近代核子物理實驗 中央研究院 物理所 章文箴 2008/07/11 (五) 台大物理系...
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![Page 1: 近代核子物理實驗 中央研究院 物理所 章文箴 2008/07/11 (五) 台大物理系 111 教室 2008 年雷射電漿物理暑期學校 【電漿實驗專題】](https://reader033.fdocument.pub/reader033/viewer/2022061519/5a4d1ace7f8b9ab0599706d2/html5/thumbnails/1.jpg)
近代核子物理實驗
中央研究院 物理所 章文箴2008/07/11 (五)
台大物理系 111 教室
2008 年雷射電漿物理暑期學校【電漿實驗專題】
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Outline
• Discovery of nuclear structure• Development of “modern” nuclear physics
Nuclear structure at extreme and excited states Hadron physics with laser-electron photon
• Laser Nuclear Physics
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Discovery of nuclear structure
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A Wide Range of Scale in Observation
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Mendeleev and Periodic Table
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Models of Atom
Thomson model of atom
Rutherford model of atom
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Rutherford experiment
•From angular distribution of rescattered -particles Rutherford concluded existence of positively charged core of atom then called nucleus
•The size of the nucleus was much smaller(10-14m) than size of the atom (10-10m)
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Angular distribution of scattered -particles
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Development of modern nuclear physics
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Stable nuclei
Stable and decaying nuclei
All observed nuclei:- stable nuclei- decaying nuclei- particle emitting nuclei
proton-rich
neutron-rich
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beta + proton neutron+ light particles
beta - neutron proton+ light particles
alpha emission of 4He2 protons + 2 neutrons
fission break-up of a nucleus two light nuclei
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Nuclear Stability
Stable nuclei
Proton unstable
Neutron unstable
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prot
ons
neutrons
Designer Nuclei in Nuclear Designer Nuclei in Nuclear LandscapeLandscape
82
50
28
28
50
82
2082
28
20stable nuclei
known nuclei
126
superheavynuclei
terra incognita
• How do protons and neutrons make stable nuclei and rare isotopes?
• What are properties of neutron matter?
• What are the heaviest nuclei that can exist?
• What is the origin of simple patterns in complex nuclei?
45Fe62Ga
11Li
225Ra
149Tb
134Sn
283112
101Sn
78Ni68Se
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Radiation Detectors
• Photographic Film To detect , and radiations
• Spark counter To detect -particles
• Ionization Chamber To detect -particles
• Cloud Chamber To detect and particles
• Geiger-Müller Tube To detect , and radiations
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What is an isomer ?
Metastable (long-lived) nuclear excited state.
‘Long-lived’ could mean
~10-19 seconds, shape isomers in alpha-clusters or
~1015 years 180Ta 9-->1+ decay.
Why/when do you get isomers?
If there is (i) large change in spin (‘spin-trap’)
(ii) small energy change
(iii) dramatic change in structure (shape, K-value)
Isomer ?
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Excited State of Nuclei
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Superdeformed Nuclei
• A band terminates when all valence particles outside a doubly magic (spherical) core are aligned
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Astrophysical Consequences of Isomers
Ta is ‘stable’ in its isomeric state, but its ground state decays in hours!
Longstanding problem as to how the isomeric state is created in nature (via eg. S-process). Possible mechanism via heavier nuclei spallation or K-mixing of higher states in 180Ta.
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+++++
---
--
225Ra
Over the last decade, tremendous progress has been made in techniques to produce designer nuclei, rare atomic nuclei with characteristics adjusted to specific research needs
45Fe
18F,22Na149Tb
nuclear nuclear structurestructure
astrophysicsastrophysics
applicationsapplications
tests of tests of fundamental fundamental
laws of naturelaws of nature
Some nuclei are more important than others
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Medical Imaging - 99mTc
Technetium-99m a metastable isomer that decays into 99Tc by emission with a half-life of 6h.
Then decays into ruthenium by emission, but with a half-life of 2.1 x 105 years.
N.B. As a gamma emitter, 99mTc remains the same element during its residence in the body so it doesn’t change its chemistry when it decays.
99 9943 43mTc Tc
99 99 043 44 1Tc Ru e
Highly penetrating radiation.
Long half-life = low activity.
