At what velocity should relativity be taken into account

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SUMMARY

In discussions regarding when to consider relativity, it is established that velocities approaching 6.5 x 106 m/s are typically within the non-relativistic range. The Lorentz factor (gamma) is a critical tool for determining the necessity of relativistic corrections. If gamma is close to 1, relativistic effects can be ignored; however, if it significantly deviates from 1, special relativity (SR) must be considered. For example, at a velocity of v = c/5, gamma is approximately 1.02, indicating that relativistic effects are minimal at such speeds.

PREREQUISITES
  • Understanding of the Lorentz factor (gamma)
  • Basic knowledge of special relativity (SR)
  • Familiarity with the photoelectric effect
  • Concept of non-relativistic vs. relativistic velocities
NEXT STEPS
  • Study the derivation and implications of the Lorentz factor (gamma)
  • Explore the principles of special relativity (SR) in detail
  • Investigate the photoelectric effect and its relationship with particle velocities
  • Learn about relativistic momentum and energy calculations
USEFUL FOR

Students preparing for physics exams, educators teaching concepts of relativity, and anyone interested in the applications of special relativity in high-velocity scenarios.

moonkey
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Homework Statement


[STRIKE]I have exams coming up and I'm just looking for an idea of when relativity should be taken into account. For example I'm just going over a question involving photoelectric effect and potential fields and de Broglie and all that jazz and the final velocity of the electron turns out to be around 6.5x106ms-1. Should I take relativity into account for this velocity or is it still safely within the margins of non-relativistic velocity? I'm thinking that it is safe to assume that it is non-relativistic but I would like some advice just in case such a question arises that involves a greater velocity.[/STRIKE]

Sorry, wrong forum. Moving to introductory

Homework Equations





The Attempt at a Solution

 
Last edited:
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I think a generally good approach if you're unsure is to work out gamma (http://en.wikipedia.org/wiki/Lorentz_factor). If it's close enough to 1 that you're happy to say gamma=1 then you don't need to to consider relativistic effects. If it's different enough to 1 that you wouldn't be happy rounding it to 1, then you will want to take SR into account.

On that wikipedia page you'll notice that for v=c/5, gamma is still only 1.02, so you can get to pretty big speeds without really needing to worry about relativistic corrections.
 

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