Diamond (Radiation) Detectors Are Forever! Harris …kagan/talks_info/IWORID04/...Diamond...

39
Diamond (Radiation) Detectors Are Forever! Harris Kagan Ohio State University IWORID 2004 July 26-29, 2004 - Glasgow, UK Outline of the Talk Introduction to Diamond Recent Results Applications Summary IWORID 2004 July 26-29, 2004 - Glasgow, UK Diamond (Radiation) Detectors Are Forever! (page 1) Harris Kagan Ohio State University

Transcript of Diamond (Radiation) Detectors Are Forever! Harris …kagan/talks_info/IWORID04/...Diamond...

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Diamond (Radiation) Detectors Are Forever!

Harris KaganOhio State University

IWORID 2004July 26-29, 2004 - Glasgow, UK

Outline of the Talk

• Introduction to Diamond

• Recent Results

• Applications

• Summary

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 1) Harris Kagan

Ohio State University

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Introduction

Motivation: Tracking Devices Close to Interaction Region of Experiments

Use at the LHC/SLHC (or similar environments e.g. BaBar, Belle):→ Inner tracking layers must provide high precision tracking (to tag b, t, Higgs, . . . )

→ Inner tracking layers must survive! → what does one do?

→ Annual replacement of inner layers perhaps?

Look for a Material with Certain Properties:• Radiation hardness (no frequent replacements)

• Low dielectric constant → low capacitance

• Low leakage current → low readout noise

• Room temperature operation, Fast signal collection time → no cooling

Material Presented Here:• Polycrystalline Chemical Vapor Deposition (pCVD) Diamond

• Single Crystal Chemical Vapor Deposition (scCVD) Diamond

On Behalf of RD42:• Reference → http://rd42.web.cern.ch/RD42

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 2) Harris Kagan

Ohio State University

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Introduction

Comparison of Various Materials

Property Diamond 4H-SiC Si

Band Gap [eV] 5.5 3.3 1.12Breakdown field [V/cm] 107 4×106 3×105

Resistivity [Ω-cm] > 1011 1011 2.3×105

Intrinsic Carrier Density [cm−3] < 103 1.5×1010

Electron Mobility [cm2V−1s−1] 1800 800 1350Hole Mobility [cm2V−1s−1] 1200 115 480Saturation Velocity [km/s] 220 200 82

Mass Density [g cm−3] 3.52 3.21 2.33Atomic Charge 6 14/6 14Dielectric Constant 5.7 9.7 11.9Displacement Energy [eV/atom] 43 25 13-20

Energy to create e-h pair [eV] 13 8.4 3.6Radiation Length [cm] 12.2 8.7 9.4Spec. Ionization Loss [MeV/cm] 4.69 4.28 3.21Ave. Signal Created/100 µm [e] 3600 5100 8900Ave. Signal Created/0.1% X0 [e] 4400 4400 8400

→ Low dielectric constant - low capacitance→ Large bandgap - low leakage current→ Large energy to create an eh pair - small signal

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Diamond (Radiation) Detectors Are Forever! (page 3) Harris Kagan

Ohio State University

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Diamond

Diamond Growth:

Micro-Wave Reactor Schematic Edge View of pCVD diamond

(Courtesy of Element Six)

• Diamonds are “synthesized” from a plasma

• The diamond “copies” the substrate

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 4) Harris Kagan

Ohio State University

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Diamond

Characterization of Diamond:

Signal formation

e-h Creation

Charged Particle

Electrodes

Diamond

Vbias

Amplifier

• Q=dtQ0 where d = collection distance = distance e-h pair move apart

• d=(µeτe + µhτh)E

• d=µEτ

with µ = µe + µh

and τ = µeτe+µhτh

µe+µh

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 5) Harris Kagan

Ohio State University

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Diamond

Diamond Properties:

Signal formation

0

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1

1.2

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1.6

1.8

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10-4

10-3

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10-1

1 10 102

Signal versus applied electric field

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0 0 .2 0 .4 0 .6 0 .8 1 1 .20

2000

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Col

lect

ion

Dis

tanc

e ( µ

m)

Electric Field (V/µm)

Mean C

harge (e)

• Contacts on both sides - structures from µm to cm

• Contacts typically: Cr/Au or Ti/Au or Ti/W → non-carbide formers

• Polycrystalline CVD diamond typically “pumps” by a factor of 1.5-1.8

• Usually operate at 1V/µm → drift velocity saturated

• Test Procedure: dot → strip → pixel on same diamond!

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Diamond (Radiation) Detectors Are Forever! (page 6) Harris Kagan

Ohio State University

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Diamond

Recent polycrystalline CVD (pCVD) diamond.

