  We describe a model of tidal disruption events (TDEs) with input physical
parameters that include the black hole (BH) mass $M_{\bullet}$, the specific
orbital energy $E$, the angular momentum $J$, the star mass $M_{\star}$ and
radius $R_{\star}$. We calculate the rise time of the TDEs, the peak bolometric
luminosity in terms of these physical parameters and a typical light curve of
TDEs for various All Sky Survey (ASS) and Deep Sky Survey (DSS) missions. We
then derive the expected detection rates and discuss the follow up of TDEs
through observations in various spectral bands from X-rays to radio
wavelengths.
