  In this work, we study neutron stars (NSs) in an ungravity (UG) inspired
model. We examine the UG effects on the static properties of the selected NSs,
in different mass and radius regimes, i.e., mini, moderate, and heavy NSs,
using a polytropic equation of state approach. Based on the observational data,
we obtain bounds on the characteristic length and scaling dimension of the UG
model. Furthermore, we obtain dynamic properties, such as inertial moment (I),
Love number (Love), and quadrupole moment (Q) of a slowly rotating NS in the
presence of the exterior gravity and ungravity fields. The UG model is also
examined with respect to the I-Love-Q universal relation.
