cosmic ray muon detection department of physics and space sciences florida institute of technology...
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![Page 1: Cosmic Ray Muon Detection Department of Physics and Space Sciences Florida Institute of Technology Georgia Karagiorgi Julie Slanker Advisor: Dr. M. Hohlmann](https://reader035.vdocuments.mx/reader035/viewer/2022062407/56649dc65503460f94aba22a/html5/thumbnails/1.jpg)
Cosmic Ray Muon DetectionCosmic Ray Muon Detection
Department of Physics and Space Sciences
Florida Institute of Technology
Georgia Karagiorgi
Julie Slanker
Advisor: Dr. M. Hohlmann
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Cosmic Ray MuonsCosmic Ray Muons
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Main goalsMain goals Equipment setup Muon flux measurement Investigation of flux variation with
– Altitude– Zenith angle– Cardinal points– Overlap area
Investigation of count rate variation with– Overlap area
– Separation distance between the paddles Investigation of “doubles’ flux” with zenith angle Muon lifetime experiment Air shower experiment
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EquipmentEquipment
2 scintillation detectors developed at Fermilab
2 PMT tubes
2 PM bases
2 Coincidence logic boards (version 1 and version2)
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Scintillation DetectorsScintillation Detectors
A scintillation detector has the property to emit a small flash of light (i.e. a scintillation) when it is struck by ionizing radiation.
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SetupSetup
The setup is such that the counter on the DAQ board and the computer are recording “coincidences”, i.e. signals sent from both detectors at the same time
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DAQ board resolving time
for coincidences = 160ns
This technique
• Results in elimination of background noise
• Offers a great number of possible experiments
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I.I. Setting up equipment Setting up equipment
• Plateau Measurements for PMTs (Procedure for finding working voltage)
Example of a plateau curve:
Plateau
Onset of regeneration effects (afterpulsing, discharges, etc)
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Plateau measurementsPlateau measurements
For coincidences
Coincidence Plateau (superimposed)
0
50
100
150
200
250
300
350
6.80 7.80 8.80 9.80
HV#13 (dial units)
Co
un
ts/2
min
s
HV#14 = 7.00
HV#14 = 7.20
HV#14 = 7.40
HV#14 = 7.60
HV#14 = 7.80
HV#14 = 8.00
HV#14 = 8.20
HV#14 = 8.40
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Plateau measurementsPlateau measurements
For coincidences
Coincidence Plateau (superimposed)
0
50
100
150
200
250
300
350
6.80 7.30 7.80 8.30 8.80
HV#14 (dial units)
Co
un
ts/2
min
s
HV#13 = 7.00
HV#13 = 7.20
HV#13 = 7.40
HV#13 = 7.60
HV#13 = 7.80
HV#13 = 8.00
HV#13 = 8.20
HV#13 = 8.40
HV#13 = 8.60
HV#13 = 8.80
HV#13 = 9.00
HV#13 = 9.20
HV#13 = 9.40
HV#13 = 9.60
HV#13 = 9.80
HV#13 = 10.00
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II.II. Flux Flux
Muons reach the surface of the Earth with typically constant flux Fμ.
(count rate)d2
Fμ = (area of top panel)(area of bottom panel)
Fμ = 0.48 cm-2min-1sterad-1 (PDG theoretical value)Count rate: 0.585cm-2min-1 (horizontal detectors)Our experimental value: 36min-1 (8% efficiency)
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With altitude
We collected data on the 7 different floors of Crawford building, on the FIT campus
All measurements were taken at a same specific location on each floor, except for the one on floor 7.
