Physics 325 Lecture 4 - Physics 325 Lecture 4 Frames of...

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Physics 325 Lecture 4 Frames of Reference We referred above to an “inertial reference frame”. What do we mean by this? An inertial reference frame (IRF) is a reference frame that is not accelerating. Not accelerating with respect to what is a good question. But it turns out that just saying it is not accelerating is usually good enough – you can say “with respect to the fixed stars” if you want to pretend that the stars are fixed. A rotating reference frame is a counter example. It is clearly an accelerating reference frame since while rotating a body has centripetal acceleration. So the earth is not really an IRF, but we calculated our acceleration in Urbana in 111 and it’s pretty small, so it’s approximately an IRF. Newton’s laws are valid only in an IRF (though you can use them to derive laws in NIRFs). Furthermore, all IRFs are equivalent so we can derive a set of rules for moving G The rules that take us from S to S’ are as follows: from one frame S to another S’ that moves with respect to S at a constant velocity : 0 v S r G S’ r G 0 constant v G ( ) ( ) () 0 00 Therefore rt rt v t =− GGG dd v v v dt dt dv dv aa dt dt Fm aF m a ′′ = −→= =→ = === GG G G (4.1) The last two equations in (4.1) show that Newton’s laws remain unchanged if we move from one IRF to another. This is known as Galilean invariance, and it is due to the fact that Newton’s 2 nd law involves a derivative of the velocity, so addition of a constant velocity drops out.
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Equation of motion o a large extent, our job in classical mechanics is to determine the equation of motion T
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Physics 325 Lecture 4 - Physics 325 Lecture 4 Frames of...

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