energy loss of protons in silicon strip detectors for computed
TRANSCRIPT
UNIVERSITY of CALIFORNIA
SANTA CRUZ
ENERGY LOSS OF PROTONS IN SILICON STRIP DETECTORSFOR COMPUTED TOMOGRAPHY
A thesis submitted in partial satisfaction of therequirements for the degree of
BACHELOR OF SCIENCE
in
PHYSICS
by
Carlin Fuerst
June 2010
The thesis of Carlin Fuerst is approved by:
Professor Hartmut SadrozinskiTechnical Advisor
Professor David P. BelangerThesis Advisor
Professor David P. BelangerChair, Department of Physics
Copyright c© by
Carlin Fuerst
2010
Abstract
Energy Loss of Protons in Silicon Strip Detectors for Computed Tomography
by
Carlin Fuerst
The purpose of this paper is to analyze the effectiveness of a prototype instrument with applications
in medical imaging. Radiobiologists at Loma Linda University Medical Center currently employ
X-ray computed tomography as an imaging solution for their proton therapy patients. Researchers
at the Santa Cruz Institute for Particle Physics have been commissioned to design and implement
a prototype imaging solution that uses protons from the treatment beam instead of X-rays. This
paper analyzes the energy loss of the particles as they pass through the tracking detectors before they
reach the calorimeter which will aid engineers in creating a final product. Our preliminary results
indicate that the GLAST 2000 detectors and electronics show us higher than expected calculated
energy absorption values, specifically differences of 121%, 129%, and 87% from the expected values
for 35MeV, 100MeV, and 250MeV beam energies.
iv
Contents
List of Figures v
List of Tables vi
Dedication vii
Acknowledgements viii
1 Introduction 11.1 Characteristics of Proton Therapy . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21.2 Description of pCT . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21.3 Proton Energy Loss . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3
2 Analysis 62.1 TOT analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6
2.1.1 Figures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 92.2 Energy loss of protons . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
3 Conclusions 20
Bibliography 21
v
List of Figures
1.1 A comparison of photon and proton energy absorption in tissue. [3] . . . . . . . . . . 31.2 PSTAR stopping power data for Silicon. [7] . . . . . . . . . . . . . . . . . . . . . . . 4
2.1 TOT histograms for all cluster sizes: 250MeV proton beam, 103.5mV threshold, allshaping resistors, internal triggering, ghosts removed . . . . . . . . . . . . . . . . . . 9
2.2 TOT histograms for all cluster sizes: 100MeV proton beam, 103.5mV threshold, allshaping currents, internal triggering, ghosts removed . . . . . . . . . . . . . . . . . . 10
2.3 TOT histograms for all cluster sizes: 35MeV beam energy, 103.5mV threshold, allshaping currents, internal triggering, ghosts removed . . . . . . . . . . . . . . . . . . 11
2.4 TOT histograms for varying cluster sizes: 250MeV beam energy, 103.5mV threshold,280kΩ shaping resistor, internal triggering, ghosts removed . . . . . . . . . . . . . . 12
2.5 TOT histograms for varying cluster sizes: 100MeV beam energy, 103.5mV threshold,280kΩ shaping resistor, internal triggering, ghosts removed . . . . . . . . . . . . . . 13
2.6 TOT histograms for varying cluster sizes: 35MeV beam energy, 103.5mV threshold,280kΩ shaping resistor, internal triggering, ghosts removed . . . . . . . . . . . . . . 14
2.7 Layer 0, 280 kΩ calibration with second order approximation . . . . . . . . . . . . . 152.8 Layer 0, 470kΩ calibration with second order approximation up to 25µs . . . . . . . 172.9 Layer 0, 180kΩ calibration with second order approximation . . . . . . . . . . . . . . 172.10 Layer 1, 280kΩ calibration with second order approximation . . . . . . . . . . . . . . 182.11 A plot of expected energy loss and calculated energy loss for all beam energies and
shaper resistors. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
vi
List of Tables
1.1 Example data for relevant proton energies in Silicon. . . . . . . . . . . . . . . . . . . 5
2.1 Calculations for Energy Loss in Silicon . . . . . . . . . . . . . . . . . . . . . . . . . . 18
vii
To my loving parents,
Peter and Lorrie Fuerst,
who have always been there for me.
viii
Acknowledgements
I would like to thank my friend and colleague Brian Colby without whose patience and clarity the
time until my graduation would extend asymptotically and Ford Hurley for allowing himself to be
muddled by my cryptic coding skills. I would also like to thank my advisor Hartmut Sadrozinski for
putting his trust in my abilities long enough for me to do something worthwhile.
