How Does Lorentz Transformation Affect Muon Decay Observations?

AI Thread Summary
The discussion centers on the application of Lorentz transformations to analyze muon decay as observed from different frames of reference. A muon traveling at 0.980c has a mean lifetime of 2.20 microseconds in its own frame, but an observer on the ground measures this lifetime to be 11.1 microseconds due to time dilation effects. The distance the muon travels in its own frame is zero, while it covers 3000 meters in the ground observer's frame, leading to confusion over the calculated time intervals. The participant grapples with the implications of the results, particularly the discrepancy between the time intervals derived from different perspectives. The discussion highlights the complexities of relativistic physics and the importance of understanding frame-dependent measurements.
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Homework Statement



Muons are created in the upper atmosphere (at a height of 3000 m) and plummet downward toward a detector at ##v=0.980c##. The mean lifetime of a muon is ##t = 2.20~\mu s##.

Find the mean lifetime of a muon measured by an observer on the ground.
Find the distance that the muon travels in its reference frame.

Use the Lorentz transforms!

Homework Equations



$$
x^{\prime} = \gamma\left(x-vt\right)\\
t^{\prime} = \gamma\left(-\frac{v}{c^2}x + t\right)\\
x = \gamma\left(x^{\prime}+vt^{\prime}\right)\\
t = \gamma\left(\frac{v}{c^2}x^{\prime} + t^{\prime}\right)
$$

The Attempt at a Solution



First, solve for ##\gamma##:
$$
\gamma = \frac{1}{\sqrt{1-\frac{v^2}{c^2}}} = \frac{1}{\sqrt{1-0.980^2}} = 5.03
$$

The mean lifetime of a muon from a ground based observer is easy. If we assume that the muon is in frame ##S^\prime##and the ground based observer is in frame ##S##, the time of decay as measured by the observer is:
$$
\Delta t = (5.03)\left(\frac{v}{c^2}(0)+(2.20~\mu s)\right)\\
\Delta t = 11.1~\mu s
$$
My problem is the second part. If I use the Lorentz transform correctly:
$$
\Delta x = 3000~m = (5.03)\left(\Delta x^{\prime} + v(0)\right)\\
\Delta x^{\prime} = 3000/5.03 = 596~m.
$$
What happens if I try to solve it the other way? Obviously the time interval is not zero:
$$
\Delta x^{\prime} = 596~m = (5.03)\left((3000~m) - v\Delta t\right)
$$
Solving for ##\Delta t##, I get:
$$
\Delta t = \frac{\frac{596~m}{5.03} - 3000~m}{-0.98c} = 9.80 \mu s
$$
Pretty cool, eh?
What exactly does that mean? The time period between measurements for the ground observer is 9.8 microseconds. However, if you divide the distance (measured by the ground observer) by the velocity of the muon, you get:
$$
\frac{3000~m}{0.98c} = 10.2 \mu s
$$
The ground observer measures that the muon is alive for 10.2 microseconds in order to reach the ground. So... what is the physical meaning of ##\Delta t = 9.8~\mu s##? That time interval is faster than the 10 microseconds required for light to traverse 3000m.

I am so confused. I expected that transforming from the primed to the unprimed coordinate system would give consistent answers. What did I do wrong?
 
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"Find the distance that the muon travels in its reference frame."

The muon is at rest within its own frame of reference, so the distance it travels within its own frame of reference is zero. But another interesting question is "During the average time that the muon decays, how far does it travel in the frame of reference of an observer on the ground."
 
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