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Symmetry Principles and Conservation Laws in Atomic and ...

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GENERAL ARTICLEask if the conservation pr<strong>in</strong>ciples are consequences of thelaws of Nature, or, rather the laws of Nature are consequencesof the symmetry pr<strong>in</strong>ciples that govern them?Until E<strong>in</strong>ste<strong>in</strong>'s special theory of relativity, it was believedthat conservation pr<strong>in</strong>ciples are the result of thelaws of Nature. S<strong>in</strong>ce E<strong>in</strong>ste<strong>in</strong>'s work, however, physicistsbegan to analyze the conservation pr<strong>in</strong>ciples asconsequences of certa<strong>in</strong> underly<strong>in</strong>g symmetry considerationsfrom which they could be deduced, enabl<strong>in</strong>gthe laws of Nature to be revealed from this analysis.Wigner's profound impact on physics is that his explanationsof symmetry considerations us<strong>in</strong>g `group theory'resulted <strong>in</strong> a change <strong>in</strong> the very perception of just whatis most fundamental, <strong>and</strong> physicists began to regard`symmetry' as the most fundamental entity whose formwould govern the physical laws. Wigner was awardedthe 1963 Nobel Prize <strong>in</strong> Physics for these <strong>in</strong>sights [3].The conservation of l<strong>in</strong>ear <strong>and</strong> angular momentum weillustrated above are consequences of <strong>in</strong>variance undercont<strong>in</strong>uous displacements <strong>and</strong> rotations respectively <strong>in</strong>homogenous <strong>and</strong> isotropic space. Likewise, the conservationof energy is a consequence of <strong>in</strong>variance undercont<strong>in</strong>uous temporal displacement.A detailed exposition of the govern<strong>in</strong>g symmetry pr<strong>in</strong>ciplesrequires group theoretical methods, <strong>and</strong> is clearlybeyond the scope of this article, but we cont<strong>in</strong>ue to dwellon some other k<strong>in</strong>ds of symmetries now <strong>and</strong> exam<strong>in</strong>etheir connections with conservation pr<strong>in</strong>ciples.Figure 1. Masters of symmetry.5. Dynamical <strong>Symmetry</strong>: Laplace{Runge{LenzVectorIt is well known that <strong>in</strong> the classical two-body Keplerproblem (gravitational Sun{Earth system, or the Coulombicproton{electron planetary model of the old-quantumtheoryof the hydrogen atom), both energy <strong>and</strong> angularmomentum are conserved. We have already discussedRefer to Resonance issues on:E<strong>in</strong>ste<strong>in</strong>, Vol.5, March <strong>and</strong> April2000.Noether, Vol.3,September 1998.Wigner, Vol.14, October 2009.RESONANCE September 2010839

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