A study of the gravitational wave form from pulsars II
Astrophysics
2009-11-07 v1
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).
Keywords
Cite
@article{arxiv.astro-ph/0110626,
title = {A study of the gravitational wave form from pulsars II},
author = {S. R. Valluri and J. J. Drozd and F. A. Chishtie and R. G. Biggs and M. Davison and S. V. Dhurandhar and B. S. Sathyaprakash},
journal= {arXiv preprint arXiv:astro-ph/0110626},
year = {2009}
}
Comments
6 pages, Sparkler talk given at the Amaldi Conference on Gravitational waves, July 10th, 2001. Submitted to Classical and Quantum Gravity