How do you explain photoplanet hypothesis?

The photoplanet hypothesis suggests that planets can form in the vicinity of stars through the accumulation of dust and gas that is influenced by the star's radiation pressure and stellar wind. This process occurs in protoplanetary disks, where particles collide and stick together, gradually building up larger bodies. The hypothesis emphasizes the role of light and radiation in shaping the conditions for planet formation, particularly in how these forces can affect the distribution and stability of material in the disk. Overall, it contributes to our understanding of how various environmental factors influence the birth and evolution of planetary systems.