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v2009.01.01 - Convex Optimization

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5.4. EDM DEFINITION 361<br />

ten affine equality constraints in all on a Gram matrix G∈ S 6 (820). Let’s<br />

realize this as a convex feasibility problem (with constraints written in the<br />

same order) also assuming 0 geometric center (819):<br />

find<br />

D∈S 6 h<br />

−V DV 1 2 ∈ S6<br />

subject to tr ( )<br />

D(e i e T j + e j e T i ) 1 2 = l<br />

2<br />

ij , j−1 = (i = 1... 6) mod 6<br />

tr ( − 1V DV (A 2 i + A T i ) 2) 1 = cos ϕi , i = 1, 2, 3<br />

tr(− 1 2 V DV ) = 1<br />

−V DV ≽ 0 (832)<br />

where, for A i ∈ R 6×6 (827)<br />

A 1 = (e 1 − e 6 )(e 3 − e 4 ) T /(l 61 l 34 )<br />

A 2 = (e 2 − e 1 )(e 4 − e 5 ) T /(l 12 l 45 )<br />

A 3 = (e 3 − e 2 )(e 5 − e 6 ) T /(l 23 l 56 )<br />

(833)<br />

and where the first constraint on length-square l 2 ij can be equivalently written<br />

as a constraint on the Gram matrix −V DV 1 via (829). We show how to<br />

2<br />

numerically solve such a problem by alternating projection inE.10.2.1.1.<br />

Barvinok’s Proposition 2.9.3.0.1 asserts existence of a list, corresponding<br />

to Gram matrix G solving this feasibility problem, whose affine dimension<br />

(5.7.1.1) does not exceed 3 because the convex feasible set is bounded by<br />

the third constraint tr(− 1 V DV ) = 1 (823).<br />

<br />

2<br />

5.4.2.2.3 Example. Kissing-number of sphere packing.<br />

Two nonoverlapping Euclidean balls are said to kiss if they touch. An<br />

elementary geometrical problem can be posed: Given hyperspheres, each<br />

having the same diameter 1, how many hyperspheres can simultaneously<br />

kiss one central hypersphere? [345] The noncentral hyperspheres are allowed,<br />

but not required, to kiss.<br />

As posed, the problem seeks the maximal number of spheres K kissing<br />

a central sphere in a particular dimension. The total number of spheres is<br />

N = K + 1. In one dimension the answer to this kissing problem is 2. In two<br />

dimensions, 6. (Figure 7)<br />

The question was presented in three dimensions to Isaac Newton in the<br />

context of celestial mechanics, and became controversy with David Gregory<br />

on the campus of Cambridge University in 1694. Newton correctly identified

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