luminosity measurement at the international linear collider

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Luminosity Measurement at the International Linear Collider Iftach Sadeh Tel Aviv University ( On behalf of the FCAL collaboration ) December 28 th 2008 http://alzt.tau.ac.il/ ~sadeh/ [email protected]

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Luminosity Measurement at the International Linear Collider. Iftach Sadeh Tel Aviv University ( On behalf of the FCAL collaboration ). December 28 th 2008. http://alzt.tau.ac.il/~sadeh/ [email protected]. Overview. 2. The International Linear Collider (ILC). - PowerPoint PPT Presentation

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Page 1: Luminosity Measurement at the International Linear Collider

Luminosity Measurement at the International Linear Collider

Iftach Sadeh

Tel Aviv University

( On behalf of the FCAL collaboration )

December 28th 2008http://alzt.tau.ac.il/~sadeh/

[email protected]

Page 2: Luminosity Measurement at the International Linear Collider

Overview

1.The International Linear Collider (ILC).

2.Luminosity measurement at the ILC.

3.Design and performance of the luminosity calorimeter (LumiCal).

4.A clustering algorithm for LumiCal.

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Page 3: Luminosity Measurement at the International Linear Collider

The ILC & The ILD detector3

Page 4: Luminosity Measurement at the International Linear Collider

LumiCal Performance requirements

1. Required precision is:

2. Measure luminosity by counting the number of Bhabha events (NB) in a well defined angular and energetic range:

3 9

3 6

3 6

10 , GigaZ (hadronic Z decays) 10 / year

~10 , 10 / year

~10 , 10 / year

L

LL

e e W WLL

e e q qL

3

1Bd

d

max

min

, rec genB B

B B gen

N NN NLL

L N N

RIGH LEFTTΔθ - θθLEFTθ

RIGHTθ

4

Page 5: Luminosity Measurement at the International Linear Collider

LumiCal Design parameters

3. Layers:

Number of layers - 30

Tungsten Thickness - 3.5 mm

Silicon Thickness - 0.3 mm

Elec. Space - 0.1 mm

Support Thickness - 0.6 mm

1. Placement:

2270 mm from the IP

Inner Radius - 80 mm

Outer Radius - 190 mm

2. Segmentation:

48 azimuthal & 64 radial divisions:

Azimuthal Cell Size - 131 mrad

Radial Cell Size - 0.8 mrad

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Page 6: Luminosity Measurement at the International Linear Collider

ares

σ(θ)

Intrinsic parameters of LumiCal

Relative energy resolution:

Position reconstruction (polar angle):

6

4

min

21.5 10

L

L

Page 7: Luminosity Measurement at the International Linear Collider

Topology of Bhabha scattering Bhabha scattering with √s = 500 GeV

θ Φ

Energy

Separation between photons and leptons, as a function of the energy of the low-energy-particle.

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Page 8: Luminosity Measurement at the International Linear Collider

Clustering Algorithm

Phase I:Near-neighbor clustering in a single layer.

Phase II:Cluster-merging in a single layer.

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Phase III:Global (multi-layer) clustering.

Page 9: Luminosity Measurement at the International Linear Collider

Overlap of multiple showers

Profile of the energy of a single 250 GeV shower.

Profile of the energy of two showers (230 and 20 GeV) separated by one Moliere radius (indicated by the circles).

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Page 10: Luminosity Measurement at the International Linear Collider

Clustering - Results (event-by-event)

Event-by-event comparison of the energy and position of showers (GEN) and clusters (REC) as a function of EGen.

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(θGen - θRec)/ θGen(ΦGen - ΦRec)/ ΦGen

(EGen - ERec)/ EGen

Page 11: Luminosity Measurement at the International Linear Collider

Summary1. Intrinsic properties of LumiCal:

Energy resolution: ares ≈ 0.21 √GeV.

Relative error in the luminosity measurement:ΔL/L = e(rec) e(stat) = 1.5 · 10-4 4 · 10-5 (at 500 fb-1).

- The reconstruction error, e(rec), is due to the error in reconstruction of the polar angle.

- The statistical error, e(stat), is due to fluctuations in the expected number of Bhabha events, ΔNB/NB, for an integrated luminosity of 500 fb-1.

- The theoretical uncertainty is expected to be ~ 2 · 10-4.

2. Partial event reconstruction (counting of radiative photons):

Merging-cuts need to be made on the minimal energy of a cluster and on the separation between any pair of clusters.

The algorithm performs with high efficiency and purity. The number of radiative photons within a well defined phase-space may be counted with an acceptable uncertainty.

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Page 12: Luminosity Measurement at the International Linear Collider

AuxiliarySlides

Page 13: Luminosity Measurement at the International Linear Collider

The ILC & The LDC detector13

Page 14: Luminosity Measurement at the International Linear Collider

Physics Background Four-fermion processes are the main background, dominated by two-photon

events (bottom right diagram).

