Calorimetry

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Physics of Electromagnetic
Calorimeters based on Crystal
Scintillators
Tetiana Hrynova
SLAC
Graduate Student Seminar Series
21April 2004
Basics
• What is Calorimeter?
– Device to measure the energy deposited by an
incoming particle
• How does it work?
– Incoming particle looses energy by interactions in the
calorimeter material
– Calorimeter material proportionally converts energy
into detectable signal (scintillation or Čerenkov light,
ionization charge)
– Photodetector converts light into electrical signal
which is proportional to the energy deposited
Tetiana Hrynova
Physics of EM calorimeters
2
Types Of Calorimeters
Air, Ice,
Water, Quartz,
Lead Glass…
Sampling
ICECUBE
CERENKOV
Homogineous
P
A
M
E
L
A
Solid State
(Si/W)
Gas
IONIZATION
H1
Noble Liquid
(Ar, Kr, Xe )
BOREXINO
SCINTILLATION
ICARUS
Scintillator
ZEUS
Advantages of
Crystal EM
Calorimeters









Good Energy Resolution
Good Detection Efficiency
Compact Mechanical Structure
Uniform Hermetic Coverage
Fine Granularity Over a Large Solid Angle
Clean Electron and Photon Identification
Radiation Damage
Readout Speed
Cost
Tetiana Hrynova
Physics of EM calorimeters
4
SM Physics in Precision ECAL
Charmonium System Observed
Through Inclusive Photons
Charmed Meson in Z Decay
Crystal Ball
Tetiana Hrynova
Physics of EM calorimeters
From R.Y.5 Zhu
New Physics in Precision ECAL
J. Gunion, in Snowmass
SUSY Breaking with Gravitino
CMS
Tetiana Hrynova
Physics of EM calorimeters
Simulations
6
Physics at BaBar
Need excellent  detection efficiency and resolution from
20 MeV to 4 GeV to study B000, bs, measurement
of R ratio using initial state radiation, etc…
Tetiana Hrynova
Physics of EM calorimeters
7
Outline
• Electromagnetic Interactions
• Principles of Scintillation Counting
• Properties & Applications of Different
Scintillators
• BaBar EMC
– Radiation Dose Monitoring
– Total Light Output
– Uniformity of the Light Output Along the
Length of the crystal
Tetiana Hrynova
Physics of EM calorimeters
8
Electron
Processes
Bremsstrahlung
dominates at
high energies
The critical energy is
the energy at which
the energy lost by
ionization is the same
as the loss by radiation
800MeV
Ec 
Z  1.2
Radiation length is the
mean distance over
which (1-1/e)E0
(63.2%) of energy is
lost due to
bremsstrahlung
Ionization dominates
at low energies
716.4  g  cm 2  A
X0 
Z ( Z  1) ln( 287 / Z )
Photon Processes
The cross-section has a
minimum:MeV photons travel
long before interacting
The mean free path at
high energies (e-folding
distance N(r)=N0e-r/
for the pair production
by a high energy
photon) is: =7X0/9
EM Showers:
From D. Perkins,
Intro to HEP, p368
simple model
• Number of particles: N(t)=2t
• Average energy of a particle: E(t)=E0/2t
• At Shower Maximum E(tmax)=Ec 
tmax=ln(E0/Ec)/ln2, Nmax=exp(tmaxln2)=E0/Ec
• Total Length of Charged Tracks Tch=2/3Ndt=
=2/3et ln2dtet(E)ln2/ln2=2/(3ln2)*E0/EcE0/Ec
tmaxlnE0; NmaxE0; TchE0
• Need MC for more accurate predictions!
Tetiana Hrynova
Physics of EM calorimeters
11
EM Showers MC : Longitudinal Profile
• Energy Deposition
dE
(bt ) a 1 e bt
 E0
dt
( a )
1 E C j 1
a  ln

