Relativistic corrections to classical physics formulae

In summary, classical formulas in physics are unchanged by the Lorentz transformation process, but the relationship between force and coordinate acceleration is more complex.
  • #1
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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  • #2
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.)
 
  • #3
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.
 
  • #4
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 ([itex]\tau)[/itex], denoted U, you have:


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

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

F = dp/[itex]\tau[/itex] = 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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  • #5
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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FAQ: Relativistic corrections to classical physics formulae

What are relativistic corrections to classical physics formulae?

Relativistic corrections refer to adjustments made to classical physics formulae in order to account for the effects of relativity, specifically the theory of special relativity. These corrections are necessary when dealing with objects moving at speeds close to the speed of light.

Why are relativistic corrections important?

Relativistic corrections are important because classical physics formulae do not accurately describe the behavior of objects moving at high speeds. These corrections allow for more accurate predictions and calculations in situations where relativistic effects are significant.

What are some common examples of relativistic corrections?

Some common examples of relativistic corrections include time dilation, length contraction, and the addition of the Lorentz factor in equations for momentum and energy. These corrections are used in various fields of physics, such as astrophysics and particle physics.

How do relativistic corrections change classical physics formulae?

Relativistic corrections typically involve adding or substituting terms in classical physics formulae to account for the effects of relativity. For example, the classical equation for kinetic energy, E = 1/2mv^2, is corrected to E = mc^2/(√(1-v^2/c^2))-1, where c is the speed of light and v is the velocity of the object.

Can relativistic corrections be ignored in everyday situations?

In most everyday situations, the effects of relativity are negligible and classical physics formulae can be used without the need for relativistic corrections. However, in situations involving high speeds, such as in space travel or particle accelerators, these corrections are necessary for accurate calculations and predictions.

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