August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity...

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June 23, 2022 Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation

Transcript of August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity...

Page 1: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

April 19, 2023 Snowmass Workshop

IP Instrumentation

Wolfgang Lohmann, DESY

Measurement of:

•Luminosity (precise and fast)

•Energy

•Polarisation

Page 2: August 2005Snowmass 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

Page 3: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 4: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

410 0.2L

bmtilt mradL

Beam Tilt

Beam Size

No effect

Page 5: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

)]}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

Page 6: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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)

Page 7: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Decouple sensor framefrom absorber frame

Sensor carriers

Absorber carriers

Concept for the Mechanical Frame

Page 8: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Fast Lumi Measurement and Beam Diagnostics

Use Electrons from Rad. Bhabha events

Page 9: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Trajectories of off momentum electrons in the first dublett

Energy and spatial distributions

Fast Lumi Measurement and Beam Diagnostics

Needs a spectrometer

there

Page 10: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Fast Lumi Measurement and Beam Diagnostics

Page 11: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

• 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

Page 12: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 13: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 14: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Beam Parameter Determination with BeamCal

Page 15: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Beam Parameter Determination with BeamCal

Page 16: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 17: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Heavy crystalsW-Diamond sandwich

sensorSpace for electronics

Technologies for the BeamCal:

•Radiation Hard

•Fast

•Compact

Page 18: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 19: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 20: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 21: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Linearity Studies with High Intensities

(PS fast beam extraction)105 particles/10 ns

Response to mip

Diamond Sensor Performance

Page 22: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Upstream momentum spectrometer

Page 23: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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!

Page 24: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Energy Measurement

Downstream SR spectrometerEnergy spectrum

After bunch crossing

Goals: •peak position,•width, •tail

Page 25: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Downstream SR spectrometer

Page 26: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

Downstream SR spectrometer

Page 27: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

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

Page 28: August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.

The needs from Detector and Machine side are different. Lets find solutions