Relativistic corrections to classical physics formulae

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SUMMARY

The discussion centers on the application of relativistic corrections to classical physics formulas, specifically momentum (p = mv), kinetic energy, and the Maxwell distribution of speeds. The Lorentz transformation equations are essential for ensuring these formulas remain valid under relativistic conditions. Key examples include the momentum equation modified to p = γm₀v, where γ is the Lorentz factor and m₀ is the rest mass. The conversation emphasizes the use of 4-vectors for a more natural representation of relativistic equations, moving away from the concept of relativistic mass.

PREREQUISITES
  • Understanding of Lorentz transformation equations
  • Familiarity with 4-vectors in physics
  • Knowledge of classical mechanics principles, including momentum and kinetic energy
  • Basic grasp of special relativity concepts
NEXT STEPS
  • Study the derivation and implications of 4-velocity in relativistic physics
  • Learn about the Lorentz factor (γ) and its role in relativistic equations
  • Explore the relationship between force and acceleration in relativistic contexts
  • Investigate the differences between relativistic mass and invariant mass
USEFUL FOR

Physicists, students of physics, and educators seeking to deepen their understanding of relativistic effects on classical mechanics formulas.

Positron137
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How are classical formulas in physics (such as p = mv, or kinetic energy, or maxwell distribution of speeds) treated with the appropriate relativistic correction/modification? Is it done by using the Lorentz transformation equations? Could anyone give me a few examples of relativistic corrections to classical formulae? Thanks.
 
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Positron137 said:
How are classical formulas in physics (such as p = mv, or kinetic energy, or maxwell distribution of speeds) treated with the appropriate relativistic correction/modification? Is it done by using the Lorentz transformation equations? Thanks.
Yes. The formulas must remain unchanged when subjected to the Lorentz transformation process. (But don't ask me how they actually do it.)
 
Thanks! :) yeah sometimes I get confused when looking at the classical formulas, and the relativistic version, and try to see how its done using the Lorentz stuff.
 
IMO, the best approach is to learn about 4-vectors. Typically, the relativistic formulas look natural as 4-vectors, while sometimes looking 'unnatural' in 3-vector notation.

For example, starting with 4-velocity as the derivative of (t,x,y,z) by proper time (\tau), denoted U, you have:


p = m U ; m is (rest) mass, p momentum.

A = proper acceleration = what is measured by an accelerometer = dU/d\tau

F = dp/\tau = m A

(in the above, I assume a particle whose rest mass does not change).

Note, this approach explains the disfavor of relativistic mass: there is no relativistic mass in any of the above forumulas. The factor γ is buried within U (and in a more complex way, within A).
 
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Positron137 said:
How are classical formulas in physics (such as p = mv, or kinetic energy, or maxwell distribution of speeds) treated with the appropriate relativistic correction/modification? Is it done by using the Lorentz transformation equations? Could anyone give me a few examples of relativistic corrections to classical formulae? Thanks.
The relativistic corrections to the first:

p = γ m0 v, with m0 = "rest mass" (the Newtonian mass concept which assumes that inertial effects are independent of speed had to be abandoned). As PAllen mentioned relativistic mass, it is easy to see where the concept of "relativistic mass" came from: one can bundle γm0 together as m = "relativistic mass", so that one gets again p = m v.

Further, F = dp / dt remains unchanged.

However, the relationship between force F and acceleration a - coordinate acceleration of an object as measured in an inertial system - is much more complex; that's a neat textbook exercise. :-p
See: http://en.wikipedia.org/wiki/Force#Special_relativity
 
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