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CSU-Pueblo
Time Dilation Effect of Special Relativity
Objective: Measure the stopping rate of muons, as a function of depth in the atmosphere to demonstration the time dilation effect of special relativity
MJolley1/1/2013
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Background
The origins of Cosmic rays are still a
mystery to scientists. In one theory Cosmic rays
originate in explosions that take place in outer
space. They are mostly protons accelerated in the remnants of these
explosions to very high velocities. This
can result in energies of 1020 eV. (Cosmic
ray 2011) Some of these cosmic rays
reach the Earth and cause showers in the
atmosphere. During cosmic ray showers
the high energy particles ionize the
atmosphere and collide with molecules
like nitrogen and oxygen. (Figure 1) The
particles are transformed into smaller,
lighter particles that swiftly decay via the
weak force, whose strength can be
described by the Fermi coupling constant (Gf), into the high energy muon
that we are able to detect at the Earth’s
surface. There are many ways to detect these muons.
Discovered in 1936 by Physicist Carl David Anderson (Encyclopedia
Britanica Online 2013), the muon was originally thought to be a meson,
which led to it being named the mu meson or muon. However, the muon
The muon was so unexpected that,
regarding its discovery, Nobel laureate Isidor
Isaac Rabi famously quipped,
“Who ordered that?”
Figure 1
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was found to interact weakly with the neutron and proton, and thus classified
as a lepton. The muon is similar to the electron in characteristic behavior
but has about 200 times the mass, giving it the nickname the ‘heavy
electron’, and a typical energy of about 20 GeV. (University of Rochester
n.d.) This large mass and relatively small force holding it together causes
the muon to decay, usually, into an electron or positron, and two neutrinos
(𝜇± →e± +2 ν). (Figure 2) These muons live for only about two millionths of a
second before they decay. When a muon enters a scintillator it loses an
amount of energy, around 50 MeV, passing through the wall. While inside,
depending on the remaining energy, the
muon can ‘come to rest’ and emit the (𝜇±
→e± +2 ν) with these particles flying off
with the muons remaining kinetic energy.
Goals
Muon decays can be detected within the scintillator tube and analyzed
by the Muon Physics software. Lifetime measurements involve muons that
enter the tube, slow, stop, and decay. These electrons will have energy of ≈
160 MeV. The experimental mean lifetime of the muon is determined in the
muon.exe program that was provided with the detector, by the ‘least-
squares fit’ to histograms in the form of:
N (t )=N0 e−tτ ,
Figure 2
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whereN ( t ) is t he distributionof particles wit h lifetime t
and N 0 is anormalizaton parameter , the number of muons ot time t=0
This equation gives τ, the measured raw lifetime, which should be
approximately 2.19703±0.11114 µs. With τ, the Gf constant can be
calculated using the equation:
Gf=ℏτ μ192 π3
m5
where
ħ (Planc k ' sConstant )=6.58×10−25GeV∗s ,m (MuonMass )=105 MeVc2
.
This can be compared to the accepted value of 1.17×10−5GeV−2 (The NIST
Reference on Consants, Units, and Uncertainty 2011), to show the strength
of the weak force.
The time dilation effect of the muons can be observed by first
extracting data from the Muon Physics program at two different elevations
for the number of observed muon decays over a given time interval. A
measurement for stopping rate is taken at a first altitude and a respective
approximated rate is determined for a second rate. The respective rate is
calculated both with time dilation effects and without. A second
measurement is then taken at the second altitude and the results are
compared. The measurements at the second altitude must take into account
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both the muon energy loss in transit from the higher altitude to the lower, as
well as variations in the shape of the muon energy spectrum, which peaks
around p=500MeV/c.
The energy loss can be accounted for by making a simple estimate for
the energy loss over the change in altitude given by the equation:
∆ E=Co∗∆H∗ρair ( ave )
WithCo=2MeVgcm2
, ΔH=¿h2−h1∨,
And ρair (ave )=1∆ H∫
h1
h2
ρ0×e−h8.4m
With ρ0=1.28×10−3 gcm3
.
The transit time from the higher altitude to the lower altitude in the lab
reference frame is denoted t and is simply determined by:
t=∆ Hc .
Using this t, the predicted stopping rate for another elevation can be
calculated using:
R( predicted)Pueblo(no time dilation)=R0×e−tτ
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where R0 is a correction factor to be calculated later.