, b  0.5
2 Ec
2
• Maximum of energy
deposition
E0
a 1
t max 
 ln
Cj
b
Ec
where Ce=-0.5 and C=0.5 and
• Photon showers are longer
b/c of the uncertainty of the
position of the first pairproduction
Plots from J.Tinslay
: 1.0,0.5,
0.1 GeV
e-
 5 GeV
e- on Cu
EM Showers MC : Lateral Profile
• Exponential Profile
• Up to tmax shower radius < X0
• After tmax multiple scattering of electrons
causes size to scale with Moliere radius
X 0 21.2 MeV
Rm 
Ec
• Cylinder of radius 2Rm contains 90% of shower
• Soft photons near the end of the shower may
travel far depending on cross-sections
Tetiana Hrynova
Physics of EM calorimeters
13
Scintillation mechanism
scintillation
Fluorescence(scintillation) –
initial excitation and
de-excitation by emission of
a longer wavelength photon
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Physics of EM calorimeters
14
Scintillation
Detection
• Transparency for
Fluorescent Radiation
• Crystals wrapped in a
reflector to collect as
much light as possible
• Photo-detector:
16.0-17.5 X0
6.1x6.0cm2
4.7x4.7cm2
– Two 2x1cm2 PID diodes
– 85% quantum efficiency
– Operated at 50V
(depletion voltage 70V)
– Shaping time .85ms (2-3
ms optimal)
• Amount of the light
collected depends on
the crystal/photodetector shape
Matching Crystal to Photo-detector
Photodiode
Photodiode requires amplification!
x256: 0-50MeV, x32: 50-400MeV,
x4: 0.4-3.2GeV, x1: 3.2-13.0GeV
Photomultiplier
Photomultiplier does not require
amplification, but has problems
working in magnetic field.
Properties of “Perfect” Scintillation
Material
•
•
•
•
•
•
High Density, High Atomic Number
Transparency for Fluorescent Radiation
Convenient Emission Wavelength
Short Decay Time
High Light Yield
Uniformity of the Light Output along the crystal
length
• High Radiation and Mechanical Hardness
• Ease to manufacture
• Low Cost
Tetiana Hrynova
Physics of EM calorimeters
17
Properties of Crystal Scintillators
Crystal
NaI(Tl)
CsI(Tl)
CsI
BaF2
BGO
PbWO4
LSO(Ce)
GSO(Ce)
Density (g/cm3)
3.67
4.51
4.51
4.89
7.13
8.3
7.40
6.71
Radiation Length (cm)
2.59
1.85
1.85
2.06
1.12
0.9
1.14
1.37
4.8
3.5
3.5
3.4
2.3
2.0
2.3
2.37
41.4
37.0
37.0
29.9
21.8
18
21
22
10k
100k
1M
10M
10M
100M
100M
Molière Radius (cm)
Interaction Length (cm)
Radiation Hardness
Hygroscopicity
Yes
Slight
Slight
No
No
No
No
No
Luminescence b (nm)
(at peak)
410
560
420
310
300
220
480
560
420
420
440
Decay Time b (ns)
230
1300
35
6
630
0.9
300
50
10
40
60
Light Yield b,c (%)
100
45
5.6
2.3
21
2.7
9
0.1
0.6
75
30
d(LY)/dT b (%/ ºC)
~0
0.3
-0.6
-2
~0
-1.6
-1.9
?
?
Crystal
Ball
CLEO
BaBar
BELLE
KTeV
(L*)
(GEM)
L3
CMS
ALICE
BTeV…
-
-
Experiment
a. at peak of emission; b. up/low row: slow/fast component; c. measured by PMT of bi-alkali cathode.
From R.Y. Zhu
Crystals Vendor Map for BaBar
It is very difficult to produce
crystals in numbers required by
HEP experiments (6580 CsI(Tl) for
BaBar, 77k PWO for CMS)
at one place in the time required!
Crismatec
Beijing
Hilger
Kharkov
Shanghai
Tetiana Hrynova
Physics of EM calorimeters
19
Kyropoulos
Growth
Method
Used in Kharkov
crystals and with
modifications in
Crismatec and
Hilger crystals
From SCINT97
p380
Bridgman-Stockbarger Growth
Method
Used for Shanghai and Beijing
CsI(Tl) crystal production
for BaBar. The pictures
shown are actually from CMS
PWO production in
Bogoroditsk, Russia
Tetiana Hrynova
Physics of EM calorimeters
21
Samples of Crystal Scintillators
BGO
CeF
BaF2
CsI
1.5 X0 Cubic
3
PbWO4
Full Size Samples
BaBar CsI(Tl): 16 X0
L3 BGO: 22 X0
CMS PWO(Y): 25 X0
Tetiana Hrynova
Physics of EM calorimeters
From R.Y. Zhu
22
Scintillation Light of 6 Samples
From R.Y. Zhu
Calorimeter Resolution
E
a
c

