Special Relativity Muon problem

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SUMMARY

The discussion centers on the muon problem in special relativity, specifically whether a muon produced at the top of the Earth's atmosphere can reach the ground before decaying. Calculations show that the time dilation experienced by the muon, traveling at 0.999c, allows it to reach the ground in approximately 3.3 x 10^-5 seconds, which is less than its dilated decay time of 4.5 x 10^-5 seconds. From the muon's perspective, the distance to the ground is length contracted to 447.1 meters, further supporting the conclusion that it reaches the ground before decaying. The logic of the argument is confirmed by the consistency of results across different reference frames.

PREREQUISITES
  • Understanding of special relativity concepts, including time dilation and length contraction.
  • Familiarity with the Lorentz factor, represented as γ (gamma).
  • Knowledge of the equations for time dilation: $$\Delta t=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}\Delta\tau$$ and length contraction: $$\Delta l'=\sqrt{1-\frac{v^2}{c^2}}\Delta l$$.
  • Basic understanding of muon decay and cosmic ray interactions with the Earth's atmosphere.
NEXT STEPS
  • Study the Lorentz transformations in detail to understand their implications in different reference frames.
  • Explore the concept of proper time and how it relates to time dilation in special relativity.
  • Investigate real-world applications of special relativity, such as GPS technology and particle physics experiments.
  • Examine the implications of relativistic speeds on particle decay and cosmic ray phenomena.
USEFUL FOR

Students of physics, educators teaching special relativity, and researchers in particle physics or cosmology will benefit from this discussion, particularly those interested in the behavior of high-speed particles like muons in Earth's atmosphere.

Diracobama2181
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Homework Statement
The height of the earth's atmosphere from top to ground is 10 km. Due to collisions of cosmic rays with the earths atmosphere, muons are produced at the top of the atmosphere
at a velocity of 0.999c where the speed of light is [tex]c=3.00*10^8 m/s[\tex]. At rest a muon decays in [tex]2*10^-6[\tex] sec.
i) Does the muon reach the ground?
If it does reach the ground
ii) How would an observer on the ground explain it?
iii) How would an observer moving with the muon explain it?
Relevant Equations
$$\Delta t=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}\Delta\tau$$
$$\Delta l'=\sqrt{1-\frac{v^2}{c^2}}\Delta l$$
i) The muon reaches the ground

ii)
To a ground observer, the decay time is dilated
$$\Delta t_d=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}\Delta\tau_d>\Delta \tau_d$$

The time for the muon to reach the ground is

$$\Delta t_g=\frac{10 km}{0.999c}< \Delta t_d$$

which is why it reaches the ground.

iii)
From the muon's frame, the ground comes toward it with a velocity v=0.999c[\itex], and hence the distance to the ground is length contracted<br /> by<br /> $$\Delta l&#039;=\sqrt{1-\frac{v^2}{c^2}}10 km$$<br /> <br /> so<br /> $$\frac{\Delta l&#039;}{0.999c}=\frac{\sqrt{1-\frac{v^2}{c^2}}10 km}{0.999c}&lt;2\times 10^{-6} s $$<br /> <br /> So the muon would reach the ground.<br /> <br /> Does this sufficiently answer the above questions? Any feedback would be greatly appreciated. Thanks.
 
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I would like to see the actual numbers to support the conclusions.
 