Using the corresponding Lorentz factors:
γ2=1.5 ,
assuming the muon stopped, on average, halfway into the scintillator,
γ1=E1mc2
the gamma factor right before it enters the scintillator
with
E1=E2+∆ E ,
E2=160MeV
the time for the path in the muon’s reference frame t’:
t '= mcρair(ave)Co
∫γ 1
γ 2 dγ√γ 2−1
.
Using t’ in the form of:
t '=(some factor )∗τ.
Compute the theoretical stopping rate in Pueblo taking relativity into
consideration:
R( predicted)Pueblo(time dilation)=R0×e(−t 'τ ).
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In order to correct for the variations in the shape of the muon energy
spectrum in the region from 160 MeV- 800 MeV, a double ratio of the two
stopping rates is determined. First, ignoring the variance in the shape of the
spectrum find:
R(ignore shape)=e−t 'τ
This is the calculated stopping rate ratio at the elevation of Pueblo. Then find
the raw stopping rate:
Rraw=Stopping rate PuebloStopping rate Monarch
This is the ratio of the two measured stopping rates at the two elevations.
Finally, take the double ratio:
Ro=Rraw
R(ignore shape)
This gives the muon spectrum correction factor, Ro. This factor is then
multiplied by the Ratios of the predictions:
RPNTD=Ro∗R( predicted)Pueblo(no time dilation)
RPTD=Ro∗R (predicted )Pueblo(timedilation )
And difference is calculated.
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EquipmentThe main parts of the equipment are the plastic scintillator,
photomultiplier tube, and the signal amplifier. The scintillator,
photomultiplier tube, and a high voltage supply are housed in an anodized
aluminum cylinder. The high voltage supply has an external control, with all
other high voltage components contained within the cylinder. The scintillator
and photomultiplier tube are fed to the signal amplifier. The scintillator is an
organic transparent mixture of a plastic solvent with an aromatic ring
structure and one or more fluors. A particle such a muon, carrying a charge,
will lose a certain amount of kinetic energy by either ionization or atomic
excitation of the solvent. This kinetic energy causes the electrons to excite
in the fluor molecules. When this electron relaxes a radiated blue light is
emitted. This activates a timing device and readout the time measurement
when another signal is detected within 20 𝜇s. This second signal, within this
time frame, can be thought of as a muon decay event. The Electron emitted
when the muon decays excites the fluor molecules similarly. These
measurements are then sent to the muon software.
Procedure
The data collection procedure begins with installing the software and
ensuring the wiring is properly connected. The detector is set up to
distinguish between muons which enter the detector one after another and
muons which actually decays within the detector by adjusting the duration of
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times between the first pulse detected in the photomultiplier tube and a
successive pulse in the tube. Another way to ensure proper lifetime
measurements is to take data over considerable time periods.
After the software and hardware is running properly the data is
collected into a .data file which can be opened in a text reading program. At
the end of each run, a screen shot is taken and saved as a .jpg file. For each
run, the .data file is uploaded into Excel. In Excel the total time of each run is
calculated. The program time stamps the runs in UNIX time and this number
car be put into an online UNIX to month-day-year time. Excel also goes
through the data and does a sum of the values that are less than 4000 in the
first row of the data file. The values in these cells represent the time
between successive signals in nanoseconds, and indicate a decay event and
therefore represent a muon lifetime. These values are then uploaded into a
Matlab file and calculations for the Fermi Coupling constant and the influx of
detected muons at the current elevation are performed.
A predicted stopping rate is calculated for the higher stopping rate
without considering time dilation. The correction factor is used to scale the
ratios of stopping rates and is compared to the actual stopping rate at the
higher altitude.
Data and Calculations
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The manual recommends that the High Voltage (HV) adjustment on the
top of the scintillator be set to between -1100 and -1200 volts (Ye 2005). The
HV was set to 9 giving a voltage reading of -11.54 which is 1/100 time the
output in the photomultiplier tube or a reading of -1154 Volts within the
photomultiplier. The time between two pulses of light can be adjusted using
the Time Adj. knob on the photomultiplier. The output of the photomultiplier
tube is connected from the detector to the electronics box and the
discriminator is set so the output is between 180 and 220 MeV. The
threshold voltage was measured to be 206 MeV.
The muon.exe program was then run for an extended period of time in
two location. The first being Pueblo, Co., having an elevation of 1420 m
above sea level (Data 2003-2012). The data was collected and stored. The
detector was then taken to an elevation of 3290 m above sea level at the
base of Monarch Mountain. (Stats and Hours n.d.) This gave a difference in
elevation (Δh) of 1870 m. Data from the Pueblo run was selected to have a
collection time comparable to that of the Monarch run.