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Gamma camera CT scanner
E.g. -camera image of 131I (from NaI solution) uptake in a normal and diseased thyroid gland, showing localisation of iodine.
E.g. tomographic image of a single anatomical level of the brain using 18F-labelled glucose.
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Gamma spectroscopy
• Radiation interaction in scintillator produces light (may be in visible range)
• Quantification of output requires light amplification and detection device(s)
• This is accomplished with the: Photocathode Photomultiplier tube
• Both components are placed together as one unit optically coupled to the scintillator
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880.P20 Winter 2006 Richard Kass
Photoelectric Effect absorbed by material, electron ejected
Compton Scatteringe-→e- “elastic scattering”
Pair Production→e+e- creates anti-matter
Basic Physics Processes in a Sodium Iodide (NaI) Calorimeter
e- e- e- e+
hv < 0.05 MeV 0.05 < hv < 10 MeV hv > 10 MeV -ray must have E>2me
The amount of light given off by NaI is proportional to the amount energy absorbed. The light yield is ~ 1 photon per 25 eV deposited in NaI, max=415 nm, decay time ~250nsec
NaI
radiation length of NaI ~2.5 cmbut only useful for E > few MeV
NaI is often used to measure the energy low gamma rays
Attenuation of the gamma rays is energy dependent
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Scintillation detector
Gamma rayScintillationevent
Reflector housingFluor crystal NaI (Tl)
Photocathode
Photoelectrons
DynodesPhotomultiplier tube
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Major components of PM Tube
• Photocathode material• Dynodes
electrodes which eject additional electrons after being struck by an electron
Multiple dynodes result in 106 or more signal enhancement
• Collector accumulates all electrons produced from final dynode
• Resistor collected current passed through resistor to generate
voltage pulse
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Generalized Detection System using a Scintillator
Oscilloscope
Scaler
Multi-ChannelAnalyzer
DiscriminatorAmplifierPre-Amp
HighVoltage
Detector
(Crystal &Photomultiplier)
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Material Density [g/cm3]
Emission Max [nm]
Decay Constant
(1)
Refractive Index (2)
Conversion Efficiency
(3)
Hygro-scopic
NaI(Tl) 3.67 415 0.23 s 1.85 100 yes
CsI(Tl) 4.51 550 0.6/3.4 s 1.79 45 no
CsI(Na) 4.51 420 0.63 s 1.84 85 slightly
CsIundoped 4.51 315 16 ns 1.95 4 - 6 no
CaF2 (Eu) 3.18 435 0.84 s 1.47 50 no
6LiI (Eu) 4.08 470 1.4 s 1.96 35 yes
6Li - glass 2.6 390 - 430 60 ns 1.56 4 - 6 no
CsF 4.64 390 3 - 5 ns 1.48 5 - 7 yes
(1) Effective average decay time For -rays.(2) At the wavelength of the emission maximum.(3) Relative scintillation signal at room temperature for -rays when coupled to a photomultiplier tube with a Bi-Alkalai photocathode.
Commonly Used Scintillators
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Material Density [g/cm3]
Emission Maximum
[nm]
Decay Constant
(1)
Refractive Index (2)
Conversion Efficiency
(3)
Hygroscopic
BaF2 4.88 315 220
0.63 s0.8 ns
1.50 1.54
16 5 no
YAP (Ce) 5.55 350 27 ns 1.94 35 - 40 no
GSO (Ce) 6.71 440 30 - 60 ns 1.85 20 - 25 no
BGO 7.13 480 0.3 s 2.15 15 - 20 no
CdWO4 7.90 470 / 540 20 / 5 s 2.3 25 - 30 no
Plastics 1.03 375 - 600 1 - 3 s 1.58 25 - 30 no
(1) Effective agerage decay time For -rays.(2) At the wavelength of the emission maximum.(3) Relative scintillation signal at room temperature for -rays when coupled to a photomultiplier tube with a Bi-Alkalai photocathode.
Commonly Used Scintillators
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Coincidence helps!
Coincidence Unit
Scaler
Multi-channelAnalyzer
Detector
Timing
Timing
Amplification
Detector
Source
Amplification
Gate
After Tsoulfanidis, 1995
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Inner BGO ball at G.A.S.P.
