August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity...
-
Upload
kristopher-craig -
Category
Documents
-
view
220 -
download
4
Transcript of August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity...
April 19, 2023 Snowmass Workshop
IP Instrumentation
Wolfgang Lohmann, DESY
Measurement of:
•Luminosity (precise and fast)
•Energy
•Polarisation
Precise Luminosity Measurement
e e e e
LumCal bgr
Bhabha
N NL
IP
VTX
FTD
300 cmBeamCal
L* = 4m
Accuracy (from Physics) O(<10-3)
4 4
4 4
( : / 3 10 ( ) 5.4 10 ( ))
( : / 6 10 ( ) 6.1 10 ( ))
OPAL L L stat theo
ALEPH L L stat theo
Gauge process: Bhabha ScatteringDevice: LumiCal 26 < < 82 mrad
Beampipe
Inner Radius of Cal.: < 4 μm
Distance between Cals.: < 100 μm
Radial beam position: < 0.6 mm
Requirements on Alignment
and mechanical Precision(MC simulations, BHLUMI)
LumiCal
LumiCalIP
Requirements on the Mechanical Design
< 4 μm
< 0.6 mm
410 0.2L
bmtilt mradL
Beam Tilt
Beam Size
No effect
)]}ln()([,0max{T
ibeami E
EEconstW
i
ii
W
WXX
Constant value))(_( radmean genrec
))(( rad
value of the constant
0.11e-3 rad
0.13e-3 rad
30 layers 15 rings
20rings
10ring
s
4 layers
15 layers
11 layers
10rings
Performance Simulations for e+e- e+e-()Event selection: acceptance, energy balance, azimuthal and angular symmetry.
Simulation: Bhwide(Bhabha)+CIRCE(Beamstrahlung)+beamspread
•More in the talks by Halina Abramowicz
20 mrad crossing angle
Beamstrahlung pair background
using serpentine field
0.E+00
1.E+09
2.E+09
3.E+09
4.E+09
5.E+09
6.E+09
8 9 10 11 12 13 14 15 16
R min (cm)
Nm
ber
of
Bh
abh
a ev
ets
per
yea
r
0
500
1000
1500
2000
2500
3000
3500
Bac
kgro
un
d (
GeV
)
Events per year
Background (GeV)
250 GeV
Number of Bhabha events as a function of the innerRadius of LumiCal
Background from beamstrahlung
A design for 20 mrad crossing angle will be done(needs time)
Decouple sensor framefrom absorber frame
Sensor carriers
Absorber carriers
Concept for the Mechanical Frame
Fast Lumi Measurement and Beam Diagnostics
Use Electrons from Rad. Bhabha events
Trajectories of off momentum electrons in the first dublett
Energy and spatial distributions
Fast Lumi Measurement and Beam Diagnostics
Needs a spectrometer
there
Fast Lumi Measurement and Beam Diagnostics
• 15000 e+e- per BX 10 – 20 TeV
(10 MGy per year)
• e+e- Pairs from Beamstrahlung are deflected into the BeamCal
GeV
• direct Photons for < 200 rad
Zero (or 2 mrad) crossing
angle
20 mradCrossing
angle
Beam Parameter Determination with BeamCal
total energyfirst radial momentthrust valueangular spreadL/R, U/D F/B asymmetries
Observables
QuantityNominal Value
Precision
x 553 nm 1.2 nm
y 5.0 nm 0.1 nm
z 300 m 4.3 m
y 0 0.4 nm
Beam Parameter Determination with BeamCal
zero or 2 mradCrossing angle
√s = 500 GeV
QuantityNominal Value
Precision
x 553 nm 4.8nm
y 5.0 nm 0.1 nm
z 300 m 11.5 m
y 0 2.0nm
Beam Parameter Determination with BeamCal
PRELIMINARY!
20 mrad crossing angle
total energyfirst radial momentthrust valueangular spreadL/R, U/D F/B asymmetries
Also simultaneous determination of several beam parameter is feasible, but: Correlations!Analysis in preparation
Observables
Beam Parameter Determination with BeamCal
Beam Parameter Determination with BeamCal
nominal setting(550 nm x 5 nm)
>100mIP
L/R, U/D F/B asymmetriesof energy in the angulartails
QuantityNominal Value
Precision
x 553 nm 4.2 nm
z 300 m 7.5 m
y 0 0.2 nm
Heavy gas ionisation Calorimeter
and with PhotoCalPhotons from Beamstrahlung
Heavy crystalsW-Diamond sandwich
sensorSpace for electronics
Technologies for the BeamCal:
•Radiation Hard
•Fast
•Compact
Detection of High Energy Electrons and Photons(Detector Hermeticity) √s = 500 GeVSingle Electrons of 50, 100 and 250 GeV, detection efficiency as a function of R (‘high background region’)(talk by V. Drugakov and P. Bambade)
Detection efficiency as a function of the pad-size (Talk by A. Elagin)
Message: Electrons can be
detected!
Red – high BGblue – low BG
Includes seismic motions, Delay of Beam Feedback System, Lumi
Optimisation etc.(G. White)
Efficiency to identify energetic electrons and photons(E > 200 GeV)
Fake rate
√s = 500 GeV
Realistic beam simulation
•Detection of High Energy Electrons and Photons
Sensor prototyping, Diamonds
ADC
Diamond (+ PA)
Scint.+PMT&
signal gate
May,August/2004 test beams
CERN PS Hadron beam – 3,5 GeV
2 operation modes:
Slow extraction ~105-106 / s
fast extraction ~105-107 / ~10ns (Wide range intensities)
Diamond samples (CVD):
- Freiburg
- GPI (Moscow)
- Element6
Pm1&2
Pads
Linearity Studies with High Intensities
(PS fast beam extraction)105 particles/10 ns
Response to mip
Diamond Sensor Performance
Upstream momentum spectrometer
ESA Test Beam Plans for 2005/2006
2x1010 electrons per bunch @ 28.5 GeV (ILC buch charge and length)Compare different measurments (this spectrometer,A- line BPMs, Synchrotron spectrometer)Accuracy goal: < 100 ppmProof of principle!
Energy Measurement
Downstream SR spectrometerEnergy spectrum
After bunch crossing
Goals: •peak position,•width, •tail
Downstream SR spectrometer
Downstream SR spectrometer
Upstream polarimeter
Polarimetry
250 GeV
25 GeV
45.59 GeV
K Moffeit 4 Apr 05
2 mradenergystripe
2 mradenergystripeBVX1
z=59.69 m
3 mradenergystripe
3 mradenergystripe
Shielding
Energy Chicane
Polarimeter Chicane
10 cm
10 meters
SynchrotronStripe Detector
SynchrotronStripe Detector
CerenkovDetector
Wiggler
Low Field
25.1 GeV
BVX2z=61.99 m
BLEXz=64.29 m
BLEXz=66.89 m
WEX1z=65.59 m
BVX3z=68.19 m
BVX4z=70.49 m
BVX5z=72.79 m
BVX6z=75.09 m
BLEXz=77.39 m
BLEXz=79.99 m
WEX1z=78.69 m
BVX7z=81.29 m
BPM BPM
BVX8z=83.59 m
BVX9z=100.59 m
BVY1z=120.59 m
BVY2z=132.59 m
BVY3z=152.59 m
Compton IP
17.8cm
QFX4z=156.59 m
35.7 GeV 12.0cm
Synchrotron StripeDetector z=143.69 m
Document on polarimetry design in Feb 2006
+ Downstream polarimeter
The needs from Detector and Machine side are different. Lets find solutions