A study of the gravitational wave form from pulsars II
S. R. Valluri, J. J. Drozd, F. A. Chishtie, R. G. Biggs, M. Davison, S. V. Dhurandhar, B. S. Sathyaprakash
Abstract
We present analytical and numerical studies of the Fourier transform (FT) of the gravitational wave (GW) signal from a pulsar, taking into account the rotation and orbital motion of the Earth. We also briefly discuss the Zak-Gelfand Integral Transform. The Zak-Gelfand Integral Transform that arises in our analytic approach has also been useful for Schrodinger operators in periodic potentials in condensed matter physics (Bloch wave functions).
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