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2. In classical mechanics, we learned that particles undergoing some sort of orbital or circular motion have angular momentum(a) But first, a little more classical mechanics. Suppose a classical particle is moving in the x, y-plane. One thing you may(c) Now that you are convinced that the commutator algebra of position and mo- mentum extends nicely to higher dimensions, le

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Q: W02 i = txÞ solution (a): alva Dz - «ру - . — Now we make a change of variables - x = xcoso-gsing ; Py = pu coso - pý siLLUNOMIC BUREAU SALOTO į = x py cos²e + x pų siuze - ypé sluRo -y kú cos²g z = x pé ( cos²ot sin²o) - y pů (sino + cos²o7 whlor AIS 20 Latet Compute the commutators- (i) [[z, ? ] = ? • iz = .By - fe i ( ₂ , &. 3. = [ ê By ĝ for x] (lz, n] = [upy , nexchange has Darification from non-disce thy - According man Nar en not avail hor tion р- 4 (1) CL + ) = (х + - + P , 2) = (х(m) [Lz, Pe] = [lz, Pu] = (lze ku] = [xpy - y Pes px] [xpy, Pu] - [ykus Pe] x (by , Pe] + [x, Pu] by -yl Pu, Px] - [y, Pu] Pe

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