How does relativity affect the detection of atmospheric muons?

In summary: No I mean I thought that since time is slowed for the muons when looking at them from a ground frame, the muons would actually take longer to reach the Earth's surface. This...this makes no sense to me.
  • #1
L_ucifer
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TL;DR Summary: I got this question on a quiz for a Coursera course on special relativity, and I'm confused about the answer. I've detailed my thinking below any help on where I went wrong would be greatly appreciated.

Question.
Muons are unstable fundamental particles. In its own rest frame, the average lifetime of a muon is t0=2×10^−6s. Thus, if initially we have No muons, after time t, the number of remaining muons is N=No e^−t/t0.

Due to collision between cosmic rays and the earth's atmosphere, No=300,000 muons are created per square meter per minute. Suppose all the muons are created at a height of 10km from the earth surface, moving towards the center of the earth at v=0.98c and can travel through the atmosphere without interactions.

Let's now compare the predictions of Newtonian mechanics and relativity. In Newtonian mechanics, we would on average detect NNewtonian muons per square meter per minute on the earth surface. In reality, relativity is important and we can detect N muons per square meter per minute.

a. NNewtonian=1, N=0.01
b. NNewtonian=1, N=10,000
c. NNewtonian=0.01, N=10,000
d. NNewtonian=1, N=1
e. NNewtonian=0.01, N=1
f. NNewtonian=0.01, N=0.01Answer.
NNewtonian is fairly easy to find. We just find the time taken for the muons to reach the surface (distance / speed ) and then put this time in the decay equation. The answer we get is 0.01.

For N, the correct logic is you need to find the relative time of a muon's lifetime. So the equation is N=No e^−t/(t0 * gamma) and t is the same. This means the correct answer is c.
My logic for N is instead of finding the relative time of a muon's lifespan, we find the relative time for the muon to reach the surface. So t = distance/speed * gamma. I'm not sure why this is wrong and why we find the relative time for a muon's lifetime instead?
EDIT:
Here's the overall equation for the correct solution:
No = 300,000
t0 = 2 * 10^-6 s
t = distance / speed = 10,000 / 0.98c
N = No * e ^ -t/(t0 * gamma)

Here's the overall equation for my solution (which is wrong):
No = 300,000
t0 = 2 * 10^-6 s
t = distance / speed = 10,000 / 0.98c
N = No * e^-(t * gamma)/t0.
 
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  • #2
L_ucifer said:
My logic for N is instead of finding the relative time of a muon's lifespan, we find the relative time for the muon to reach the surface. So t = distance/speed * gamma. I'm not sure why this is wrong and why we find the relative time for a muon's lifetime instead?
Why didn't this give the same numerical answer?
 
  • #3
PeroK said:
Why didn't this give the same numerical answer?
Edited the question and adding the same changes here:
Here's the overall equation for the correct solution:
No = 300,000
t0 = 2 * 10^-6 s
t = distance / speed = 10,000 / 0.98c
N = No * e ^ -t/(t0 * gamma)

Here's the overall equation for my solution (which is wrong):
No = 300,000
t0 = 2 * 10^-6 s
t = distance / speed = 10,000 / 0.98c
N = No * e^-(t * gamma)/t0.
 
  • #4
What's your reasoning for putting the ##\gamma## where you did in the last equation?
 
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  • #5
L_ucifer said:
Edited the question and adding the same changes here:
Here's the overall equation for the correct solution:
No = 300,000
t0 = 2 * 10^-6 s
t = distance / speed = 10,000 / 0.98c
N = No * e ^ -t/(t0 * gamma)
The logic here is that in the ground frame the muon's lifetime is dilated. If we use primes for measurements in the ground frame, then:
$$N = N_0 e^{-\frac{t'}{t'_0}} = N_0 e^{-\frac{t'}{\gamma t_0}} = N_0 e^{-\frac{d'}{v\gamma t_0}}$$
L_ucifer said:
Here's the overall equation for my solution (which is wrong):
No = 300,000
t0 = 2 * 10^-6 s
t = distance / speed = 10,000 / 0.98c
N = No * e^-(t * gamma)/t0.
This makes no sense to me. If we use the muon frame, then we have:
$$N = N_0 e^{-\frac{t}{t_0}} = N_0 e^{-\frac{d}{v\gamma t_0}} = N_0 e^{-\frac{d'}{v\gamma t_0}}$$Since the distance to the ground in the muon frame is ##d = \dfrac{d'}{\gamma}##, where ##d'## is the distance to the ground in the Earth frame.
 