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The τ was taken from the upper right hand side of the screen after
each run was saved.
The average of these measured lifetimes was then used in the calculation of
the Fermi Coupling Constant using the mass of the muon to be106 MeVc2
(al.
2012) and ħ to be 6.58×10−25GeV∗s (The NIST Reference on Consants, Units,
and Uncertainty 2011). The value obtained for the Fermi Coupling Constant
with the Pueblo data and the Monarch data are, 1.18×10−5GeV−2 and
1.19×10−¿GeV−2¿ respectively. With an accepted value of 1.7×10−5GeV−2 these
measurements give a percent error of 0.855% and 1.17% respectively.
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The stopping rate for each elevation was also determined with a MATLAB
program. The data from the muon apparatus is loaded into an Excel file. In
the Excel spreadsheet the total time duration of each run is calculated by
taking the last number stamped in the UNIX time code and subtracting the
first UNIX time code. These numbers are stored in a separate sheet in the
file. Cells where decay events are indicated by a number under 40000 and
indicate the time between successive light pulses. Numbers above 40000
indicate a time interval where no decay events took place. The total number
of muon decay events is determined by totaling the cells with values under
40000. This number is also stored in the separate sheet.
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The total time duration of the data collection in Monarch was 19 hours
27 minutes and 24 seconds. It was determined that the 21st set of data taken
at the pueblo elevation had a reasonably close collection time to that of the
Monarch run with a total of 22 hours 10 minutes and 39 seconds. The
stopping rates for each of the elevations was shown to be 0.0284 muonssec and
0.0644 muonssec , respectively.
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The transit time in the observer’s reference frame, ignoring relativity is
determined to be 6.28 µsec or t=2.85 τ . Using this number the non-corrected
stopping rate ratio for Monarch is:
R( predicted)Pueblo(no timedependence)=R0×0.057
Where R0 is the correction factor.
In order to accurately predict the stopping rate ratio a few corrections
must be calculated. First, as a muon travels through the air it inevitably
loses energy. This energy loss was estimated using the air density averaged
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over the change in elevation and resulted in ρair=972 gm3 . Using this result
∆ E=364MeV .Adding ΔE to E2=160MeV , E1=524 MeV was determined. This
value of E1 was then divided by the muons mass times c2 to determine the
muon’s gamma factor right before it enters the photomultiplier tube, γ1=4.9 .
This gamma factor is used in the integral to determine the transit time in the
particle’s rest frame, t '=2.38μsec. The predicted ratio in pueblo becomes
R( predicted)Pueblo (timedilation)=R0×0.339
and the ratio which still ignores the shape of the muon energy spectrum
becomes
R(ignore shape)=0.339
The second correction that must be done was to correct for the variations in
the shape of the muon energy spectrum. First the raw stopping rates at the
two elevations were calculated giving Rraw=0.02840.0644
=0.441. Then a double ratio
was calculated , Ro=0.4410.339
=1.30.
Finally, the double ratio is used in the two predicted equations,
R( predicted)Pueblo(no time dilation)=1.30×0.056=0.0749 and
R( predicted)Pueblo(time dilation)=1.30×0.339=0.441. The prediction which does not take
time dilation into account is off by a factor of 5.89 when compared to the
actual raw data..
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Results and ConclusionThe main goal of the experiment was to show, through measurement and
comparison, that muons travelling at very high speeds, those near the speed
of light, exhibited the time dilation effect of Einstein’s Special Relativity. This
was done by measuring the decay of muons in the photomultiplier tube and
determining the mean lifetime of these muons. This lifetime along with the
time dilated lifetime was put into ratios and compared. The comparison
leads to the conclusion that the actual measured ratio of muon decays is
much more like the calculation of the time dilated prediction rather than the
non-time dilated prediction. This shows that hypothesis that there are no
time dilation effects happening must be rejected and that the measured data
is more consistent and more supportive of the relativistic hypothesis. The
Fermi Coupling Constant calculation was fairly close to the accepted value.
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Encyclopedia Britanica Online. 2013. s.v."Carl David Anderson". Accessed April 2013. http://www.britannica.com/EBchecked/topic/23589/Carl-David-Anderson.
n.d. Stats and Hours. Accessed Jan 2013. http://www.skimonarch.com/index.php/generalinfo/stats-a-hours.
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The NIST Reference on Consants, Units, and Uncertainty. 2011. Fundamental Physical Constants. June 2. Accessed Jan 2013. http://physics.nist.gov/cgi-bin/cuu/Value?bgspu.
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