Relativistic Velocity: Speed Limits & Ranges Explained

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    Relativistic Velocity
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SUMMARY

Relativistic velocity refers to speeds where relativistic effects become significant, particularly when the Lorentz factor, γ, is substantially greater than 1. For instance, at v=0.1c (10% of the speed of light), γ is approximately 1.005, which is not considered significantly larger than 1 for practical purposes. However, for applications like GPS satellites, where velocities are relativistic, these effects must be accounted for to ensure accurate positioning. The kinetic energy of a particle is defined as E_{kin.}=(γ -1)mc², and deviations from classical kinetic energy necessitate the use of relativistic formulas when speeds approach significant fractions of the speed of light.

PREREQUISITES
  • Understanding of Lorentz factor (γ) in special relativity
  • Basic knowledge of kinetic energy equations
  • Familiarity with the speed of light (c) and its implications
  • Concept of time dilation in relativistic physics
NEXT STEPS
  • Study the implications of relativistic effects on GPS technology
  • Explore the derivation and applications of the Lorentz factor (γ)
  • Learn about relativistic corrections to classical mechanics
  • Investigate the series expansion of relativistic equations for practical applications
USEFUL FOR

Physicists, aerospace engineers, and students of relativity seeking to understand the implications of relativistic velocities and their effects on energy and time dilation in high-speed contexts.

nelufar
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Which velocity can be said to be relativistic velocity? I mean is there any range beyond which velocities can be called as relativistic velocities?
 
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All velocities are relativistic, but relativistic effects will not be easily noticeable until the speed is large enough to make

\gamma=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}

(where v is the speed, and c is the speed of light)

significantly larger than 1.

An example: suppose that v=0.1c, i.e. 10% of the speed of light. Then gamma is about 1.005. Is that significantly larger than 1? That depends on that you're doing. Sometimes a 0.5% correction to the non-relativistic result isn't important, and sometimes it is.
 
Is same true for relativistic energies also?
 
The kinetic energy of a particle is E_{kin.}=(\gamma -1)mc^2 if this deviates substantially from classical kinetic energy you should use the relativistic result.

So you could use as a criterium: if 2 (\gamma -1)c^2/v^2 is significantly larger than 1 you deal with relativistic velocities...
 
Consider the orbital speed of a satellite or spacecraft : ~17,000mph. For an astronaut, this is not a relativistic velocity, meaning he won't notice the time dilation on his watch from takeoff to landing. For a GPS satellite, however, this is a relativistic velocity and must be accounted for in its functioning in order for GPS positions to be accurate.
 
nelufar said:
Is same true for relativistic energies also?
To see the answer to your question it helps to use the series expansion

\frac{1}{\sqrt{1-x}}=1+\frac{1}{2}x+\frac{3}{8}x^2+\frac{5}{16}x^3+\dots

The kinetic energy is

(\gamma-1)mc^2=\bigg(1+\frac{1}{2}\bigg(\frac{v^2}{c^2}\bigg)+\frac{3}{8}\bigg(\frac{v^2}{c^2}\bigg)^2+\frac{5}{16}\bigg(\frac{v^2}{c^2}\bigg)^3+\dots-1\bigg)mc^2=\frac12mv^2\bigg(1+\frac34\bigg(\frac{v^2}{c^2}\bigg)+\frac58\bigg(\frac{v^2}{c^2}\bigg)^2+\dots\bigg)

Note that the first term after the last equality sign is just the non-relativistic kinetic energy. The other terms are relativistic corrections to the non-relativistic result. If the speed is large enough these terms can't be ignored.
 

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