  • #6
Ibix said:
What's your reasoning for putting the ##\gamma## where you did in the last equation?
I put gamma there because I thought it'd take more time for the muons to reach the ground, instead of thinking of the muon's lifetime becoming dilated.
 
  • #7
L_ucifer said:
I put gamma there because I thought it'd take more time for the muons to reach the ground, instead of thinking of the muon's lifetime becoming dilated.
You mean the faster the muon moves, the more time it takes to reach the ground?
 
  • #8
PeroK said:
You mean the faster the muon moves, the more time it takes to reach the ground?
No I mean I thought that since time is slowed for the muons when looking at them from a ground frame, the muons would actually take longer to reach the Earth's surface. This is why in my solution the time for a muon to reach the Earth's surface is greater in the relative solution than in the Newtonian solution. In mathematical terms, my understanding was: tNewtonian =10000/0.98c < trelative = tNewtonian * gamma

EDIT: grammar
 
  • #9
L_ucifer said:
No I mean I thought that since time is slowed for the muons when looking at them from a ground frame, the muons would actually take longer to reach the Earth's surface.
Quite the opposite! Do the maths, as they say. In the ground frame, a muon travels a distance ##d## at speed ##v##. How much time passes for the muon?
 
  • #10
L_ucifer said:
No I mean I thought that since time is slowed for the muons when looking at them from a ground frame, the muons would actually take longer to reach the Earth's surface.
Longer than what? Don't forget that in the muon frame the distance to the Earth's surface is shorter than ##d##. The muon may live longer in its own frame but it doesn't have to travel that far.
 
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  • #11
kuruman said:
Longer than what? Don't forget that in the muon frame the distance to the Earth's surface is shorter than ##d##. The muon may live longer in its own frame but it doesn't have to travel that far.
I don't follow this at all. The muon's lifetime (##t_0##) is defined in its rest frame. In the ground frame, it has a longer lifetime than this - of ##\gamma t_0##.
 
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  • #12
I guess what I wanted to say didn't come out right. It's better with equations.
If one calculates ##v## in the muon's frame, the distance is ##\frac{d}{\gamma}## and the time is ##t_0## so ##v=(\frac{d}{\gamma})\frac{1}{t_0}##.
If one calculates ##v## in the Earth's frame, the distance is ##d## and the time is ##\gamma t_0## so ##v=d\frac{1}{\gamma t_0}##.
I fixed the offending statement in the earlier post.
 
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FAQ: How does relativity affect the detection of atmospheric muons?

How does relativity affect the lifespan of atmospheric muons?

Relativity, specifically time dilation, significantly extends the lifespan of atmospheric muons. Muons are created in the upper atmosphere and have a very short half-life of about 2.2 microseconds. However, due to their high velocities, time dilation as predicted by special relativity causes their internal clocks to run slower relative to an observer on Earth, allowing many of them to reach the surface before decaying.

Why is the speed of atmospheric muons important in the context of relativity?

The speed of atmospheric muons is crucial because it is a significant fraction of the speed of light, which makes relativistic effects like time dilation and length contraction prominent. These effects are essential for explaining why muons, which should decay quickly, are detectable at the Earth's surface.

What role does length contraction play in the detection of atmospheric muons?

Length contraction, another consequence of special relativity, means that from the muon's perspective, the distance it has to travel to reach the Earth's surface is shorter than it would be in the Earth's reference frame. This contraction helps explain why muons can cover the distance to the surface before decaying.

How do experiments confirm the relativistic effects on atmospheric muons?

Experiments confirm relativistic effects on atmospheric muons by comparing the number of muons detected at different altitudes. The observed muon flux at the Earth's surface is much higher than would be expected without time dilation, confirming the predictions of special relativity.

What would be observed if relativity did not affect atmospheric muons?

If relativity did not affect atmospheric muons, we would observe far fewer muons at the Earth's surface. The majority of them would decay long before reaching the ground, given their short half-life, and the detected flux would be significantly lower than what is actually measured.

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