  Fast Radio Bursts (FRBs) are short duration highly energetic dispersed radio
pulses. We developed a generic formalism (Bera {\em et al.}, 2016) to estimate
the FRB detection rate for any radio telescope with given parameters. By using
this model, we estimated the FRB detection rate for two Indian radio telescope;
the Ooty Wide Field Array (OWFA) (Bhattacharyya {\em et al.}, 2017) and the
upgraded Giant Metrewave Radio Telescope (uGMRT) (Bhattacharyya {\em et al.},
2018) with three beam forming modes. In this review article, I summarize these
two works. We considered the energy spectrum of FRBs as a power law and the
energy distribution of FRBs as a Dirac delta function and a Schechter
luminosity function. We also considered two scattering models proposed by Bhat
{\em et al.} (2004) and Macquart \& Koay (2013) for these work and I consider
FRB pulse without scattering as a special case for this review. We found that
the future prospects of detecting FRBs by using these two Indian radio
telescopes is good. They are capable to detect a significant number of FRBs per
day. According to our prediction, we can detect $\sim 10^5-10^8$, $\sim
10^3-10^6$ and $\sim 10^5-10^7$ FRBs per day by using OWFA, commensal systems
of GMRT and uGMRT respectively. Even a non detection of the predicted events
will be very useful in constraining FRB properties.
