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of pairs which are near each other in φ (40 ◦ to 48 ◦ ) they all together pick up the bubble correlation and thus these pairs of pairs over all show about a 0.4% correlation. In the -4.0 < Δ P $^{t}$1 +Δ P $^{t}$2 < -1.0 region the correlation increases from 0.4% to 1%, while in the 1.0 < Δ P $^{t}$1 + Δ P $^{t}$2 < 4.0 region the correla- tion decreases from 0.4% to -0.2%. This means the pairs of pairs are anti-aligned at a higher rate than aligned. This anti-alignment is what is predicted by the color magnetic field effect presented above. In fact the anti-alignment increases with p t as the ratio bubble particle to background increases. However these predicted color magnetic effects have not been searched for yet and therefore there is no experimen- tal evidence for them. Experimental investigations of STAR TPC detector charged particle correlations provide a method of obtaining experimental confir- mation of the anti-alignment caused by the color 

magnetic field. 

## VIII. SUMMARY AND DISCUSSION 

In this article we summarize the assumptions made and the reasoning that led to the develop- ment and construction of our parton bubble model (PBM)[6], which successfully explained the charge- particle-pair correlations in the central (0-10% cen- trality) √ s NN = 200 GeV Au Au data[12]. The PBM is also consistent with the Au Au central col- lision HBT results. This is presented and discussed in Sec. 4 of Ref.[6] and Sec. I and II of this pa- per. In Sec. III we discussed extending our model, which was a central collision model, to be able to treat the geomery of bubble production for 0-80% collision centralities (PBME[13]) such as measured 

