Radiatively enhanced elasticity and turbulence in clumpy tori of Active Galactic Nuclei

Abstract

The paper assumes radiation forces proportional to distance between equal temperature clouds. However, we assume there are clouds in any direction. The forces then cancel almost entirely, besides small velocity effects. Therefore, the presented theory is inadequate.

10 pages, 5 figures, accepted by MNRAS, this paper has been withdrawn by the authors due to an essential flaw in the assumptions