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Through the ATOMIUM project, based on an ALMA large program, we aim to present a consistent view of a sample of 17 nearby cool evolved stars (Aymptotic Giant Branch and red supergiant stars).\n  Methods. Here we present VLT/SPHERE-ZIMPOL polarimetric maps obtained in the visible of 14 out of the 17 ATOMIUM sources. They were obtained contemporaneously with the ALMA high spatial resolution data. To help interpret the polarized signal, we produced synthetic maps of light scattering by dust, through 3D radiative transfer simulations with the RADMC3D code.\n  Results. The degree of linear pola","authors_text":"A. Baudry, A. de Koter, A. M. S. Richards, A. Zijlstra, B. Pimpanuwat, C. A. Gottlieb, D. Gobrecht, E. Cannon, E. Lagadec, F. De Ceuster, F. Herpin, H. S. P. M\\\"uller, I. El Mellah, I. McDonald, J. Bolte, J. Malfait, J. M. C. Plane, J. Yates, K. M. Menten, K. T. Wong, L. B. F. M. Waters, L. Decin, M. D. Gray, M. Jeste, M. Montarg\\`es, M. Van de Sande, P. Kervella, R. Sahai, S. 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