  We study the feasibility of realizing supersymmetric new inflation model,
introduced by Senoguz and Shafi in [1], for $SU(5)$ and flipped $SU(5)$ models
of grand unified theories (GUTs). This realization requires an additional
$U(1)_R \times Z_{n}$ symmetry for its successful implementation. The standard
model (SM) gauge singlet scalar components of $24_H$ and $10_H$ GUT Higgs
superfields are respectively employed to realize successful inflation in
$SU(5)$ and flipped $SU(5)$ models. The predictions of the various inflationary
observables lie within the recent Planck bounds on the scalar spectral index,
$n_s$, for $n \geq 5$ in $SU(5)$ model and for $n \geq 6$ in flipped $SU(5)$
model. In particular, the tensor to scalar ratio $r$ and the running of
spectral index $d n_s/ d\ln k$ are negligibly small and lie in the range,
$10^{-12} \lesssim r \lesssim 10^{-8}$ and $10^{-9} \lesssim dn_s/d\ln k
\lesssim 10^{-3}$, for realistic values of $n$. In numerical estimation of the
various predictions, we fix the gauge symmetry breaking scale, $M$, around $2
\times 10^{16}$ GeV. The issue of gauge coupling unification in $R$-symmetric
$SU(5)$ is evaded by adding vectorlike families with mass splitting within
their multiplets. The dilution of monopoles beyond the observable limit is
naturally achieved in the breaking of $SU(5)$ gauge symmetry during inflation.
A realistic scenario of reheating with non-thermal leptogenesis is employed for
both models. The predicted range of reheat temperature within Planck bounds, $3
\times 10^{7}\text{ GeV }\lesssim T_r \lesssim 2 \times 10^{9}$ GeV, is safe
from the gravitino problem for the gravitino mass, $m_{3/2} \gtrsim 10$ TeV.
Finally, the $U(1)_R \times Z_{n}$ symmetry is also observed to play a crucial
role in suppressing the various fast proton decay operators.