1
1 Introduction
Doctors at Loma Linda University Medical Center (LLUMC) currently employ a proton
accelerator to generate a beam of high-energy protons for the purpose of treating cancerous tumors.
The benefit of this form of radiation therapy is the ability to treat localized, isolated, solid tumors
before they spread to other tissues and to the rest of the body[1]. While the treatment uses protons,
X-ray Computed Axial Tomography (CAT) is currently used to generate three dimensional images
of the patients’ tumors. The drawbacks of this combination of proton treatment and X-ray imaging
are that the instrumentation for both exist in separate rooms due to the size of the apparatus which
requires the patient to be moved around and that the fundamental differences between the ways
in which protons and photons interact with matter may limit the physical insight that we glean
from the images. As a solution, engineers at the Santa Cruz Institute for Particle Physics (SCIPP)
have been commissioned by LLUMC to develop the hardware for a Proton Computed Tomography
(pCT) system that uses protons from the accelerator to image cancer patients. This is currently
being done with Silicon Strip Detectors (SSDs) and custom readout electronics that were originally
designed for the Gamma-ray Large Area Space Telescope (GLAST) aka Fermi for which SCIPP was
a contributing research group. This paper will describe the progress of hardware development and
analysis of the energy loss of protons through the tracking SSDs before they are inevitably measured
by the calorimeter and the implications of this on the eventual imaging solution[2].
2
1.1 Characteristics of Proton Therapy
Using high-energy protons for radiation oncology was first proposed in 1946 and since
then, several hospitals around the world have built proton accelerators for this purpose[1]. In the
accelerator, hydrogen atoms are stripped of their electrons and sent through a vacuum tube within a
pre-accelerator. At this point, the protons have each gained 2MeV in kinetic energy before entering
the synchrotron where they travel around the loop 10 million times per second, gaining energy every
trip from a radio frequency cavity in the loop. By the time the protons leave the accelerator, they
have an energy between 70 and 250MeV. It is the nature of charged particles at these energies to
penetrate matter while depositing a fraction of their energy via the excitation of electrons in the
material. This interaction is described by the Bethe-Bloch formula which gives the mean stopping
power of a material as a function of particle energy. In this model and range of energies, higher
energy particles deposit less energy-per-distance penetrated than lower energy particles. This results
in the particles depositing most of their energy deep inside a material, as opposed to near the surface
as with X-rays, and this energy loss is characterized by what is called a Bragg peak. With a range of
proton energies and a rotating beam aperture, the dose can be localized in a discrete volume within
the patient resulting in a lower amount of collateral healthy tissue damage than X-ray therapy.
1.2 Description of pCT
The system currently in development at SCIPP through collaboration with LLUMC called
pCT will provide doctors with an imaging solution that utilizes protons originally intended for
radiation therapy which would simplify and potentially improve the process of treatment. The
pCT system would contain as few as three main detectors for the purpose of particle tracking: Two
tracking SSDs to record the X and Y positions of incident particles and a CsI calorimeter to measure
the energy of said particles. The position trackers also have the ability to measure charge deposited
in the detector in the form of TOT, or time over threshold, by converting the signal of the charge in
3
Figure 1.1: A comparison of photon and proton energy absorption in tissue. [3]
a strip entering the GTFE (GLAST Tracker Front End chip) into a pseudo-Gaussian via the shaper.
The voltage in the shaper is compared to a threshold voltage via a discriminator and the amount of
time that this voltage is larger than the threshold voltage is the TOT reading[4].
A modified version of the GLAST readout electronics has been developed at SCIPP to take
data with the SSDs on a scale useful to the project and a Data Acquisition (DAQ) system based
on the one developed for the Particle Tracking Silicon Microscope (PTSM)[5] at SCIPP is being
employed to record the data. These images will be used by doctors to locate and measure tumors
for accurate targeting during treatment.