III.III. Investigation of flux variation Investigation of flux variation
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With altitude
Results:
III.III. Investigation of flux variation Investigation of flux variation
Flux vs. floor level
0
0.0005
0.001
0.0015
0.002
0.0025
0.003
0.0035
0.004
0 1 2 3 4 5 6 7 8
floor
flux
(cou
nt/m
in.c
m^2
.ste
rad)
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With zenith angle θ
Expected result:
Fμ ~ cos2 θ
III.III. Investigation of flux variation Investigation of flux variation
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With zenith angle θ
Rotation mount for support of the setup:
III.III. Investigation of flux variation Investigation of flux variation
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With zenith angle θ
Results:
(7th floor Crawford)
III.III. Investigation of flux variation Investigation of flux variation
Flux vs. zenith angle
0
0.0005
0.001
0.0015
0.002
0.0025
0.003
0.0035
0.004
-150 -100 -50 0 50 100 150
zenith angle θ (degrees)
Flu
x (c
ount
/min
.cm
^2.s
tera
d)
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With zenith angle θ
Results:
(7th floor Crawford)
III.III. Investigation of flux variation Investigation of flux variation
Flux vs. cosine squared of zenith angle (expect lin. dependence)
0
0.0005
0.001
0.0015
0.002
0.0025
0.003
0.0035
0.004
0 0.2 0.4 0.6 0.8 1 1.2
cosine squared of zenith angle θ (degrees)
Flu
x (
count/
min
.cm
^2.s
tera
d)
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With zenith angle θ
Results:
(Observatory)
III.III. Investigation of flux variation Investigation of flux variation
flux vs. θ
0
0.0005
0.001
0.0015
0.002
0.0025
0.003
0.0035
0.004
-100 -50 0 50 100
θ (degrees)
flux
(cou
nt/m
in.c
m^2
.ste
rad)
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With zenith angle θ
Results:
(Observatory)
III.III. Investigation of flux variation Investigation of flux variation
flux vs. (cosθ)^2
0
0.0005
0.001
0.0015
0.002
0.0025
0.003
0.0035
0.004
0 0.2 0.4 0.6 0.8 1 1.2
(cosθ)^2
flux
(cou
nt/m
in.c
m^2
.ste
rad)
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With cardinal points
Results:
(Senior Lab)
III.III. Investigation of flux variation Investigation of flux variation
(total) count rate with azimuthal angle θEW rotation
0.000.501.001.502.002.503.003.50
-100 -50 0 50 100
angle θ (degrees)
cou
nt
rate
(m
in^
-1)
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With cardinal points
Results:
(Senior Lab)
III.III. Investigation of flux variation Investigation of flux variation
(total) count rate with cosine squared of azimuthal angle θ
EW rotation
0.00
1.00
2.00
3.00
4.00
0.000 0.200 0.400 0.600 0.800 1.000 1.200
cos 2(θ)
cou
nt
rate
(m
in^
-1)
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With cardinal points
Results:
(Senior Lab)
III.III. Investigation of flux variation Investigation of flux variation
(total) count rate with azimuthal angle θNS rotation
0.00
1.00
2.00
3.00
4.00
-100 -50 0 50 100
angle θ (degrees)
cou
nt
rate
(m
in^
-1)
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With cardinal points
Results:
(Senior Lab)
III.III. Investigation of flux variation Investigation of flux variation
(total) count rate with cosine squared of azimuthal angle θ
NS rotation
0.00
1.00
2.00
3.00
4.00
0.000 0.200 0.400 0.600 0.800 1.000 1.200
cos 2(θ)
cou
nt
rate
(m
in^
-1)
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With cardinal points
Results:
(Senior Lab)
III.III. Investigation of flux variation Investigation of flux variation
Superimposed count rate for NS and EW rotation
0.000.501.001.502.002.503.003.504.00
-100 -50 0 50 100
zenith angle θ (degrees)
coun
t rat
e (c
ount
s/m
in)
EW rotation
NS rotation
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III.III. Investigation of flux variation Investigation of flux variation
With overlap area
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With overlap area
Results:
III.III. Investigation of flux variation Investigation of flux variation
