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    1. WaTTacK 23 months ago | reply

      Well, nice pic indeed. But why is the circled part so? I mean where does (1+(gamma²/2)+...) come from?
      (I have not studied relativity that much, I am just curious. But then again I think it is more of a mathematical approssimation which anyway I don't get.)

    2. zugaldia 23 months ago | reply

      That's the Lorentz Factor ( What this development does is bringing a "classic" equation for the kinetic energy from a relativistic equation (top left). The only assumption is that velocity is way smaller than the speed of light (v << c, that is gamma << 1). Hope it helps.

    3. WaTTacK 23 months ago | reply

      Ok, that's great. Thanks. I did read the link, without actually grasping a lot of it though (silly me).
      The part of the picture that troubles me is when you go from [(1-γ²)^(-1/2)] to [(1+γ²/2)+...].
      I do have some reminiscences from physics class of the first substitutions in the first two rows, but I don't get that particular approximation.
      Is there any chance you could explain it simply to a physics noob like me?

    4. zugaldia 23 months ago | reply

      Not a problem. That's called a Taylor series approximation ( Basically, when you do such an approximation, the first few terms in the series account for most of the value of the function at a particular point. In our case, we're assuming that v (velocity) is way smaller than the speed of light (this is called "classic conditions"), and so v/c is very close to zero. Therefore, we can do a Taylor series approximation "at gamma = 0".

      You can see the complete result from Wolfram Alpha (

    5. WaTTacK 23 months ago | reply

      Oh, that was it. That's why I couldn't understand it, I never studied the Taylor series.
      Thanks a lot mate!

    6. zugaldia 23 months ago | reply

      My pleasure.

    7. troncim 2 months ago | reply

      I'm so hold.

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