1.3 Proton Energy Loss
The intent of these analyses is to measure the energy loss of protons as they pass through
the SSDs and compare this measurement to theory. The theoretical model which applies in this case
is the Bethe-Bloch equation, Eq. 1.1, which describes the energy loss per unit thickness dE/dx per
4
10
100
1000
0.1 1 10 100 1000
Sto
ppin
g P
ower
(M
eV c
m2 /g
)
Energy (MeV)
Mean Stopping Power of Protons in Silicon
Figure 1.2: PSTAR stopping power data for Silicon. [7]
unit via the ionization of the atoms in a material[6]:
−dE
dx= Kz2 Z
A
1β2
[12
ln2mec
2β2γ2Tmax
I2− β2 − δ
2
](1.1)
In this case, K/A ≈ 0.307MeVg−1cm2 , Z is the atomic number of the absorber, z is the charge
of the incident particle in units of fundamental charge, β is the special relativistic vc , mec2 is ≈
0.510MeV, γ is the Lorentz factor, Tmax is the maximum kinetic energy which can be imparted to
a free electron in a single collision (see below), and I is the mean excitation energy (10eV). Tmax is
described as the following:
Tmax =2mec
2β2γ2
1 + 2γme/M + (me/M)2(1.2)
where M is the incident particle mass (MeV/c2). The National Institute of Standards and Technology
(NIST) provides tables for the stopping powers, within 1 percent, of protons in different materials
which include minor corrections to the Bethe-Bloch equation shown above.
With these data one can determine the total energy deposited within a material using the
5
integral ∆E =∫
dEdx dx or an equivalent small thickness approximation.
Table 1.1: Example data for relevant proton energies in Silicon.
Beam Energy Total Stopping Expected Energy Loss(MeV) Power (MeVcm2/g) in 400µm Si (MeV)3.50×101 1.302×101 1.21×100
1.00×102 5.838×100 5.44×10−1
2.50×102 3.165×100 2.95×10−1
6
2 Analysis
2.1 TOT analysis
At LLUMC The detector board was placed such that the tracking detectors were in the
path of the proton beam. Tests were performed at various energies and readout configurations and
data were collected. First, we see histograms of the TOT measurements from the SSDs for a beam
energy of 250MeV (Fig. 2.1) at a threshold voltage of 103.5mV, internal triggering, and ”ghosting”
events (events for which multiple strips went over threshold that were not adjacent) removed for
four different chip regions: The X plane (Layer 1) region and three regions on the Y plane (Layer
0); each corresponding to a pair of GTFEs that share a distinct shaping current. Increasing the
current feeding the shaper by reducing the resistance in the circuit reduces the shaping time, the
time it takes the shaper to reach a maximum voltage. Increasing the resistance, however, may cause
the shaped pulse to be longer which may cause overflow in the TOT data. As we can see from
Fig. 2.1 the MPV TOT increases inversely with shaper current (i.e. increases directly with shaper
resistance) which is what we expect.
Next we see histograms of the TOT (Fig. 2.2 and 2.3) for energies 100MeV and 35MeV
with similar results. An interesting thing to note is that as the incident particle energy decreases for
a given region we see the MPV TOT increases which means that the amount of energy deposited
increases which we know from Fig. (1.2). Also as particle energy decreases the amount of overflow,
events for which measurement was higher than the maximum value, in the layer 1 increases from
7
≈ 5% of total events to 9% and 20% for 250, 100, and 35MeV, respectively. At 35MeV in layer 0
region 1 (Fig. 2.3(b)) we can see that a large number of events are overflow. Also at 35MeV the
histograms are considerably less smooth than their 100 and 250MeV counterparts. This may be
explained by the Bethe-Bloch equation which shows that energy deposited by particles increases as
their total energy decreases which means that the energies of particles passing through the detectors
may become more varied as the initial beam energy decreases.
Because of the way the GTFEs work it is possible for more than one strip on the SSD to
gain enough charge to go above threshold which we call a ”cluster”. When this happens, a single
TOT is recorded: the largest value of TOT of all strips hit in an event. Because of this wider
distribution of charge, we might expect to see a lower MPV TOT for a given beam energy as the
number of strips in a cluster increases. What we do see, rather, is little or no difference in the mean
TOT for varying cluster sizes. In fact, in some cases i.e. 250MeV beam energy (Fig. 2.4), we see the
MPV TOT slightly increase suggesting more charge was deposited in the SSD. For 100MeV (Fig.