flux vs. overlap area
0
0.0015
0.003
0.0045
0.006
0.0075
0.009
0.0105
0 20 40 60 80 100 120
% overlap
flux
(cou
nt/m
in.c
m^2
.ste
rad)
Series1
Series2
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IV.IV. Investigation of count rate variation Investigation of count rate variation
With overlap area
Results:
count rate vs. overlap area (min separation distance)
y = 0.2971x + 1.4425
R2 = 0.9938
y = 0.2575x + 1.5875
R2 = 0.99980
5
10
15
20
25
30
35
0 20 40 60 80 100 120
% overlap
coun
t rat
e (m
in^-
1)
Series1
Series2
Linear (Series1)
Linear (Series2)
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IV.IV. Investigation of count rate variation Investigation of count rate variation
With separation distance d between the two paddles
Expected results: count rate is proportional to stereo angle viewed along a specific direction
stereo angle vs. d
0
0.5
1
1.5
2
0 2 4 6 8
d (in multiples of l)
ster
eo a
ngle
(*π
ste
rad)
Values calculated using Mathematica integral output
Rectangular arrangement; top/bottom phase constant (lxl); d varies (multiples of l)
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IV.IV. Investigation of count rate variation Investigation of count rate variation
With separation distance d between the two paddles
Results:
count rate (about vertical direction) vs. separation distance d
0.00
2.00
4.00
6.00
8.00
10.00
12.00
0 20 40 60 80 100 120
distance d (cm)
coun
ts/m
in
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Using the DAQ v.1 board, we recorded low energy (decaying) muon events on the computer.
These events are called “doubles.”
V.V. Investigation of “doubles’ flux” variation Investigation of “doubles’ flux” variation
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With zenith angle θ
Results:
(Observatory)
V.V. Investigation of “doubles’ flux” variation Investigation of “doubles’ flux” variation
data plot for double hits at different angles
0
20
40
60
80
100
120
140
160
180
200
-100 -50 0 50 100
angle θ (degrees)
# of doubles
% of doubles
total # of hits
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We collected data of double events We plotted tdecay of an initial sample N0 of low energy muons We fit the data to an exponential curve of the form: N(t) = N0e^(-t/T);
where T = muon lifetime
VI.VI. Muon lifetime experiment Muon lifetime experiment
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Results:
y = -63.856 + 616.791e-0.4552x
Lifetime T:T = 2.1965μs
Tth = 2.1970μs
VI.VI. Muon lifetime experiment Muon lifetime experiment
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Results:
y = 14.7029 + 1493.09e-0.4601x
Lifetime T:
T = 2.1733μs
Tth = 2.1970μs
VI.VI. Muon lifetime experiment Muon lifetime experiment
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Results:
Lifetime T:
T = 2.1422μs
Tth = 2.1970μs
VI.VI. Muon lifetime experiment (verification) Muon lifetime experiment (verification)
N(t) = No e (-t/T)y = 696.16e-0.4668x
R2 = 0.996
0
100
200
300
400
500
600
700
800
0 5 10 15 20
time t (microseconds)
N(t
) (s
ampl
e)
noise level
N(t) before noisesubtraction
Expon. (N(t) beforenoise subtraction)
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Results:
Lifetime T:
T = 2.1678μs
Tth = 2.1970μs
VI.VI. Muon lifetime experiment (verification) Muon lifetime experiment (verification)
N(t) = No e (-t/T) [after noise subtraction]
y = 465.2e-0.4613x
R2 = 0.9795
0
100
200
300
400
500
600
0 5 10 15 20
time t (microseconds)
N(t
) (r
emai
ning
sam
ple)
after noise subtraction
Expon. (after noisesubtraction)
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In progress…
Make use of: DAQ v.2 board – GPS option Another 5 detector setups assembled
during QuarkNet
IX.IX. Air shower experiment Air shower experiment
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ReferencesReferences http://pdg.lbl.gov/2002/cosmicrayrpp.pdf http://www2.slac.stanford.edu/vvc/cosmicrays/crdctour.html http://hermes.physics.adelaide.edu.au/astrophysics/muon/