(Courtesy of Element Six)

Left: Enhanced surface of pCVD diamondRight: Recent pCVD wafer ready for test - Dots are 1 cm apart

Wafers can be grown >12 cm diameter, >2 mm thickness.

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 7) Harris Kagan

Ohio State University

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Diamond

In 2000 RD42 entered into a Research Program with Element Six to increasethe charge collected from pCVD diamond.

Research Program Diamond Measured with a 90Sr Source:

• System Gain = 124 e/mV• QMP = 7600e (62mV)• Mean Charge = 9800e (79mV)

• Source data well separated from 0• Collection Distance now 275µm• Most Probable Charge now ≈ 8000e• 99% of PH distribution now above3000e

• FWHM/MP ≈ 0.95 — Si has ≈ 0.5• This diamond available in large sizes

The Research program worked!

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 8) Harris Kagan

Ohio State University

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Diamond

History of Diamond Progress

*

*Charge Collection in DeBeers CVD Diamond

0

100

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1994 1995 1996 1997 1998 1999 2000 2001 2002

RD42 Goal

Time (year)

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ion

Dis

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ron

s)

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 9) Harris Kagan

Ohio State University

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Diamond - Tracking Studies

Diamond Tracking Planes:

Photo of Two Diamond Tracking Planes PH Distribution on each Strip

channel number [ ]0 20 40 60 80 100 120

sig

nal

ch

arg

e, t

wo

str

ips

[e]

-5000

0

5000

10000

15000

20000

25000CDS-90

mean values on channels

Diamond Tracker CDS-90, Signal Charge on Strips

• Use same electronics as Silicon• Uniform signals on all strips → new metalisation• Pedestal separated from “0” on all strips• 99% of entries above 2000 e• Mean signal charge ∼ 8640 e → new metalisation• MP signal charge ∼ 6500 e

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 10) Harris Kagan

Ohio State University

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Diamond Radiation Hardness Studies with Trackers

Proton Irradiation Studies with Trackers:

Signal to Noise

2 strip transparent signal to single strip noise [ ]0 50 100 150 200 250

entr

ies/

bin

[1/

100]

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400

500

600

700

800before irradiation

mean 57, most prob. 41FWHM 54

after 1 E15 protons/cm2

mean 49, most prob. 35FWHM 41

Diamond CDS-69 at 0.9 V/µm

after 2.2 E 15 protons/cm2

and re-metalizationmean 47, most prob. 35FWHM 36

Signal from Irradiated Diamond Tracker

• Dark current decreases with fluence• S/N decreases at 2× 1015/cm2

• Resolution improves at 2× 1015/cm2

Resolution

entr

ies/

2µm

[ ]

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700

800

Residual Distributions, Proton Irradiated Diamond

Diamond CDS-69

before irradiationσ = 11.5 µm

2-strip center ofgravity method

0

200

400

600

800

1000

CDS-69

after 1E15 p/cm2

σ = 9.1 µm

residual, uh-ut, [µm]-100 -80 -60 -40 -20 0 20 40 60 80 100

0

200

400

600

800

1000

1200

CDS-69

after 2.2 E 15 p/cm2

and re-metalization

σ = 7.4 µm

Irradiation to 1016 protons/cm2 presently underway!

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 11) Harris Kagan

Ohio State University

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Diamond Radiation Hardness Studies with Trackers

Pion Irradiation Studies with Trackers:

Signal to Noise

2-strip transparent signal to single strip noise [ ]0 50 100 150 200 250

entr

ies

0

100

200

300

400

500

600

700

800

CDS-38 at 0.6 V/µmbefore irradiation

mean 66most prob. 44FWHM 58

cm2⁄after 2.9 E 15 π

mean 28

and re-metalization

most prob. 21FWHM 27

Signal Distributions from Diamond Tracker

Resolution

entr

ies/

2µm

0

50

100

150

200

250CDS-38before irradiation

σ = 13.7 µm

2-strip center of gravity

method

Residual Distributions in Diamond Tracker

residual, uh-ut [µm]-100 -80 -60 -40 -20 0 20 40 60 80 100

entr

ies/

2µm

0

50

100

150

200

250

300CDS-38

cm2⁄after 2.9 E 15 π

σ = 10.6 µm

and re-metalization

2-strip center of gravitymethod

• Dark current decreases with fluence

• 50% loss of S/N at 2.9× 1015/cm2

• Resolution improves 25% at 2.9× 1015/cm2

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 12) Harris Kagan

Ohio State University

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Diamond - Tracking Studies

Radiation Hard Diamond Tracking Modules:

20 40 60 80 100 120 140 160 1800

500

1000

1500

2000

2500

htempNent = 37904 Mean = 50.2RMS = 16.38

max abs(tim-346)<2 && sig<170 htempNent = 37904 Mean = 50.2RMS = 16.38

• Large (2cm × 4cm) Module constructed with new metalisation

• Fully radiation hard SCTA128 electronics → 25ns peaking time

• Tested in a 90Sr → ready for beam test and irradiation

• Charge distribution cleanly separated from the noise tail → S/N > 8/1

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 13) Harris Kagan

Ohio State University

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New Type of CVD Diamond: Single Crystal CVD Diamond

Could we make a CVD diamond with improved characteristics?

