Special Relativity and Decaying Particles

In summary, pions are a type of meson that is commonly created during collisions in scientific accelerators or when cosmic rays collide with particles in the upper part of the Earth's atmosphere. A particular type of pion, known as π+, has a mass of 139.6 MeV/c2 and a total energy of 1.25 X 105 MeV. In its own frame of reference, it has a lifetime of 38 nsec before it decays. Using the equations E=K+mc^2 and ##\gamma=\sqrt{1-v^2/c^2}##, it can be determined that the particle is moving at a speed close to the speed of light, with a value of ##\gamma
  • #1
Rapier
87
0

Homework Statement


Pions are part of a class of short-lived particles called mesons which commonly created during the collisions in scientific accelerators or when cosmic rays collide with particles in the upper part of the Earth's atmosphere. A type of pion known as a π+ has a mass of 139.6 MeV/c2. One particular π+ was created during a collision in the Earth's upper atmosphere and has an total energy E= 1.25 X 105 MeV. As measured in its own frame, it has a life time of 38 nsec before it decays.
a) If it decays at a point 146 meters above sea-level, how high above sea-level was the comsic-ray collision that created the pion?

hcollision = m
255345.052163 NO

HELP: Provide this information in the frame of reference of an observer on earth.
HELP: How are the total energy and mass of an object related?

b) How long does the particle live in the frame of reference of an observer on earth??
Δtearth = nsec

c) In the frame of reference of the pion, how far does it traveled before it decayed?
Δxπ = m *
11.39 OK

Homework Equations


d ' = dγ
γ = sqrt (1 - v^2/c^2)
E = K - mc^2
K = mc^2[(1/γ)-1]

The Attempt at a Solution


I used total energy + rest energy (E + mc^2) = kinetic energy (K). When I solved K for V I found that the particle was moving nearly at the speed of light. .999999999004c (that's 9 9s).

I used that speed to calculate my γ = 4.46318e-5.

d' = dγ
11.39m = d (4.46318e-5)
d = 255199.052163 m

The particle decayed 146m about sea level so d+146 = 255345.052163.

But it tells me no, so I believe the error might have come in calculating my V. If I can get A, B will be no problem...but I'm stuck.

Help! Thanks!
 
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  • #2
You have a sign error in one of your equations. The total energy is the sum of the rest energy and the kinetic energy.

Your value for ##\gamma## can't possibly be correct since ##\gamma \ge 1##.
 
  • #3
vela said:
You have a sign error in one of your equations. The total energy is the sum of the rest energy and the kinetic energy.

Your value for ##\gamma## can't possibly be correct since ##\gamma \ge 1##.

I corrected my sign error: E = k + mc^2. However, that doesn't really change anything. My energy is 1.25e5 and the 139.6 MeV of mass isn't making any appreciable change in my kinetic energy. I'm getting the same answer.
 
  • #4
What are you getting for ##\gamma##? You should get ##\gamma=895##.
 
Last edited:
  • #5



I can confirm that your calculations for part (a) are correct. The error may have come from rounding off your calculated speed, which could have affected your calculated value for γ. Try using more significant figures in your calculations to see if that makes a difference. Additionally, make sure that your units are consistent throughout your calculations.

For part (b), the particle's lifetime in the frame of reference of an observer on Earth can be calculated using the formula Δtearth = γΔtπ, where Δtπ is the lifetime of the pion in its own frame of reference. Using the value for γ that you calculated in part (a), you can find the particle's lifetime in the Earth frame of reference.

For part (c), the distance traveled in the pion's own frame of reference can be calculated using the formula Δxπ = vΔtπ, where v is the speed of the pion as calculated in part (a). This will give you the distance traveled before the pion decays.

Remember to check your units and use appropriate significant figures throughout your calculations. Keep up the good work!
 

1. What is special relativity?

Special relativity is a theory proposed by Albert Einstein in 1905 that explains how objects move in space and time. It states that the laws of physics are the same for all observers in uniform motion, and that the speed of light is constant in all inertial reference frames.

2. How does special relativity relate to decaying particles?

Special relativity predicts that particles moving at high speeds will experience time dilation, where time appears to slow down for the particle compared to an observer at rest. This means that particles with short lifetimes, such as decaying particles, may appear to live longer to an observer moving at high speeds.

3. What is the difference between special relativity and general relativity?

Special relativity only applies to objects moving at constant speeds in a straight line, while general relativity also takes into account the effects of gravity and accelerated motion. General relativity is a more comprehensive theory that builds upon the principles of special relativity.

4. How are decaying particles studied in special relativity?

Decaying particles are studied using equations derived from special relativity, such as the time dilation formula. Scientists can also use particle accelerators to study the behavior of particles moving at high speeds, and compare their results to predictions made by special relativity.

5. What are some practical applications of special relativity and decaying particles?

Special relativity and the study of decaying particles have practical applications in fields such as particle physics, nuclear medicine, and astrophysics. They have also contributed to the development of technologies such as GPS systems, which rely on precise measurements of time and space. Understanding these concepts also allows scientists to make more accurate predictions and calculations in various areas of research.

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