The analysis of large order bessel functions in gravitational wave signals from pulsars

In this work, we present the analytic treatment of the large order Bessel functions that arise in the Fourier transform. (FT) of the gravitational wave (GW) signal from a pulsar. We outline several strategies, which employs asymptotic expansions in evaluation of such Bessel functions, which also happen to have large argument. Large order Bessel functions also arise in the Peters-Mathews model of binary inspiralling stars emitting GW and several problems in potential scattering theory. Other applications also arise in a variety of problems in applied mathematics as well as in the natural sciences and present a challenge for high performance computing (HPC).