  We try to study the thermodynamical features of a non-commutative inspired
Schwarzschild-anti-deSitter black hole in the context of entropic gravity
model, particularly for the model that is employed in a broad range of scales,
from the short distances to the large distances. At small length scales, the
Newtonian force is failed because one finds a linear relation between the
entropic force and the distance. In addition, there are some deviations from
the standard Newtonian gravity at large length scales.