• Remove the grain boundaries, defects, charge trapping etc.• Lower operating voltage.• Eliminate pumping.

This is single crystal CVD (scCVD) diamond: [Isberg et al., Science 297 (2002) 1670].

CD135 - Both Sides - Pumped (Sr-90 source)

0 10000 20000 30000 40000 50000

Signal Size (Electrons)

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Num

ber

per

400

Ele

ctro

ns

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 14) Harris Kagan

Ohio State University

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Single Crystal CVD Diamond

HV and Pumping Characteristics

HV (Volts)0 100 200 300 400 500

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llect

ion

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ce (

mm

)

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071415b OSU HV Curve

Time (min)1 10 10

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um

)

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071415 Pump-up Curve (HV=500V)

• High quality scCVD diamond collects all the charge at E=0.2V/µ!

• High quality scCVD diamond does not pump!

But...

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 15) Harris Kagan

Ohio State University

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Single Crystal CVD Diamond

But for Other Diamonds

HV (Volts)0 100 200 300 400 500

HV (Volts)0 100 200 300 400 500

Co

llect

ion

Dis

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ce (

mm

)

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CD134 OSU HV Curve

HV (Volts)0 100 200 300 400 500

HV (Volts)0 100 200 300 400 500

Co

llect

ion

Dis

tan

ce (

mm

)

0

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CD135 OSU HV Curve

HV (Volts)0 100 200 300 400 500 600 700 800 900

HV (Volts)0 100 200 300 400 500 600 700 800 900

Co

llect

ion

Dis

tan

ce (

mm

)

0

0.05

0.1

0.15

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CD136 OSU HV Curve

HV (Volts)0 100 200 300 400 500

Co

llect

ion

Dis

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ce (

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)

0

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CD137 OSU HV Curve

Not that easy to make!

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 16) Harris Kagan

Ohio State University

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Single Crystal CVD Diamond

Largest scCVD Diamond:

• Began with 4mm × 4mm• Today 7mm × 7mm• Well on our way to 8mm × 8mm sizes!

Impurities, Defects and Dislocations: Photo-Luminescence Measurements

Left Image: High purity, no nitrogen, no dislocations.Middle Image: Contains nitrogen - NV centre, 575 nm PL.Right Image: Contains dislocations, broad band blue PL.

May be able to unravel the compexity of the CVD process!

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 17) Harris Kagan

Ohio State University

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Single Crystal CVD Diamond

Charge Collection Properties: Transient Current Measurements (TCT)

• Measure charge carrier properties separately for electron and holes• Use α-source (Am241) to inject charge

- penetration ≈ 14 µm (thickness of diamonds ≈ 470 µm)

- use positive and negative applied voltage

• Amplify ionization current

Extracted parameters: Transit time, velocity, lifetime, space charge, pulse shape, charge.

Preliminary Results: saturated velocity ve = 96 km/s, vh = 141 km/slifetimes ≈ 34 ns >> transit time (charge trapping not the issue)

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 18) Harris Kagan

Ohio State University

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Applications

CVD Diamond Used or Planned for Use in Several Fields

• High Energy Physics

• Heavy Ion Beam Diagnostics

• Sychrotron Radiation Monitoring

• Neutron and α Detection

Applications Discussed Here

• Pixel DetectorsATLAS, CMS

• Beam MonitoringBaBar

Belle

ATLAS

CMS

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 19) Harris Kagan

Ohio State University

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Diamond Pixel Detectors

ATLAS FE/I Pixels (Al)

• Atlas pixel pitch 50µm × 400µm• Over Metalisation: Al• Lead-tin solder bumping at IZM in Berlin

CMS Pixels (Ti-W)

• CMS pixel pitch 125µm × 125µm• Metalization: Ti/W• Indium bumping at UC Davis

→ Bump bonding yield ≈ 100 % for both ATLAS and CMS devices

New radiation hard chips produced this year.