2.5) we do see a slight decrease in the MPV TOT as cluster size increases but the decrease is not
significant. For 35MeV (Fig. 2.6) we do see a marked difference in MPV TOT for events with three
strips over threshold but as the distribution bleeds into overflow, it is difficult to make a judgment
on the significance of the increase.
If we look at the proportions of cluster sizes in Fig. 2.4(d), 2.6(d), and 2.5(d) we see a
clear difference for 35MeV from 100 or 250MeV. The proportion of two and three strip events to
single strip events increases noticeably. One possible explanation for this could be multiple Coulomb
scattering which describes the scattering of nuclei as they pass close to other nuclei. The equation
for the angle which encompasses 98% of the projected distribution is as follows[6]:
θ0 =13.6MeV
βcpz√
x/X0[1 + 0.038ln(x/X0)] (2.1)
According to Physics Letters B, ”here, p, βc, and z are the momentum, velocity, and charge number
of the incident particle, and x/X0 is the thickness of the scattering medium in radiation lengths”.
In this case, z=1 for a proton, βc is 7.974×107m/s for a 35MeV proton, p is 8.621×10−7 MeV∗sm , and
8
x is the detector thickness of 400µm. X0 is defined by the following equation:
X0 =716.4ρA
Z(Z + 1)ln(287/√
Z)(2.2)
which, since ρ=2.33g/cm2, A=28 and Z=14 for silicon, gives us a value of 9.45cm. This means that
θ0 is 0.0102 radians. With a thickness of 400µm, θ0 times the thickness will give us the approximate
scattering length of 2.33µm. With a detector strip pitch, or distance between strips, of 228µm this
means that multiple Coulomb scattering does not account for the increase of larger cluster sizes.
An alternate explanation is that the increased energy deposition from lower energy particles is just
enough to set strips that were otherwise charged for 100 and 250MeV beams over the threshold.
9
2.1.1 Figures
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
2000
4000
6000
8000
10000
X Plane Entries 414089
Mean 12.46
Overflow 4756
Constant 5.725e+004
MPV 9.341
Sigma 1.392
X Plane
(a) Layer 1; 280kΩ resistor; Median: 11.3
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
10
20
30
40
50
60
Region 1 Y Entries 4278Mean 24.08Overflow 159Constant 275.1MPV 19.64Sigma 3.044
Region 1 Y
(b) Layer 0 region 1; 470kΩ resistor; Median: 23.3
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
2000
4000
6000
8000
10000
12000
Region 2 Y Entries 397755
Mean 10.61
Overflow 5431
Constant 6.677e+004
MPV 7.365
Sigma 1.192
Region 2 Y
(c) Layer 0 region 2; 280kΩ resistor; Median: 8.9
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
50
100
150
200
250
300
350
400
Region 3 Y Entries 10215Mean 9.504Overflow 131Constant 1848MPV 6.239Sigma 1.07
Region 3 Y
(d) Layer 0 region 3; 180kΩ resistor: Median: 7.7
Figure 2.1: TOT histograms for all cluster sizes: 250MeV proton beam, 103.5mV threshold, allshaping resistors, internal triggering, ghosts removed
10
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
1000
2000
3000
4000
5000
X Plane Entries 410523
Mean 21.66
Overflow 3.509e+004
Constant 2.762e+004
MPV 16.97
Sigma 2.978
X Plane
(a) Layer 1; 280kΩ resistor; Median: 20.5
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
5
10
15
20
25
30
Region 1 Y Entries 3435Mean 35.85Overflow 1103Constant 105MPV 40.52Sigma 8.043
Region 1 Y
(b) Layer 0 region 1; 470kΩ resistor; Median: 42.5
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
1000
2000
3000
4000
5000
6000
Region 2 Y Entries 395720
Mean 20
Overflow 2.989e+004
Constant 2.804e+004
MPV 14.49
Sigma 2.78
Region 2 Y
(c) Layer 0 region 2; 280kΩ resistor; Median: 17.9
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
20
40
60
80
100
120
Region 3 Y Entries 7185Mean 17.12Overflow 465Constant 541.6MPV 11.29Sigma 2.473
Region 3 Y
(d) Layer 0 region 3; 180kΩ resistor; Median: 14.5
Figure 2.2: TOT histograms for all cluster sizes: 100MeV proton beam, 103.5mV threshold, allshaping currents, internal triggering, ghosts removed
11
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
200
400
600
800
1000
1200
1400
1600
X Plane Entries 137209
