  The Generalized Uncertainty Principle (GUP) is motivated by the premise that
spacetime fluctuations near the Planck scale impose a lower bound on the
achievable resolution of distances, leading to a minimum length. Inspired by a
semiclassical method that integrates the GUP into the partition function by
deforming its phase space, we induce a modification on the thermodynamic
quantities of the MIT bag model that we propose serves as an effective
semiclassical description of deconfined quark matter in a space with minimal
length. We investigate the consequences of this deformation on the
zero-temperature limit, revealing a saturation limit for the energy density,
pressure and baryon number density and an overall decrease of the thermodynamic
quantities which suggests an enhanced stability against gravitational collapse.
These findings extend existing research on GUP-deformed Fermi gases.
Ultimately, our description introduces effects of quantum gravity in the
equations of state for compact stars in a mathematically simple manner,
suggesting potential for extension to more complex systems.
