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IBM Research 10/26/2011 © 2011 IBM Corporation On the Calibration of Alpha Sciences Proportional Counters Michael Gordon ([email protected]) Ken Rodbell IBM Research 1101 Kitchawan Road Yorktown Heights, NY 10598

On the Calibration of Alpha Sciences Proportional …ewh.ieee.org/soc/cpmt/presentations/cpmt1110w-4.pdf · – Semiconductor labs ... 0 0.25 0.5 0.75 1 1.25 1.5 1.75 2 Energy (MeV)

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IBM Research

10/26/2011 © 2011 IBM Corporation

On the Calibration of Alpha Sciences Proportional Counters

Michael Gordon ([email protected])

Ken Rodbell

IBM Research1101 Kitchawan RoadYorktown Heights, NY 10598

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation2 10/26/2011

Outline

How is the discriminator set on Alpha Sciences counter and what is thealpha-particle energy associated with the setting? What is the impact ofcutting out the low energy alphas from a sample?

– Introduction

– Background

– Overview of the Alpha Sciences proportional counters

– Our low-energy alpha-particle source

– Results

– Conclusion

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation3 10/26/2011

Introduction

We review a technique for determining the alpha-particle energy associated with a discriminator setting.

We have a low energy “thick” alpha-particle source that was developed for this work.

The alpha particles from this source stop in the gas within the active volume of the detector (important for association between pulse-height analysis and alpha-particle energy).

We compared the count rate of the source vs discriminator setting in the proportional counter, and the count rate of the same source with a silicon surface barrier detector to obtain an energy scale.

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation4 10/26/2011

Background

Many labs have Alpha Sciences proportional counters– Material labs– Semiconductor labs

Recently, several labs participated in a “round-robin” study of both low and ultra-low emissivity samples, “Multicenter comparison of alpha particle measurements and methods typical of semiconductor processing”* – Very few constraints were placed on the measurement

• No sample preparation or measurement protocol• Samples were in many pieces that could be tiled to account for different sizes of the

tray/active area of the counter– There was a ~ 2X difference between the largest and smallest sample

emissivity measured– It was proposed that this difference could be due to the discriminator settings

on the individual detectors• Most people “assume” that the discriminators are set to 1 MeV

* http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=5784521

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation5 10/26/2011

Cutaway section of an old Alpha Sciences counter

cathode plane

anode wires

6 mm

6 mmcathode

sample tray

anode

Cross section of counter

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation6 10/26/2011

0

0.05

0.1

0.15

0.2

0.25

0 1 2 3 4 5 6 7 8 9 10

Energy (MeV)

dE/d

X (M

eV/m

m)

0

24

48

72

96

120

Ran

ge (m

m)

SRIM simulations of alpha-particles in Ar gas

36.2 mm1.43”

104.8 mm4.25”

The counter gas used is Ar/CH4

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation7 10/26/2011

SRIM simulations of alpha-particles in Ar gas

0

0.05

0.1

0.15

0.2

0.25

0 0.25 0.5 0.75 1 1.25 1.5 1.75 2

Energy (MeV)

dE/d

X (M

eV/m

m)

0

4

8

12

16

20

Ran

ge (m

m)

~1.1 MeV α-particles have a 6 mm rangehigher-energy alpha particle will not stop in the detector volume

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation8 10/26/2011

The low-energy α-sourceWe need a low-energy α-source (so that the α’s stop in the active volume in the counter)We made an alpha-particle source from natural Samarium since it’s one of the lowest energy naturally-occurring α-particle emitterSm has 3 naturally-occurring α-emitting radioactive isotopes, – only 147Sm is important, due to the shorter ½ life compared to 148Sm, or 149Sm

0.01311.27E151.93148Sm

13.8

15

Abundance (%)

>1E16 (stable?)

1.07149Sm

8501.06E112.25147Sm

Specific activity

(α/sec-g)

½-life (years)

α-energy (MeV)

Sm Isotope

http://www.nndc.bnl.gov/chart/Chart of the Nuclides, GE, 13th ed.

)/()/(

(sec)2

2/1 molgAmolatomsNx

TLnSA =

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation9 10/26/2011

Table of natural alpha-particle emitters and their energies

Source- unknown, yellowed sheet in my lab

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation10 10/26/2011

0.1

1

10

100

0 1 2 3 4 5

Energy (MeV)

Cou

nts/

hr/

chan

nel

Energy spectrum from Sm source, in vacuum

measured spectrum

noisedifference

110310-sm-1

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation11 10/26/2011

1

10

100

1000

10000

0 2 4 6 8 10

Energy (MeV)