Mean 34.07
Overflow 2.955e+004
Constant 6918
MPV 32.12
Sigma 3.85
X Plane
(a) Layer 1; 280kΩ resistor; Median: 36.5
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
10
20
30
40
50
Region 1 Y Entries 57079
Mean 37.17
Overflow 5.584e+004
Constant 1.057e+004
MPV 437.4
Sigma 131
Region 1 Y
(b) Layer 0 region 1; 470kΩ resistor; Median: N/A
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
100
200
300
400
500
600
700
Region 2 Y Entries 51731Mean 31.75Overflow 9721Constant 3104MPV 28.64Sigma 3.074
Region 2 Y
(c) Layer 0 region 2; 280kΩ resistor; Median: 33.1
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
50
100
150
200
250
300
350
400
Region 3 Y Entries 26974Mean 26.19Overflow 5732Constant 1419MPV 21.52Sigma 3.031
Region 3 Y
(d) Layer 0 region 3; 180kΩ resistor: Median: 27.1
Figure 2.3: TOT histograms for all cluster sizes: 35MeV beam energy, 103.5mV threshold, allshaping currents, internal triggering, ghosts removed
12
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
1000
2000
3000
4000
5000
6000
7000
8000
9000
X Plane Entries 356346
Mean 12.45
Overflow 3977
Constant 4.956e+004
MPV 9.335
Sigma 1.383
X Plane
(a) 1 strip over threshold
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
200
400
600
800
1000
1200
X Plane Entries 52016Mean 12.54Overflow 597Constant 7131MPV 9.379Sigma 1.384
X Plane
(b) 2 strips over threshold
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
20
40
60
80
100
X Plane Entries 4005Mean 13.19Overflow 78Constant 470.9MPV 9.51Sigma 1.619
X Plane
(c) 3 strips over threshold
Num strips X0 2 4 6 8 10 12
0
50
100
150
200
250
300
350
310´X Plane Entries 414089
Mean 1.142
Overflow 4
X Plane
(d) Cluster size
Figure 2.4: TOT histograms for varying cluster sizes: 250MeV beam energy, 103.5mV threshold,280kΩ shaping resistor, internal triggering, ghosts removed
13
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
500
1000
1500
2000
2500
3000
3500
4000
4500
X Plane Entries 339185
Mean 21.72
Overflow 2.906e+004
Constant 2.273e+004
MPV 16.99
Sigma 2.997
X Plane
(a) 1 strip over threshold
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
200
400
600
800
1000
X Plane Entries 67438Mean 21.39Overflow 5570Constant 4695MPV 16.82Sigma 2.841
X Plane
(b) 2 strips over threshold
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
10
20
30
40
50
X Plane Entries 3137Mean 21.15Overflow 273Constant 197MPV 16.86Sigma 2.826
X Plane
(c) 3 strips over threshold
Num strips X0 2 4 6 8 10 12
0
50
100
150
200
250
300
350310´
X Plane Entries 410523
Mean 1.173
Overflow 1
X Plane
(d) Cluster size
Figure 2.5: TOT histograms for varying cluster sizes: 100MeV beam energy, 103.5mV threshold,280kΩ shaping resistor, internal triggering, ghosts removed
14
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
200
400
600
800
1000
X Plane Entries 84404
Mean 33.73
Overflow 1.629e+004
Constant 4580
MPV 31.56
Sigma 3.52
X Plane
(a) 1 strip over threshold
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
50
100
150
200
250
300
350
400
450
X Plane Entries 38562Mean 34.06Overflow 8024Constant 1942MPV 32.14Sigma 3.895
X Plane
(b) 2 strips over threshold
s)mToT (0 5 10 15 20 25 30 35 40 45 50
0
20
40
60
80
100
X Plane Entries 13568Mean 37.09Overflow 5044Constant 445.3MPV 38.55Sigma 6.666
X Plane
(c) 3 strips over threshold
Num strips X0 2 4 6 8 10 12
0
10000
20000
30000
40000
50000
60000
70000
80000
X Plane Entries 137209
Mean 1.555
Overflow 0
X Plane
(d) Cluster size
Figure 2.6: TOT histograms for varying cluster sizes: 35MeV beam energy, 103.5mV threshold,280kΩ shaping resistor, internal triggering, ghosts removed
15
2.2 Energy loss of protons
To convert our TOT measurements into energy deposited we need to look at our TOT/Charge
calibration data. Calibration takes place when a 46pF capacitor is charged with a known calibration
voltage and the resulting charge is injected into a strip on the SSD. This creates a pulse within the
GTFE’s shaper which then gives us a TOT reading. With these data, we can create fits to correlate
input charge with TOT, for a given threshold voltage, 103.5mV in this case.