ACACSS
BGO BGO BALBALLL
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Projectile Fragmentation Reactions
hotspot
Excited pre-fragment
Finalfragment
projectile
target
Energy (velocity) of beam > Fermi velocity inside nucleus ~30 MeV/uCan ‘shear off’ different combinations of protons and neutrons.Large variety of exotic nuclear species created, all at forward angleswith ~beam velocity. Some of these final fragments can get trapped in isomeric states.
Problem 1: Isotopic identification. Problem 2: Isomeric identification.
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Recoil – Decay –Tagging (RDT) method
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Nucleonic matter
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Hadronic Properties of GeV Photon
Vector-Meson Dominance Model
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Energy loss by Bremsstrahlung (charge particles)
Effect plays a role only for e± and ultra-relativistic µ (>1000 GeV)
Ec(e-) in Cu(Z=29) = 20 MeV, Ec(µ) in Cu ≈ 1 TeV.muons in multi-GeV range can traverse thick layers of dense matter.
Bremsstrahlung
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Laser-Electron-PhotonS facility
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LEPS Facilities Worldwide
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Laser-Electron-PhotonS facility
b) Laser hutch
a) Storage Ring
c) Experimental hutch
Compton -ray
Laser light
3.3 GeV electron Recoil electron
Tagging counter
Collision
Energy spectrum of
BCS photons
Bremsstrahlung
Backward-Compton scattering
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Linearly Polarized Photon
• Backward Compton scattering with UV laser light• Intensity (typ.) : 2.5 * 106 cps• Tagging region : 1.5 GeV< E < 2.4 GeV• Linear polarization : 95 % at 2.4 GeV
E (Tagger) (GeV) E (GeV)
Cou
nts
Line
ar p
olar
izat
ion
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Photon Flux
Laser and electron
Laser &Wavelength
Output Power
Repetition Rate
Pulse length
Electron Current & Energy
Photon Flux & Emax
SPring-8 Paladin 355 nm
8W 80MHz 5ps 100mA8 GeV
700 KHz2.5 GeV
TPS AVAI
266 nm3W 100KHz 25ns 300mA
3.3 GeV1.2 MHz0.6 GeV
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Super Photon Ring 8 GeV (SPring-8)
Harima Science Garden City
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SPring-8 Beam-Lines
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Synchrotron Radiation
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Ar ion laser (MLUV,CW 5.5W)
Polarizationrotator
Focusing lens
Laser System
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e Collision in Storage Ring
Tagging counter
Bending magnet
Straight section
e’
Lasere- (8GeV)
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Experimental Hutch
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LEPS Detector System
1m
TOF wall
MWDC 2
MWDC 3
MWDC 1
Dipole Magnet (0.7 T) Start counter
Silicon VertexDetector
AerogelCherenkov(n=1.03)
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nKKKn
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Elementary Observables
• Momentum• Time-of-Flight• Energy Loss• Particle Identification• Invariant Mass Reconstruction
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Momentum Measurements
• Definition Newtonian Mechanics
Special Relativity
• But how does one measure “p”?
mvp
mvp
21
1
cv
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Momentum Measurements Technique
• Use a spectrometer with a constant magnetic field B.
• Charged particles passing through this field with a velocity “v” are deflected by the Lorentz force.
• Because the Lorentz force is perpendicular to both the B field and the velocity, it acts as centripetal force “Fc”.
• One finds
BvqFM
RmvFc
2
qBRmvp
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Momentum Measurements Technique
• Knowledge of B (magnetic field) and R (bending radius) needed to get “p”
• B is determined by the construction/operation of the spectrometer.
• “R” must be measured for each particle.
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Bending Magnet in Spectrometer
12 sinsin
/
/ dzBce
eqp yxz
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Typical parameters: L=5~8 mm, d=2mm, wire=20m.
Secondary coordinate: Crossed wire planes; Charge division (resistive wires); Segmented cathode plane.