Cou

nts/

hr/

chan

nel

Energy spectrum from 232Th source, in vacuum

measured spectrum

β’s, noise

difference

110218-232th-1

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation12 10/26/2011

Alpha Sciences counter with Ortec discrete electronics

amp discrim. CAMACcounter

+HV

Charge-sensitivepreamp

Anode

CathodeSample/ tray

Using off-the-shelf electronics allows for easy adjustment and repair

MCA

Applied VoltagePul

se A

mpl

itude

Ion saturation

Propregion

Geigerregion

Applied Bias

1 MeV

2 MeV

From Knoll

Analytical formfor cylindrical geo.b

a)/ln(

)(abr

VrE =

For r=a, V=800V, E~106 V/m

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation13 10/26/2011

Pulse-height spectrum from sources in the Alpha Sciences counter

0.01

0.1

1

10

100

1000

0 200 400 600 800 1000

Channel

Cou

nts/

hr/

chan

nel

0.01

0.1

1

10

100

1000

0 200 400 600 800 1000

Channel

Cou

nts/

hr/

chan

nel

Ultra-low activity sample

GC9-111024

A2110311-20.01

0.1

1

10

100

1000

0 200 400 600 800 1000

Channel

Cou

nts/

hr/

chan

nel

A2110311-1

Sm source 232Th source

noise

noise, β’s

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation14 10/26/2011

Energy spectrum of Sm source, energy loss from sample through cathode

0.01

0.1

1

10

100

0 0.5 1 1.5 2 2.5 3

Energy (MeV)

Cpu

nts/

hr/

chan

nel

0.01

0.1

1

10

100

0 0.5 1 1.5 2 2.5 3

Energy (MeV)

Cpu

nts/

hr/

chan

nel

0.01

0.1

1

10

100

0 0.5 1 1.5 2 2.5 3

Energy (MeV)

Cpu

nts/

hr/

chan

nel

vacuum

air

air + mylar

2 mm gap

2.5 mm gap

3 mm gap

gap

~1 MeV energy lossin air and mylar- beforeα’s reach active area

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation15 10/26/2011

Energy spectrum of 232Th source, energy loss from sample through cathode

0.1

1

10

100

1000

10000

100000

0 2 4 6 8 10

Energy (MeV)

Cou

nts/

hr/

chan

nel 2.5 mm gap, in vacuum

2.5 mm gap, air + mylar

Passage of the alphas in the gap and mylar causes reduction in maximum energy and in the flux

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation16 10/26/2011

Results

Integrate the measured alpha particle energy spectrum from the samarium source, using the silicon detector, above a given threshold (eg E>0.25 MeV, E>0.5 MeV, E>0.75 MeV and E>1.0 MeV)

Repeat integration for each of the source-to-detector gaps

Plot the resulting integrated count rate vs energy

Integrate the count rate for the Alpha Sciences counter above a given ADC voltage threshold (eg V>0.5V, V>0.9V, V>1.5V,V >2.0V) using the discrete electronics

We can correlate the pulse height with energy- given the MCA spectrum from the Alpha Sciences counter, and the maximum energy in the alpha particle energy spectra

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation17 10/26/2011

Results

0

50

100

150

200

250

300

350

400

450

0 0.5 1 1.5 2 2.5 3

Energy (MeV)

Cou

nts/

hr/

chan

nel

2 0

0

50

100

150

200

250

300

350

400

450

0 0.5 1 1.5 2 2.5 3

Energy (MeV)

Cou

nts/

hr/

chan

nel

2 0

0

50

100

150

200

250

300

350

400

450

0 0.5 1 1.5 2 2.5 3

Energy (MeV)

Cou

nts/

hr/

chan

nel

2 0

Si detector data

gas counter data2 mm gap

2.5 mm gap

3 mm gap

O.50.9

1.5

2.02.5

data from Si detector “fits” thegas counter data with a ~2.5 mm gap

0 count rate with this source is ~1-1.3 MeV

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation18 10/26/2011

Response of Alpha Sciences counter, original electronics

55000

60000

65000

70000

75000

80000

0 0.05 0.1 0.15 0.2 0.25 0.3 0.35

Discriminator setting (V)

coun

ts/ h

r

Th source

A1111019

0

50

100

150

200

250

300

0 0.05 0.1 0.15 0.2 0.25 0.3 0.35

Discriminator setting (V)

coun

ts/ h

r

A1111018

Sm source

Zero count rate corresponds to a total energy loss of 2.25 MeV

Raising the discriminator level lowersthe detection efficiency (lowers the count rate) for a thick source

The slope of count rate vs discriminator setting, and the discriminatorsetting where the count rate goes to zero, will depend on the amplifier gain

IBM Research & IBM Systems and Technology Group

© 2010 IBM Corporation19 10/26/2011

Conclusion

– We have shown the energy spectrum from a low-energy Sm α-particle source.

– There is an appreciable energy-loss of low-energy α’s before they reach the active gas volume in the Alpha Sciences counters.

– While the discriminator can be set higher to reduce the background count rate, it cuts out the detection of low-energy α’s.

– The efficiency of detection in these counters is energy-dependent.

– What energy α’s are really important for samples that we measure?

– What is the α-particle energy associated with the discriminator setting on your Alpha Sciences counters?