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Unformatted text preview: r = ˙ θ ˆ θ d dt ˆ θ =˙ θ ˆ r Coriolis and Centrifugal . . . ±a =2 ±ω × ±v±ω × ( ±ω × ± r ) ±a =2 ω [ v r ˆ θv θ ˆ r ] + ω 2 r ˆ r Calculus and other math Z dv vv = ln  vv  + constant Z vdv Av 2 ± B = 1 2 A ln  Av 2 ± B  + constant f ( xx ) ² f ( x )+ f ± ( x )( xx )+ 1 2 f ±± ( x )( xx ) 2 + ··· ea ² 1a + 1 2 a 2 . . . a ³ 1 sin a ² a1 6 a 3 . . . a ³ 1 cos a ² 11 2 a 2 . . . a ³ 1 If b = e a then a = ln b (1p ) q ² 1qp + 1 2 q ( q1) p 2 + ··· p ³ 1 2...
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This note was uploaded on 04/29/2008 for the course PHYS 230 taught by Professor Harris during the Fall '07 term at McGill.
 Fall '07
 Harris
 Acceleration

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