Address of fired wire(s) give one dimensional information.
d= 2mm(x)~600m
Multi Wire Proportional Chamber (MWPC)G.Charpak 1968 ,nobel prize 1992
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Electric field E
BL
T vB
E
T 0
1 2 2
Drift Chambers
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Target, Upstream Spectrometer, Dipole Magnet
LH2 Target (50 mm long)
Cherenkov Detector
SSDDrift Chamber
Start Counter
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Dipole Magnet and Drift Chambers
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tcL
cLt
Combine TOF with p (momentum measurement)
12
22
00 L
tcpmmp
Time-of-Flight (TOF) Measurements
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Fast detectors : plastic scintillator
plastic scintillator,→generation→transmission of scintillation light→detection photomultiplier tube (expensive)
Organic Scintillator (plastics or liquid solutions)
Up to 10000 photons per MeVLow Z; ρ~1gr/cm3Doped, large choice of emission wavelength;ns decay times.Tracking, TOF, trigger, veto counters,sampling calorimeters.
Example: BC-408Rise time 0.9nsDecay time 2.1 nsWavelength length of Max. Emission 408nmRatio H:C 1.104
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Time-of-Flight Wall
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Particle Identification by TOF
Mass(GeV)
Mom
entu
m (G
eV)
K/ separation (positive charge)
K++
Mass/Charge (GeV)
Eve
nts
Reconstructed mass
d
p
K+
K-
+-
TOFlv
pvm ,
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More Complex Observables
• Invariant Mass Reconstruction• Identification of decay vertices
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Invariant Mass Reconstruction
• In special relativity, the energy and momenta of particles are related as follow
• This relation holds for one or many particles. In particular for 2 particles, it can be used to determine the mass of parent particle that decayed into two daughter particles.
42222 cmcpE
Pp1p
2p
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Invariant Mass Reconstruction (cont’d)
• Invariant Mass
• Invariant Mass of two particles
• After simple algebra
22242 cpEcm PPP
221
221
42 cppEEcmP
cos2 22121
422
421
42 cppEEcmcmcmP
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Signal of K+K-
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Finding V0sproton
pion
Primary vertex
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(1115) p+- Reconstruction
Requiring decay vertex (p-) outside target
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Laser Nuclear Physics
ulis2007.celia.u-bordeaux1.fr/telechargement/Wednesday_AM/ULIS07_JG.ppt
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Achievable Laser Intensity
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Historical background About 20 years ago (1988), Boyer et al. Discuss
ed the possibility of inducing nuclear transitions using a laser
Discussion between K. Ledingham (Glasgow Univ.) and J. Magill (ITU) on the possibility of inducing 238U(,f)
First successful experiment at VULCAN, RAL (UK) in 2000, followed by NOVA, LLNL(USA)
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Lasers entering nuclear science ...
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bbbbbbbbbbbbb
Nuclear Reactions Triggered by LasersJETI chamber
PW VULCAN target chamber
30 TW LOA laser
UHI10 target chamber at SLIC
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targ
et
The cascade process of energy transfer from the laser pulse to the radiations
• Primary processes are due to the action of the laser EM field on a plasma
• Fast electrons initiate secondary processes
TW laserpulse plasma
plasma
fast e-
1010 K
protons
ions
gamma rays
mono energetic gamma rays
positrons (anti matter)
fast neutrons
>1018 W/cm2>1018 W/cm2
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Bremsstrahlung applications
• Multi-MeV electrons are stopped in thick high Z material
• They radiate typical bremsstrahlung rays (few 10 MeV)
• production of medical isotopes through transmutation
• studies of alternative research paths to classical reactor-induced reaction for transmutation purposes
• measurement of nuclear data
• diagnostic tools for plasma physic experiments
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1018 1019 1020 1021 1022 1023 1024
1
10
100
1000
Jena
Recent experiemntal data PIC simulation (Esirkepov) Zagar et al. Extrapolation curve
Vulcan
Extrapolation curve
Max
imum
Pro
ton
Ener
gy (M
eV)
Laser Intensity × Wavelength Squared (Wm2/cm2)
Laser proton production
Maximum p+ energy is a function of I2
Emax = a(I2)
For I2 > 1019 :a ~ 4 or 3 x 10-9 MeV = 0.5
Mendonca, Spencer, 2000
Average proton energy is approximately 5 to 10 times smaller.
Higher efficiency: 10 % to 20% achievable (even 50 %)
High-intensity, ultra-fast laser pulse: 1020 W/cm2, λ ≈ 1 μm
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Proton Beam Applications• Fast proton radiography (ns pulses)• Proton induced fission (p,f) measurement of
new cross sections on highly radioactive actinides
• Spallation related studies (Mc Kenna et al.) • Neutron source via (p,xn) reactions (Zagar et a
l.) • ITU project of H-loaded Pd film to optimize
yield and energy distribution of emitted protons
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Other laser-driven ion beams ?