Charge (fC)0 5 10 15 20 25 30 35 40 45 50
ToT
(us
)
0
10
20
30
40
50
Calibration 0gtfe3Entries 3582Mean x 24.21Mean y 8.556RMS x 11.47RMS y 3.678
/ ndf 2c 0.008252 / 6p0 19.24± 0.508 p1 1.372± 0.354 p2 0.0226± -0.0006945
0gtfe3Entries 3582Mean x 24.21Mean y 8.556RMS x 11.47RMS y 3.678
/ ndf 2c 0.008252 / 6p0 19.24± 0.508 p1 1.372± 0.354 p2 0.0226± -0.0006945
Calibration
Figure 2.7: Layer 0, 280 kΩ calibration with second order approximation
As 2.7 shows, for example, we get a relationship for GTFE 3, Layer 0 that TOT = −0.508+
0.354Q− 6.95×10−4Q2. If we apply the mean TOT for a given beam energy to this formula, we can
solve for Q and the lower root, on the ascending side of the quadratic, should be the value for the
mean of the charge deposited in the detector. Because of the limitations of the calibration routine,
calibration data plateaus at 25µs which is half of the maximum TOT the prototype can record. For
beam test TOT data larger than 25µs the fits were extrapolated using the equations acquired from
the calibration graphs which introduces a large amount of error for large TOTs.
Since using the mean, according to the histograms, isn’t precise as there will always be
16
some overflow, we use the median, which is close to the mean (about 10% less than the mean in the
case of Fig. 2.1(a)) and isn’t affected by overflow, to estimate the real mean which will become more
important for the cases with high overflow. This means that the calculations of the energy using
the median will be an underestimate of the energy that could be calculated with the true mean.
When the charge is found, we can then convert it to energy using the following relationship:
∆E
Q=
Ei
e≈ 0.02247
MeV
fC(2.3)
where E is the energy deposited in MeV, Q is the charge deposited in fC, e is the elementary charge
of an electron (≈ 1.602×10−4fC), and Ei is the energy required to create an electron-hole pair
(≈ 3.6×10−6MeV). We can then compare this to the mean energy loss as outlined by NIST (Fig.
1.2) with the following equation:
∆E ≈ dE
dx(MeV cm2/g)ρSi∆x (2.4)
where ρSi is the density of Silicon (≈ 2.33 gcm3 ) and ∆x is the detector thickness (.04cm). Since the
mean energy deposited according to Eq. 2.4 at 100MeV is approximately 0.54MeV and the change
in stopping power is less than 1% for this change in energy this is a good approximation for the
energy deposited within 0.005MeV. Comparing this to the value of 1.24MeV we get from applying
the median TOT of 17.9µs from table 2.1 to the calibration fit and Eq. 2.3 we see a difference
experimental of 129% from the predicted value. Similarly the results of 0.56MeV and 2.71MeV we
get for 250MeV and 35MeV beams differ from the expected values of 0.30MeV and 1.21MeV by 87%
and 124% respectively. Table 2.1 and Fig. 2.11 show the results for the calculated mean energy loss
along with the expected energy loss for various energies and shaping resistors.
If we compare the energies calculated between layer 1 and layer 0 region 2, we would expect
to see very similar results as the energy lost when the beam passed through layer 0 would barely
affect the energy loss in layer 1. Expected Energy Loss column of table 2.1 show, for example,
0.544MeV vs. 0.546MeV for a 100MeV beam for layers 0 and 1 respectively. What we see in fact is
a substantial difference between the two results of 1.24MeV and 0.81MeV.
