  We investigate the thermodynamics of the Schwarzschild-Tangherlini black hole
in the context of the generalized uncertainty principle (GUP). The corrections
to the Hawking temperature, entropy and the heat capacity are obtained via the
modified Hamilton-Jacobi equation. These modifications show that the GUP
changes the evolution of the Schwarzschild-Tangherlini black hole. Specially,
the GUP effect becomes susceptible when the radius or mass of the black hole
approaches the order of Planck scale, it stops radiating and leads to black
hole remnant. Meanwhile, the Planck scale remnant can be confirmed through the
analysis of the heat capacity. Those phenomena imply that the GUP may give a
way to solve the information paradox. Besides, we also investigate the
possibilities to observe the black hole at the Large Hadron Collider (LHC), and
the results demonstrate that the black hole cannot be produced in the recent
LHC.