The cuts reduce the background to the level of 10-4

ffeeeeFour-fermion processes

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Page 15: Luminosity Measurement at the International Linear Collider

Selection of Bhabha events

Right side signal

Left

sid

e si

gnal

deg5

rad310

LRLR RERE ,min1.0

Simulation distribution

Distribution after acceptance and energy balance selection

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RIGH LEFTTΔθ - θθLEFTθ

RIGHTθ

Page 16: Luminosity Measurement at the International Linear Collider

Detector signal

Distribution of the deposited energy spectrum of a MIP (using 250 GeV muons):MPV of distribution = 89 keV ~ 3.9 fC.

Distributions of the charge in a single cell for 250 GeV electron showers.

The influence of digitization on the energy resolution and on the polar bias.

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ares

σ(θ)

Page 17: Luminosity Measurement at the International Linear Collider

ares

Digitization

σ(θ)

Δθ

Page 18: Luminosity Measurement at the International Linear Collider

Thickness of the tungsten layers (dlayer)

σ(θ)Δθ

ares

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Page 19: Luminosity Measurement at the International Linear Collider

Number of radial divisions

σ(θ) Δθ

min

2

L

L

-1

5

500GeV

1.23nb

500 fb

4 10

s

L

N

N

Dependence of the polar resolution, bias and subsequent error in the luminosity measurement on the angular cell-size, lθ.

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Page 20: Luminosity Measurement at the International Linear Collider

Inner and outer radii

Beamstrahlung spectrum on the face of LumiCal (14 mrad crossing angle): For the antiDID case Rmin must be larger than 7cm.

-1500 fbL

63.2 10 rad

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Page 21: Luminosity Measurement at the International Linear Collider

MIP (muon) Detection in LumiCal Many physics studies demand the ability to detect muons (or the lack thereof) in

the Forward Region.

Example: Discrimination between super-symmetry (SUSY) and the universal extra dimensions (UED) theories may be done by measuring the smuon-pair production process. The observable in the figure, θμ, denotes the scattering angle of the two final state muons.

“Contrasting Supersymmetry and Universal Extra Dimensions at Colliders” – M. Battaglia et al. (http://arxiv.org/pdf/hep-ph/0507284)

1 1 1 1

2UED:

~ 1 coscos

e e

d

d

0 01 1

2SUSY:

~ 1 coscos

e e

d

d

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Page 22: Luminosity Measurement at the International Linear Collider

MIP (muon) Detection in LumiCal

Multiple hits for the same radius (non-zero cell size).

After averaging and fitting, an extrapolation to the IP (z = 0) can be made.

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Page 23: Luminosity Measurement at the International Linear Collider

1. High beam-beam field (~kT) results in energy loss in the form of synchrotron radiation (beamstrahlung).

2. Bunches are deformed by electromagnetic attraction: each beam acting as a focusing lens on the other.

Change in the final state polar angle due to deflection by the opposite bunch, as a function of the production polar angle.

Beam-Beam effects at the ILC

Since the beamstrahlung emissions occur asymmetrically between e+ and e-, the acolinearity is increased resulting in a bias in the counting rate.

“Impact of beam-beam effects on precision luminosity measurements at the ILC”

– C. Rimbault et al. (http://www.iop.org/EJ/abstract/1748-0221/2/09/P09001/)

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Page 24: Luminosity Measurement at the International Linear Collider

Effective layer-radius, reff(l) & Moliere Radius, RM

Dependence of the layer-radius, r(l), on the layer number, l.

RM

r(l)

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Distribution of the Moliere radius, RM.

Page 25: Luminosity Measurement at the International Linear Collider

Clustering - Algorithm

Phase I:Near-neighbor clustering in a single layer.

Phase II:Cluster-merging in a single layer.

Longitudinal shower shape.

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Page 26: Luminosity Measurement at the International Linear Collider

Clustering Algorithm26

Phase III:Global (multi-layer) clustering.

Page 27: Luminosity Measurement at the International Linear Collider

Clustering - Energy density corrections

Event-by-event comparison of the energy of showers (GEN) and clusters (REC).

Before After

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Page 28: Luminosity Measurement at the International Linear Collider

Clustering - Results28

(2→1): Two showers were merged into one cluster.

(1→2): One shower was split into two clusters.

The Moliere radius is RM (= 14mm), dpair is the distance between a pair of showers, and Elow is the energy of the low-energy shower.

Page 29: Luminosity Measurement at the International Linear Collider

Clustering - Geometry dependence29

96 div

48 div

24 div

Page 30: Luminosity Measurement at the International Linear Collider

Clustering - Results (measurable distributions)

Energyhigh

θhigh θlow

Energylow

Δθhigh,low Energy and polar angle (θ) of high and low-energy clusters/showers.

Difference in θ between the high and low-energy clusters/showers.

Merging-cuts:Elow ≥ 20 GeV , dpair ≥ RM

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Page 31: Luminosity Measurement at the International Linear Collider

Clustering - Results (relative errors) Dependence on the merging-cuts of the errors in counting the number of

single showers which were reconstructed as two clusters (N1→2), and the number of showers pairs which were reconstructed as single clusters, (N2→1).

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