Diracobama2181 said:
Homework Statement:: The height of the Earth's atmosphere from top to ground is 10 km. Due to collisions of cosmic rays with the Earth's atmosphere, muons are produced at the top of the atmosphere
at a velocity of 0.999c where the speed of light is c=3.00*10^8 m/s[\tex]. At rest a muon decays in 2*10^-6[\tex] sec.&lt;br /&gt; i) Does the muon reach the ground?&lt;br /&gt; If it does reach the ground&lt;br /&gt; ii) How would an observer on the ground explain it?&lt;br /&gt; iii) How would an observer moving with the muon explain it?&lt;br /&gt; &lt;b&gt;Relevant Equations::&lt;/b&gt; $$\Delta t=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}\Delta\tau$$&lt;br /&gt; $$\Delta l&amp;#039;=\sqrt{1-\frac{v^2}{c^2}}\Delta l$$&lt;br /&gt; &lt;br /&gt; i) The muon reaches the ground&lt;br /&gt; &lt;br /&gt; ii)&lt;br /&gt; To a ground observer, the decay time is dilated&lt;br /&gt; $$\Delta t_d=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}\Delta\tau_d&amp;gt;\Delta \tau_d$$&lt;br /&gt; &lt;br /&gt; The time for the muon to reach the ground is&lt;br /&gt; &lt;br /&gt; $$\Delta t_g=\frac{10 km}{0.999c}&amp;lt; \Delta t_d$$&lt;br /&gt; &lt;br /&gt; which is why it reaches the ground.&lt;br /&gt; &lt;br /&gt; iii)&lt;br /&gt; From the muon&amp;#039;s frame, the ground comes toward it with a velocity v=0.999c[\itex], and hence the distance to the ground is length contracted&amp;lt;br /&amp;gt; by&amp;lt;br /&amp;gt; $$\Delta l&amp;amp;#039;=\sqrt{1-\frac{v^2}{c^2}}10 km$$&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; so&amp;lt;br /&amp;gt; $$\frac{\Delta l&amp;amp;#039;}{0.999c}=\frac{\sqrt{1-\frac{v^2}{c^2}}10 km}{0.999c}&amp;amp;lt;2\times 10^{-6} s $$&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; So the muon would reach the ground.&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; Does this sufficiently answer the above questions? Any feedback would be greatly appreciated. Thanks.&amp;lt;br /&amp;gt;
&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; &amp;lt;blockquote data-attributes=&amp;quot;member: 493650&amp;quot; data-quote=&amp;quot;PeroK&amp;quot; data-source=&amp;quot;post: 6616605&amp;quot; class=&amp;quot;bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch&amp;quot;&amp;gt; &amp;lt;div class=&amp;quot;bbCodeBlock-title&amp;quot;&amp;gt; PeroK said: &amp;lt;/div&amp;gt; &amp;lt;div class=&amp;quot;bbCodeBlock-content&amp;quot;&amp;gt; &amp;lt;div class=&amp;quot;bbCodeBlock-expandContent js-expandContent &amp;quot;&amp;gt; I would like to see the actual numbers to support the conclusions. &amp;lt;/div&amp;gt; &amp;lt;/div&amp;gt; &amp;lt;/blockquote&amp;gt;i) The muon reaches the ground&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; ii)&amp;lt;br /&amp;gt; To a ground observer, the decay time is dilated&amp;lt;br /&amp;gt; $$\Delta t_d=\frac{1}{\sqrt{1-\frac{0.999c^2}{c^2}}}\Delta\tau_d=22.4 \tau_d=4.5 *10^{-5}s&amp;amp;gt;\Delta \tau_d$$&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; The time for the muon to reach the ground is&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; $$\Delta t_g=\frac{10 km}{0.999c}=3.3*10^{-5} s&amp;amp;lt; \Delta t_d$$&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; which is why it reaches the ground.&amp;lt;br /&amp;gt; &amp;lt;br /&amp;gt; iii)&amp;lt;br /&amp;gt; From the muon&amp;amp;#039;s frame, the ground comes toward it with a velocity v=0.999c[\itex], and hence the distance to the ground is length contracted&amp;amp;lt;br /&amp;amp;gt; by&amp;amp;lt;br /&amp;amp;gt; $$\Delta l&amp;amp;amp;#039;=\sqrt{1-\frac{v^2}{c^2}}10 km=447.1 m$$&amp;amp;lt;br /&amp;amp;gt; &amp;amp;lt;br /&amp;amp;gt; so&amp;amp;lt;br /&amp;amp;gt; $$\frac{\Delta l&amp;amp;amp;#039;}{0.999c}=\frac{\sqrt{1-\frac{v^2}{c^2}}10 km}{0.999c}=1.5*10^{-6}&amp;amp;amp;lt;2\times 10^{-6} s $$&amp;amp;lt;br /&amp;amp;gt; &amp;amp;lt;br /&amp;amp;gt; These should be the approximate values, but I am actually more concerned whether the logic of my argument actually works (ie, if the above relations actually hold, then I have shown that the muon does actually reach the ground) Thanks.
 
Diracobama2181 said:
These should be the approximate values, but I am actually more concerned whether the logic of my argument actually works (ie, if the above relations actually hold, then I have shown that the muon does actually reach the ground) Thanks.
There's no logic to say whether the muon reaches the ground or not. It depends entirely on whether the muon is traveling fast enough. Your calculations show that ##0.999c## is fast enough.
 
PS It's interesting that SR is taught in this way that emphasises the difference between reference frames. The physics is the same, so there must be a common test for whether the muon reaches the ground.

If we let the depth of the atmosphere be ##D## (in the Earth frame) and the proper lifetime of the muon to be ##\tau##, then:

In the ground frame the muon exists for a time ##\Delta t = \gamma \tau## and travels a distance ##d = v\Delta t = \gamma v \tau## in that time. The test for reaching the ground is ##d > D##. I.e.
$$\gamma v > \frac D \tau$$In the muon frame, we have a distance to Earth of ##D' = \frac D \gamma##, hence a time of ##\Delta t' = \frac {D'} v = \frac {D}{\gamma v}##. The test to hit the ground is ##\Delta t' < \tau## hence:$$\gamma v > \frac D \tau$$ So, from that point of view it's the same test/criteria in both frames. That seems to me more logical and more in keeping with the principle of relativity.

Also, if anyone else anywhere in the universe is given the same data, then they can do the same calculations and come to the same conclusion.
 
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By the logic of my argument, I simply mean that is showing the time of of travel less than the time of decay sufficient to show that the muon would have to reach the ground. I have recently contacted my professor however, and they said this form of argument doesn't work, and I would have to give the distance that the muon traveled before decaying. His answer confused me though and I suppose I am still confused as to why my solution would not sufficiently answer the above question.
 
Diracobama2181 said:
By the logic of my argument, I simply mean that is showing the time of of travel less than the time of decay sufficient to show that the muon would have to reach the ground. I have recently contacted my professor however, and they said this form of argument doesn't work, and I would have to give the distance that the muon traveled before decaying. His answer confused me though and I suppose I am still confused as to why my solution would not sufficiently answer the above question.
I don't see it makes any difference. Either the muon hits the ground before it decays; or, the muon would travel further than the distance to the Earth's surface before it decays; it's all the same.

It's a shame if you have done the problem correctly and yet you're still confused.
 
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