Bond Tension
?
In astrophysics, early accretion is driven by microscopic interactions like surface adhesion and inelastic collisions. As bodies grow, self-gravity becomes the primary binding force.
This simulation condenses these complex cohesive processes into a single parameter: "Bond Tension". It models internal tensile strength and structural cohesion — the ability to resist deformation and fragmentation.
High tension helps objects maintain structural integrity, while low tension makes them vulnerable to the black hole's tidal shear forces once they cross their effective Roche limit.