A study of the gravitational wave form from pulsars

S. R. Valluri, J. J. Drozd, F. A. Chishtie, R. G. Biggs, M. Davison, Sanjeev V. Dhurandhar, B. S. Sathyaprakash

Research output: Contribution to journalArticlepeer-review

9 Scopus citations


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 wavefunctions) and holds promise for the study of periodic GW signals for long integration times.

Original languageEnglish (US)
Pages (from-to)1327-1334
Number of pages8
JournalClassical and Quantum Gravity
Issue number7
StatePublished - Apr 7 2002

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy (miscellaneous)


Dive into the research topics of 'A study of the gravitational wave form from pulsars'. Together they form a unique fingerprint.

Cite this