By assumption of a low-energy string theory in
addition to the necessity of the semi-classic expansion on
action, we study Hawking temperature and entropy of Kerr-
Sen black hole. These subjects, recently have introduced in
the literature and consist of the new terms of temperature
and entropy as the expansion form with powers of h. Comparing
the results with the high energy black hole demonstrates
how the semi-classic approximation affects the thermodynamics
of the Kerr-Sen black hole, corrected terms
classical action and the entropy.
کلید واژگان :
Hawking temperature · Plank constant · Corrected entropy · Action