17
Charge (fC)0 5 10 15 20 25 30 35 40 45 50
ToT
(us
)
0
10
20
30
40
50
Calibration 0gtfe1Entries 3584Mean x 24.19Mean y 20.9RMS x 11.47RMS y 5.704
/ ndf 2c 1.363e-025 / 0p0 59.78± 0.9729 p1 9.648± 1.233 p2 0.3423± -0.005503
0gtfe1Entries 3584Mean x 24.19Mean y 20.9RMS x 11.47RMS y 5.704
/ ndf 2c 1.363e-025 / 0p0 59.78± 0.9729 p1 9.648± 1.233 p2 0.3423± -0.005503
Calibration
Figure 2.8: Layer 0, 470kΩ calibration with second order approximation up to 25µs
Charge (fC)0 5 10 15 20 25 30 35 40 45 50
ToT
(us
)
0
10
20
30
40
50
Calibration 0gtfe4Entries 3584Mean x 24.2Mean y 10.85RMS x 11.46RMS y 4.543
/ ndf 2c 0.02095 / 7p0 8.949± -0.01401 p1 0.6382± 0.5233 p2 0.01237± -0.002953
0gtfe4Entries 3584Mean x 24.2Mean y 10.85RMS x 11.46RMS y 4.543
/ ndf 2c 0.02095 / 7p0 8.949± -0.01401 p1 0.6382± 0.5233 p2 0.01237± -0.002953
Calibration
Figure 2.9: Layer 0, 180kΩ calibration with second order approximation
18
Charge (fC)0 5 10 15 20 25 30 35 40 45 50
ToT
(us
)
0
10
20
30
40
50
Calibration 1gtfe3Entries 3586Mean x 24.19Mean y 14.35RMS x 11.46RMS y 6.11
/ ndf 2c 0.002381 / 4p0 22.53± 0.2871 p1 1.825± 0.6558 p2 0.0354± -0.002567
1gtfe3Entries 3586Mean x 24.19Mean y 14.35RMS x 11.46RMS y 6.11
/ ndf 2c 0.002381 / 4p0 22.53± 0.2871 p1 1.825± 0.6558 p2 0.0354± -0.002567
Calibration
Figure 2.10: Layer 1, 280kΩ calibration with second order approximation
Table 2.1: Calculations for Energy Loss in Silicon
Beam Shaping Median Mean Mean ExpectedEnergy Layer Resistor TOT Charge Energy Energy Loss(MeV) (kΩ) (µs) Deposited Loss in 400µm
(fC) (MeV) Si (MeV)0 470 — —† —† 1.21
35 0 280 33.1 120.6 2.71 1.211 280 36.5 80.7 1.81 1.250 180 27.1 —† —† 1.210 470 42.5 41.3 0.93 0.54
100 0 280 17.9 55.1 1.24 0.541 280 20.5 35.9 0.81 0.550 180 14.5 34.4 0.77 0.540 470 23.3 19.9 0.45 0.30
250 0 280 8.9 24.9 0.56 0.301 280 11.3 18.1 0.41 0.300 180 7.7 16.2 0.36 0.30
† TOT did not correspond to a charge according to calibration data fits.
19
0
0.5
1
1.5
2
2.5
3
50 100 150 200 250 300
Ene
rgy
Loss
(M
eV)
Energy (MeV)
Mean Stopping Power of Protons in Silicon
Expected Energy LossLayer 0 Energy Loss for 470kΩLayer 0 Energy Loss for 280kΩLayer 0 Energy Loss for 180kΩLayer 1 Energy Loss for 280kΩ
Figure 2.11: A plot of expected energy loss and calculated energy loss for all beam energies andshaper resistors.
20
3 Conclusions
Our findings show a 121%, 129%, and 87% discrepancy between the predicted and ex-
perimentally measured values of the energy deposited in the GLAST 2000 SSDs for proton beam
energies of 35MeV, 100MeV, and 250MeV, respectively. This means that measuring the energy of
the particle that was lost directly via the SSDs may not be an accurate method. An analysis of the
energy detected by the calorimeter with and without the SSDs would show greater insight into the
effects of the SSDs on the particles and thus the effectiveness of the SSDs in measuring energy.
Sources of error may include charge sharing between several strips or a different thickness
of detector than assumed but as charge sharing would result in a lower TOT and therefore lower
energy measured and the detectors should be close to the referenced thickness within less than 1µm
these sources are unlikely and would have little effect anyway.
21
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