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We investigate clusters of misaligned (inclined) tori orbiting a centralstatic Schwarzschild black hole. To this purpose we considered a set ofgeometrically thick, pressure supported, perfect fluid tori analyzing purelyhydrodynamic models. We study the tori collision emergence and, consequently,the stability properties of the aggregates composed by tori with differentinclination angles relative to a fixed distant observer. The aggregate oftilted tori is modeled as a single orbiting configuration, by introducing aleading function governing the distribution of toroids around the black holeattractor. Eventually the tori agglomerate can be seen, depending on the torithickness, as a (multipole) gobules of orbiting matter, with different toroidalspin orientations , covering the embedded central black hole. These systems areshown to include tori with emerging instability phase related to accretion ontothe central black hole. Therefore we provide an evaluation of quantitiesrelated to tori energetics such as the mass-flux, the enthalpy-flux, and theflux thickness depending on the model parameters for polytropic fluids.Consequently this analysis places constraints on the existence and propertiesof tilted tori and aggregate of misaligned disks. Some notes are included onaggregates including proto-jets, represented by open cusped solutionsassociated to the geometrically thick tori.

Embedded BHs and multipole globules: Clustered misaligned thick accretion disks around static SMBHs