7 Corr  (DEG) Correlation p$_{t}$ greater 0.8 and less 2.0 GeV/c STAR Au Au Central 200 GeV Soft modified HIJING AuAu 200 GeV  B 0.0 to 4.0 bubbles added  0.0   0.3  0.3   0.6  0.6   0.9  0.9   1.2  1.2   1.5 FIG. 5: In each of the five labeled Δ η bins we show the Δ φ total correlation for the CI as a function of Δ φ . The STAR Au + Au central trigger analysis results from the formulae of Ref.[12] are shown as a solid line. The parton bubble model predictions are shown by the circular points(o) which are large enough to include the statistical errors from a 2 million event sample. The vertical correlation scale is not offset and is correct for the largest Δ η bin, 1.2 < Δ η < 1.5, and is the lowest bin on the figure. As one proceeds upwards to the next bin Δ η the correlation is offset by +0.01. This is added to the correlation of each subsequent Δ η bin. The smallest Δ η and top of Figure 12 has a +0.04 offset. A solid straight horizontal line shows the offset for each Δ η bin. Each solid straight horizontal line is at 1.0 in correlation strength. The 0-10% centrality in HIJING corresponds to impact parameter (b) range 0.0 to 4.0 fm. The agreement is very good. IV. GLASMA FLUX TUBE MODEL size of 1/ Q s . Q s is the saturation momentum of par- tons in the nuclear wavefunction. These longitudinal color electric and magnetic fields generate topologi- cal Chern-Simons charge[21] which becomes a source for particle production. The transverse space is filled with flux tubes of large longitudinal extent but small transverse size ∼ Q $_{−}$1 s . Particle production from a flux tube is a Poisson process, since the flux tube is a coherent state. As the partons emitted from these flux tubes locally equilibrate, transverse flow builds due to the radial flow of the blast wave[22]. The flux tubes that are near the surface of the fireball get the largest A glasma flux tube model (GFTM)[17] that had been developed considers that the wavefunctions of the incoming projectiles, form sheets of color glass condensates (CGC)[18] that at high energies collide, interact, and evolve into high intensity color elec- tric and magnetic fields. This collection of primor- dial fields is the Glasma[19, 20], and initially it is composed of only rapidity independent longitudinal color electric and magnetic fields. An essential fea- ture of the Glasma is that the fields are localized in the transverse space of the collision zone with a