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 20) Harris Kagan

Ohio State University

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Diamond Pixel Detectors

Results from an ATLAS pixel detector

1 Chip Assembly

2x8 Chip Assembly (Module)

1 Chip IV Curve

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 21) Harris Kagan

Ohio State University

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Diamond Pixel Detectors

Results from an ATLAS pixel detector

1 Chip Source Test (Am241) 1 Chip Source Test (Cd109)

Americium 241 deposits ≈ 4600eCadmium 109 deposits ≈ 1600e

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 22) Harris Kagan

Ohio State University

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Diamond Pixel Detectors

Results from an ATLAS pixel detector

1 Chip Beam Test (x-Resolution)

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800

1000

-0.2 -0.1 0 0.1 0.2

Resy/mm

1 Chip Beam Test (y-Resolution)

0

50

100

150

200

250

300

350

400

-0.4 -0.2 0 0.2 0.4

Resy/mm

Pitch is 50µm × 400µmSpatial Resolution ≈ pitch/

√12

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 23) Harris Kagan

Ohio State University

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Diamond Pixel Detectors

Results from a CMS pixel detector

Efficiency Resolution

• Results with 200µm collection distance diamondEfficiency ∼ 94%Spatial resolution ∼ 31µm for 125µm pitch

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 24) Harris Kagan

Ohio State University

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Diamond Pixel Detectors

Results from a CMS pixel detector

Efficiency vs Pixel

• Inefficient pixels due to bump bonding and/or electronics - shown in pulser tests

• Excellent correlation between beam telescope and pixel tracker data!

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 25) Harris Kagan

Ohio State University

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Radiation Monitoring - New Application - BaBar, Belle, ATLAS, CMS

Motivation:

→ Radiation monitoring crucial for Si operation/abort system of BaBar, Belle, LHC

→ Abort beams on large current spikes

→ Measure calibrated daily and integrated dose

Style:

• DC current or Slow Readout• Requires low leakage current• Requires small erratic dark currents• Allows simple measuring scheme

• Examples: BaBar, Belle, CMS

• Single Particle Counting• Requires fast readout (GHz range)• Requires low noise• Allows timing correlations

• Example: ATLAS

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 26) Harris Kagan

Ohio State University

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Radiation Monitoring

The BaBar/Belle Diamond Radiation Monitor Prototypes:

• Package must be small to fit in allocated space• Package must be robust

Schematic View

Diamond

Au Contact

In SolderHV Insulation

Ground BraidKapton Insulation

Copper Shield

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 27) Harris Kagan

Ohio State University

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Radiation Monitoring - BaBar

The BaBar/Belle Diamond Radiation Monitor Prototypes:

→ BaBar/Belle presently use silicon PIN diodes, leakage current increases 2nA/krad

→ After 100fb−1 signal≈10nA, noise≈ 1-2µA

→ Large effort to keep working, BaBar PIN diodes will not last past 2005

Photo of BaBar Prototype Devices Photo of Installed BaBar Device

BaBar device inside the silicon vertex detector.

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 28) Harris Kagan

Ohio State University

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Radiation Monitoring - Belle

The BaBar/Belle Diamond Radiation Monitor Prototypes:

Photo of Belle Prototype Device Photo of Installed Belle Device

Belle device just outside the silicon vertex detector.

IWORID 2004

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Diamond (Radiation) Detectors Are Forever! (page 29) Harris Kagan

Ohio State University

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Radiation Monitoring

Results on Calibration in BaBar:

• In BaBar during injection relative to silicon diodes: 5.9mrad/nC (Feb)• In BaBar during injection relative to silicon diodes: 5.8mrad/nC (Apr)• Correlation coefficient unchanged over several months

Diamond Current/nA0 5 10 15 20 25 30 35 40 45 50

Dio

de

Rat

e/m

Rad

/s

0

50

100

150

200

250

300

0.2552 ±p0 = -4.897

0.01263 ±p1 = 5.916

February

BE:MID rate vs BE diamond current 0.2552 ±p0 = -4.897

0.01263 ±p1 = 5.916

Diamond Current/nA0 5 10 15 20 25 30 35 40 45 50

Dio

de

Rat

e/m

Rad

/s0

50

100

150

200

250

300

0.2533 ±p0 = -7.085

0.01236 ±p1 = 5.801

April

BE:MID rate vs BE diamond current 0.2533 ±p0 = -7.085

0.01236 ±p1 = 5.801

Calibration repeatable over many months

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 30) Harris Kagan

Ohio State University

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Radiation Monitoring

Data Taking in BaBar:

0

5

10

15

20

25

0 2500 5000 7500 10000 12500 15000 17500 20000 225000

200

400

600

800

1000

1200

1400

1600

1800

20000 2500 5000 7500 10000 12500 15000 17500 20000 22500

BE diamond current

BE:MID diode signal current (Sig 11)

LER current

Time/seconds

Dia

mon

d/D

iode

cur

rent

/nA

Time/secondsH

ER

cur

rent

/mA

Fast Abort Soft Abort

System operating for 18 months in BaBar and works well!

