  The present work examines the possibility of warm inflationary paradigm in
the modified gravity theory with fractal geometry. By choosing the normal fluid
as radiation fluid and the effective fluid (with the extra term in modified
field equation) as the inflaton field both strong and weak dissipative regimes
have been studied using slow roll approximation with quasi-stable criteria for
radiation. Finally, using the Planck data set, the present model has been
analyzed for various choices of the fractal function and the dissipation
parameter.