b ,
E
E
E
d
   
f
E
• Stochastic term(a):
– Shower fluctuations, photoelectron statistics, material in front of
calorimeter
• Constant term(b): detector non-uniformity, calibration uncertainty
• c: electronic noise summed over readout channels within a few
Moliere radii
• Position resolution depends on the effective Moliere radius and the
transverse granularity of the calorimeter
 means summation in quadrature
Tetiana Hrynova
Physics of EM calorimeters
24
L3 BGO Resolution
Contribution
“Radiative”+Intrinsi
c
Temperature
Calibration
Overall
Barrel
0.8%
0.5%
0.5%
1.07%
Endcaps
0.6%
0.5%
0.4%
0.88%
12k BGO
From R.Y. Zhu
CMS PWO Resolution
Beam Test
77k PWO
Crystal
Calorimetry
at High
Energies
Designed Resolution
From R.Y. Zhu
BaBar CsI(Tl) Resolution
Crystal Calorimetry at
Low Energies
M. Kocian, SLAC, CALOR2002
0.03-3 GeV
3-9 GeV, 12h
0.00613 GeV, 1/2h
6580 CsI(Tl)
Good light yield of CsI(Tl)
provides excellent energy
resolution at B factory
energies
Energy Resolution
• Energy resolution for the detection of photons from 0 in the
range from 20 MeV to 4 GeV:
E
(2.30  0.03  0.3)%

 (1.35  0.08  0.2)%
4 E (GeV )
E
• The stochastic term comes from: fluctuations in photon
statistics, electronic noise and beam background
• The constant term arises from non-uniformity in light
collection ( 0.5%), front and rear shower leakage ( 1%)
and uncertainties in calibration (0.25%)
• Systematic errors come from fixing of the shapes for 
energy distributions which are convoluted for the purpose of
0 fit
Tetiana Hrynova
Physics of EM calorimeters
28
EMC Backgrounds
& Rad Damage
10MeV
• Mostly photons <10MeV
• Leads to formation of color
centers which cause
absorption bands in the
front 10-15cm of the crystal
• Caused by impurities
• Results in:
100MeV
 Decrease in the light yield
(LY)
 Non-uniformity of the LY
along the crystal length
(worsens energy resolution)
Tetiana Hrynova
Physics of EM calorimeters
29
Absorption, cm-1
Transmitance,%
Absorption Bands
Exposures: 0, 1, 10, 100, 1000 rad
top to bottom
Transmitance=1-e-kd, where
k is absorption coefficient
d is thickness of sample in cm
OH- absorption band is
located at the maximum of the
scintillation emission
CsI(Tl) absorption
CsI(OH) absorption
CsI(Tl) emission
EMC Calibrarions
• Inter crystal Calibrations
• Shower corrections
Tetiana Hrynova
Physics of EM calorimeters
31
Source Measurement of LY
Typical source spectrum:
Tetiana Hrynova
• Neutron generator
activated fluid circulates on
demand though an array of
thin tubes in front of all
crystals
• 6.13MeV photons from 19F
 16N 16O* 16O
• 16N lifetime is 7 sec
• Resolution of the light
yields is 0.33%
• Measured every 1-2 month
• Individual crystal
calibration!
Physics of EM calorimeters
32
Bhabha calibrations
M. Kocian, CALOR2002
Crystal Response Uniformity
 rays
Uniformity is influenced by:
PMT,
PD

PD
PMT
Back (5%)
Tetiana Hrynova
crystal clarity
 wrapping
 surface finish
 radiation damage
Require less then 0.5%
contribution to E/E for up
to 5 GeV.
Front (2%)
Physics of EM calorimeters
34
Checking
the Uniformity
Gain changes obtained
using the radioactive
source (s) and Bhabha (B)
calibrations: possible
probe of LY uniformity
along crystal length.
Statistical errors are:
• 0.33 % for the source
• 2 % for the Bhabhas
No non-uniformity seen.
Tetiana Hrynova
Physics of EM calorimeters
35
Background Distribution
Occupancy obtained
using random triggers.
LER
HER
• Single Beam Backgrounds
 Lost primary beam particles
 In fwd/bwd direction in
horizontal plane
• Luminosity Backgrounds
 Small angle Bhabhas
 More uniform dose
distribution
Tetiana Hrynova
Physics of EM calorimeters
(plot by S.Robertson)
36
Radiation Monitoring in EMC
•
•
•
•
•
Tetiana Hrynova
Array of 115 RadFETs
Maximum dose seen 1150 Rad
Dose has a rate of 4-12 Rad/fb-1
Dose budget is 10 kRad over BaBar life
Dose map similar to beam bkg distributions
Physics of EM calorimeters
Plots by J. Stelzer
37
Leakage Currents (LC)
• Leakage current is an
average current flowing
though the diode
• Increases with time
because of diode
radiation damage
• Can be used to
calculate the dose
accumulated by EMC
Plot by I. Eschrich
time, s
Ecr
( I beamson  I nobeams )
Dose 