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 31) Harris Kagan

Ohio State University

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Radiation Monitoring

Leakage Current in BaBar

• Diamonds have received 250kRad 60Co plus 750kRad while installed

• No observed change in leakage current (<0.1nA) or fluctuations (30pA)• Data directly from BaBar SVTRAD system• Electronic noise (≈ 0.5nA) substracted off

0

0.02

0.04

0.06

0.08

0.1

0.12

20 40 60 80 100 120 140February 5, No Beams Time (s)

Cur

rent

(nA

)

April 17, No Beams Time (s)

Cur

rent

(nA

)

0

0.02

0.04

0.06

0.08

0.1

0.12

20 40 60 80 100 120 140

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 32) Harris Kagan

Ohio State University

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Radiation Monitoring

Discovery of Erratic Dark Currents

It is observed the diamond current increases as the magnetic field goes off.

This happens every time the field goes off in BaBar

The Eratic Dark Currents have been reproduced in the laboratory!

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 33) Harris Kagan

Ohio State University

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Radiation Monitoring

Discovery of Erratic Dark Currents

Eratic Dark Currents go away every time the magnetic field is turned on!

Origin is still a mystery

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 34) Harris Kagan

Ohio State University

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Radiation Monitoring

Very Fast Time Scale (ns) in BaBar

• Use a fast amplifier to look at PIN-diode and diamond signals• Trigger on the PIN-diode signal• Look at fast spikes: red = diamond, black = PIN-diode

Diamond is fast enough (< 20 ns) → now used in BaBar abort systemInstallation of full diamond system possible in summer 2005

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 35) Harris Kagan

Ohio State University

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Radiation Monitoring

The CMS Diamond Radiation Monitor Program:

• Diamond activity has begun!

• Test beam emulating beam accident - unsynchronised beam abort - 1012 protons lostin 260 ns in CMS

• Worst case 100x unsynchronised beam abort over several turns - protection requiresearly detection

• Possible location in the CMS detector:

Monitors

Simulation of a Beam Accident in CMS

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 36) Harris Kagan

Ohio State University

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Radiation Monitoring

The ATLAS Diamond Radiation Monitor Program:

• Diamond activity has begun!

• Time of flight measurement to distinguish collisions from background

• Located behind pixel detector forward disks in pixel support tube

• Possible ATLAS scenario:

Beam Condition Monitor in ATLAS

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 37) Harris Kagan

Ohio State University

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Summary

CVD Diamond as Radiation Tolerant Detectors

• High Quality pCVD diamond (ccd up to 275 µm) are readily available in large sizes

MP signal ≈ 8000 e

99% of charge distribution above 3000 e

Attained S/N=60/1 with 2µs shaping time; 8/1 at 25ns

• Radiation Tests show tolerance up to 2× 1015/cm2

Using trackers allows a correlation between S/N and Resolution

Dark current decreases with fluence Some loss of S/N with fluence Resolution improves with fluence

• Present pCVD diamonds should surpass performance of silicon at around 1015p/cm2

scCVD Diamonds May Overcome the Limitation of pCVD Material

• Full signal collection at E<<1V/µm

• Long charge lifetime• Very little trapping- uniform detector

Many Applications Benefit from use of Diamond

• Beam Monitoring Now - BaBar, Belle• Strip or Pixel detectors for the future

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 38) Harris Kagan

Ohio State University

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Future Plans for RD42

• Charge Collection

Continue research program to improve pCVD material:

collection distance → 300µm (Q = 10, 800e)

→ improved uniformity

→ identification of trapping centers

Begin research program on scCVD diamond

• Radiation Hardness of Diamond Trackers and Pixel Detectors

Continue tracker irradiations this year, add pixel irradiations

With Protons:

→ 5× 1015/cm2 → Now

With Pions:

→ 5× 1015/cm2

• Beam Tests with Diamond Trackers and Pixel Detectors

→ trackers with intermediate strips, SCTA128 electronics

→ pixel detectors with ATLAS and CMS radhard electronics now available!

→ construct the first full ATLAS diamond pixel module

• Material Research

→ Florence, OSU, Paris, Rome

IWORID 2004

July 26-29, 2004 - Glasgow, UK

Diamond (Radiation) Detectors Are Forever! (page 39) Harris Kagan

Ohio State University