A study of the gravitational wave form from pulsars

Valluri, S. R., Drozd, J. J., Chishtie, F. A., Biggs, R. G., Davison, M., Dhurandhar, Sanjeev V. and Sathyaprakash, Bangalore Suryanarayana ORCID: https://orcid.org/0000-0003-3845-7586 2002. A study of the gravitational wave form from pulsars. Classical and Quantum Gravity 19 (7) , 1327. 10.1088/0264-9381/19/7/314

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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 and a special class of the generalized hypergeometric function of potential relevance. The Zak–Gelfand integral transform that arises in our analytic approach has also been useful for Schrödinger operators in periodic potentials in condensed matter physics (Bloch wave functions) and holds promise for the study of periodic GW signals for long integration times.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	IOP Publishing
ISSN:	0264-9381
Last Modified:	24 Oct 2022 10:46
URI:	https://orca.cardiff.ac.uk/id/eprint/45828

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