Relativistic and not relativistic motions

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SUMMARY

The discussion focuses on the distinction between relativistic and non-relativistic motions, specifically highlighting the equations x=gtt/2 for non-relativistic motion and x=cc/g(coshgt'/c-1) for relativistic motion. It is established that non-relativistic motion can result in velocities exceeding the speed of light (c), while relativistic motion maintains |v(t)| < c. The conversation also emphasizes the importance of integrating dp/dt=f(t) to derive relativistic motions and discusses the implications of the SR velocity addition formula on resultant velocities.

PREREQUISITES
  • Understanding of special relativity concepts, particularly velocity addition.
  • Familiarity with calculus, specifically integration techniques.
  • Knowledge of relativistic momentum and its mathematical representation.
  • Basic principles of uniformly accelerated motion.
NEXT STEPS
  • Study the derivation of relativistic momentum using the formula p=mv/√(1-v²/c²).
  • Explore the implications of the SR velocity addition formula in various scenarios.
  • Investigate the mathematical integration of dp/dt=f(t) for different functions f(t).
  • Learn about the physical interpretations of acceleration as velocity approaches the speed of light.
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Physicists, students of advanced mechanics, and anyone interested in the principles of special relativity and motion dynamics.

bernhard.rothenstein
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We say that the uniformly accelerated motion x=gtt/2 is not a relativistic motion because after a sufficiently long time of motion v=gt can exceed c. we say that x=cc/g(coshgt'/c-1) is a relativistic motion because the velocity of the motion it describes never becomes c. Do you know other such "relativistic motions?"
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Just integrate dp/dt=f(t) for any function f(t), and you will have a
"relativistic motion". If you want x(t), just find v=dx/dt from
v=p/\sqrt{p^2+m^2}, and integrate.
 
Alternately, given any function v(t) < c, one can compute the acceleration required to cause the specified motion. The only thing "special" about special relativistic motion is that |v(t)| < 1. One can also show that the rate of change of momentum with respect to time becomes infinite as v->c, i.e.

[tex] \frac{dp}{dt} = \frac{dp}{dv} \frac{dv}{dt} = \frac{m}{{\left( 1 - \frac{v^2}{c^2} \right)} ^ \frac{3}{2}} \frac{dv} {dt}[/tex]

Thus as v->c, dp/dt becomes infinite.

One does not really need dynamics to see this, the fact is that if one adds together any number of velocities less than 'c' using the SR velocity addition formula, one gets a resultant velocity less than 'c'.

The process of accelerating is just a process of "adding to" one's original velocity. One must use the SR form of the velocity additon law.

Delta-v = a * delta t

is true only in the objects rest frame, the SR velocity additon formula converts the delta-v in the objects rest frame into the delta-v in the coordinate frame.
 
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