dt
M cr
M cr  LYcr
Tetiana Hrynova
Physics of EM calorimeters
38
Dose accumulated by EMC
RadFETs
Leakage Currents
• Differ by scaling factor, shape similar
• EC sees ~30% more dose then measured by RadFETs
Tetiana Hrynova
Physics of EM calorimeters
39
Crystal LY change by vendor
Source of difference – different growth methods results in :
• Different distribution of Tl along the length of the crystal
• Different distribution of impurities along the length of the crystal
Tetiana Hrynova
Physics of EM calorimeters
40
Comparison to expected dose
rates in CMS
BaBar
Tetiana Hrynova
Dose Rates in Gy(100Rad)/h
expected in the regions of CMS
ECAL at lumi 1034 cm-2s-1
Physics of EM calorimeters
41
Other Uses for Scintillating Crystals
• Medicine – PET/CT scanners,
Gamma-cameras
• Geophysics – search for minerals
• Nuclear Physics / Ecology – radiation
control, sample testing
• Technology – baggage
/cargo scanning
Tetiana Hrynova
Physics of EM calorimeters
42
Future Calorimeters
Si/W for
PAMELA
MINOS, Plastic Scintillator
ATLAS LAr EMC
Tetiana Hrynova
Physics of EM calorimeters
43
Cosmic Ray Air Shower Detection
p, γ,ν interaction
Using
Atmosphere
as a Calorimeter
Air Fluorescence
Air Fluorescence Detector
(Fly’s Eye, HiRes, EUSO/OWL)
Air Cherenkov
Particle Shower
Ground Array (AGASA, Auger..)
1~2km
Tetiana
FromHrynova
Katsushi
Physics
of EM calorimeters
Arisaka, Calor
2002
44
And much, much more…
• EMC Calibrations see talk by M.Kocian
http://3w.hep.caltech.edu/calor02/abstract/Presentation/cryst
al/kocian.pdf
• EMC electronics see talk by I. Eschrich
http://3w.hep.caltech.edu/calor02/abstract/Presentation/electro
nics/eschrich.pdf
• PDG2004
• BaBar NIM paper
• R. Wigmans, Calorimetry, Oxford, 2000
• J. Birks, The Theory and Practice of Scintillation Counting,
Pergamon Press, 1964
• Proceedings of Calorimetry in HEP (even years), SCINT
(odd years), Techniques and Concepts of HEP
Tetiana Hrynova
Physics of EM calorimeters
45
Energy Transfer Losses
Scintillation Quantum Efficiency(): =SQ,
where
 is conversion efficiency determined by
crystal lattice and not sensitive to radiation
Q is determined by type of luminescence
center
• the light output is ~ QCa where Ca is
activator concentration and it might
change
S is energy transfer to emission center
• it is known that CsI(CO3)
crystals with concentrations
of CO32- two orders of
magnitude less than Tl+ ions
give competitive light output,
thus they capture some part
of the charge carriers
Longitudinal Shower Profile
Z
Lead
82
Iron
26
Aluminium 13
• As Z increases, the shower maximum shifts to greater
depth
• A Z increases, the shower profile decay more slowly
beyond shower maximum
Tetiana Hrynova
Physics of EM calorimeters
47
Light Output of BaBar CsI(Tl) Crystals
241Am
Counts
spectrum
produced by
crystal+PMT+
EMC readout
system
• 241Am source: 60keV 
• 3.6eV needed to creat e-h pair in
Si (16667 e-)
• Corresponds to 86.72ADC counts
• Using 6.13MeV source determine
that 57.8keV/ADC count is
deposited (2 diodes averaged!)
• This gives 3322
photoelectrons/MeV with PD
0.85ms readout time
• Compare to 7300
photoelectrons/MeV with PMT
2.0ms readout time
ADC counts
Tetiana Hrynova
Plot from M. Kocian
Physics of EM calorimeters
48
Dose Accumulated by EMC
Dose calculated using LC shows:
~45% of EMC dose is
accumulated during injection.
Tetiana Hrynova
Physics of EM calorimeters
49
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