High-Intensity Laser Heavy Ion Acceleration
Radioactive ion beams Stable ion beams
Applications
Limits of nuclear stability“search for super heavies”
Production of radio pharmaceutical
Transmutation Heavy Ions for Space Propulsion
Actinide Nuclear Chemistry
High-Intensity Laser Heavy Ion Acceleration
Radioactive ion beams Stable ion beams
Applications
Limits of nuclear stability“search for super heavies”
Production of radio pharmaceutical
Transmutation Heavy Ions for Space Propulsion
Actinide Nuclear Chemistry
2,0x1019 4,0x1019 6,0x1019 8,0x1019 1,0x10200,1
1
10
C2+
Pb46+
D+ (gas jet)
C6+Al
C4+
C5+
F7+C6+
O
Al13+
Ene
rgy/
nucl
eon
(MeV
)
Laser Intensity (Wcm-2m2)
proton Emax scales as (I2)1/2
McKenna PRL 91
Zepf PRL 90
Pb36+
C3+
Clark PRL 85
C4+C5+
C3+ Hegelich PRL 89
Fritzler PRL 89
• Both radioactive and stable ion beams could be studied
40 MeV 16O ions,
120 MeV 35Cl ions,
500 MeV 208Pb ions
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Heavy ion acceleration & applications
laser
focusing primary target:ion production, selection
and acceleration
ions
vacuum 10-4 mbar
Be sec. target holderand window
products
sec.
targ
et
He atmosphere
laser
focusing primary target:ion production, selection
and acceleration
ions
vacuum 10-4 mbar
Be sec. target holderand window
products
sec.
targ
et
He atmosphere
Be sample holder
accelerator
ion beam ions
vacuum 10-6 mbar
Be window
N2 cooling
products
targ
et
He atmosphere
Be sample holder
accelerator
ion beam ions
vacuum 10-6 mbar
Be window
N2 cooling
products
targ
et
He atmosphere
Comparison of two experimental designs for production and detection of super-heavy elements.
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Laser induced neutron sources
Big Stationary Neutron Sources Flux [neutrons/cm2s] Traditional Reactor from 107 to 1013 High Flux Research Reactor up to 1015 Accelerator Driven Spallation up to 1014 Compact and Portable Neutron Sources Typical Source Strength
[neutrons/s] Radioactive Neutron Sources 105 to 107 Spontaneous Fission Sources around 1010 Portable Neutron Generators 108 to 1010 Lasers on Solid Targets Reaction(s)
Used Measured Source Strength [neutrons/shot]
Laser Energy [J/shot]
Lancaster 7Li(p,n)7Be 2×108 sr-1 69 Yang natZn(p,xn)Ga ≈ 1010 230 Yang 7Li(p,n)7Be 5×1010 230 Zagar natPb(p,xn)Bi 2×109 400
0 5 10 15 20 25 30 35104
105
106
107
108
109
10 20 30 40
109
1010
1011
1012 measured
Boltzmann fit (kT = 5 MeV)
Pro
tons
(1/M
eV)
Energy (MeV)
235U fission spectrum
Neu
trons
(1/M
eV)
Energy (MeV)
2x109 neutrons
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Laser Generated Neutron Sources
Some General Properties• Compact Table-Top Sources (!)• Fast Neutrons – Broad Spectrum• Forward Directed Beams• Pulsed Operation • Very Short Pulse Durations (!)• High Repetition Rates• Useful Source Strengths
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Conclusions and perspectives• Giant pulse single shot and high repetition rate tabletop lase
r have demonstrated their abilities to produced beam of electron and ions
• This research field is developing fast with fast development of high intensity laser
• Lasers do offer a new approach to studying material behavior under neutral and charge particle irradiation without resource to reactors or accelerators
• Currently laser light can directly accelerate electrons to relativistic speeds, and can consequently accelerate protons and other ions. In near future lasers will be able to accelerate protons to relativistic speeds directly
• New table-top radiation sources will become available• We have shown possible applications of laser accelerated e
lectrons, protons, gammas, neutrons• One can expect that these systems can be put to use as str
ong, and possibly compact sources, for nuclear applications.
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END