayTracking Array and otherIntegrated Infrastructure Initiatives
A Superconductive Linac as a test benchfor Eurisol
Nuclear Structure andDynamics at the limits (spin and isospin)
PIAVE
First superconduttive RFQ in operation in the world
PIAVE first beams in Dic 20041603+: I= 430 pna; transmission 40-50%
129Xe18+: I = 5.5 pna; transmission 25-30%Injection Test in ALPI: since Feb 2005
PIAVEALPIECR
RFQQWR
SRFQ1 SRFQ2
QWR
1.3 MeV/u
PIAVE
EXPERIMENTALHALLS 1, 2
EX.
HALL
3
CR10 CR9 CR8 CR7 CR6 CR5 CR4 CR3 B2
CR12 CR13 CR14 CR15CR16 CR17 CR18 CR19 CR20 B4
COLD BOX
TANDEM
β=0.056, 80 MHz, full Nb
β=0.13 160 MHz Nb/Cu
β=0.11, 160 MHz,Nb/Cu
B3
β=0.110, 160 MHz,Pb/Cu
2.3 MV/m 4.4 MV/m
Larger Beam IntensitiesSuperconductive LINAC with Nb/Cu resonators
Intensities ~ 100 pnA
LinacLinac ALPIALPITandem XTUTandem XTU
++
LinacLinac ALPIALPI
++
PiavePiave
Test of the standard model
Test of the trapping efficiency
Trapping of Francium atoms
EXOTICEXOTIC :Light exotic beams by inverse kinematics reactions
Production reactions
p(17O, 17F )n3He(6Li, 8B )n7Li(9Be, 6He )10B
p(7Li, 7Be )n
p(14N, 14O )n 3He(16O, 18Ne )n
5 MeV
100 MeV
BNCT Be converterU target
ISCLRFQ
Source TRIPS
Ion source
Isotope separator
ALPIExp. SRFQ
Charge state separator
High resolutionspectrometer
Chargebreeder
Neutron rich unstable beams Starting construction 2005
238UPrimary p beam Fission fragments
converter
n
1 mA *100 MeV = 100 kW 1013-14 f/s300 W
108 132Sn/s0.02 pnA
132Sn at 16 MeV/uALPI
Supercond.p linac
100 MeV
Be or 13C100 kW
4 Kg UCx
238UPrimary p beam Fission fragments
238UPrimary p beam Fission fragments
converter
n
converter
n
1 mA *100 MeV = 100 kW 1013-14 f/s300 W
108 132Sn/s0.02 pnA
132Sn at 16 MeV/uALPI
Supercond.p linac
100 MeV
Be or 13C100 kW
4 Kg UCx
132Sn at 16 MeV/uALPI
Supercond.p linac
100 MeV
Be or 13C100 kW
132Sn at 16 MeV/uALPI
Supercond.p linac
100 MeV
Be or 13C100 kW
4 Kg UCx
ISOL facility
SPES p and d driverEp,d=100 MeV I~1-10 mA
Spiral2 project
GANIL
SPES projectLNL
Fragments produced by each proton(in the Ucx target)
Sn132
The nominal beam is of 1.7 x 1016 p/s.
Tetrahedral symmetry and
Spherical harmonicsTetrahedral symmetry in nuclei ?
The lowest order: λ=3
Shells at
Z,N= 16, 20, 32, 40, 56, 70
J. Dudek et al., PRL 88 (2002) 252502
Quasi-elastic reactions?
Summary
• LNL as a multidisciplinary nuclear physics based user oriented laboratory
•Nuclear Structure and Reaction based facilities•Infrastructure for applied physics•Interdisciplinary and biomedical physics facilities
• LNL as an high intensity stable heavy beam facility :a short term perspective
• Neutron rich radioactive beams at LNL : the SPES project
• New detectors (Prisma-Clara) and powerful Ge detectors based on gamma ray tracking
LaboratoriNazionalidiLegnaro
129 Guests
45 Fellowships and grants
23 Students and Ph.D. Students
297 Italian researcher126 EU researcher119 non EU researcher
14 workshops and meetings
74 Publications in Journals
20 International Conferences
Present ALPI output energy –Tandem injector
Tandem 15 MV; F,F1998 : 11 Pb/Cu cryostats2003: 13 Nb/Cu cryostats
ALPI
0
5
10
15
20
25
30
0 20 40 60 80 100 120 140
AALP
I out
put [
MeV
/u]
ALPI Dec 1998
ALPI 2003 (low beta not included)
ALPI 2003 (low beta included)
12C6+ 28Si11+ 40Ca14+ 63Cu17+
16O7+ 32S12+ 58Ni17+ 79Br18+ 90Zr19+ 127I 21+
LEGNARO
Near future switching from a Tandem to a q+ injector (PIAVE)
ALPI Output with the two Injectors
0
10
20
30
0 50 100 150 200 250A
E/A
[MeV
/u]
Tandem+ALPI (G-F) (1-10 pnA)
PIAVE+ALPI (40-200 pnA)
New Injector
Tandem
• MORECURRENT
• HEAVIERMASSES
• MORE BEAM TIMEAVAILABLE (TWO INJECTORS)
LEGNARO
Energy outputPIAVE injection, 2004 ALPI
LEGNARO
0.0
5.0
10.0
15.0
20.0
25.0
30.0
0 50 100 150 200 250A
MeV/u
High currentHigh energy
12C5+ 16O6+
14N5+ 40Ar8+ 58Ni11+ 84Kr12+ 120Sn16+ 132Xe17+ 181Ta 24+ 197Au26+ 208Pb25+ 238U28+
12C5+ 16O7+
14N6+ 40Ar14+ 58Ni17+ 84Kr18+ 120Sn19+ 132Xe27+ 181Ta 24+ 197Au29+ 208Pb25+ 238U31+
1
PIAVE: - 2 SRFQs at the design accelerating fields- 8 low β resonators at 5 MV/m
ALPI - 12 low β resonators operating at 4.4 MV/m- 44 medium β resonators operating at 4.4 MV/m- 8 high β resonators operating at 5.5 MV/m