We investigate critical phenomena during the gravitational collapse of a massive scalar field under two distinct semiclassical loop quantum gravity (LQG) approaches within spherical symmetry. Numerical simulations reveal that the massive scalar field in both semiclassical frameworks exhibits two distinct types of critical behavior, consistent with the classical scenario. When the scalar field’s mass parameter is small, type II critical phenomena emerge, with the resulting echoing periods and critical exponents precisely matching those obtained in general relativity. In contrast, a large mass parameter triggers type I critical phenomena, where the resulting black holes possess a finite minimum mass. These findings suggest that semiclassical corrections from LQG have a negligible impact on the dynamics of critical collapse.

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• Alternative gravity theories
• Loop quantum gravity