The gravitational wave pulsar signal with Jovian and lunar perturbations and orbital eccentricity corrections

Details The gravitational wave pulsar signal with Jovian and lunar perturbations and orbital eccentricity corrections The gravitational wave pulsar signal with Jovian and lunar perturbations and orbital eccentricity corrections

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cqgra..23.3323v&link_type=abstract

Classical and Quantum Gravity, Volume 23, Issue 10, pp. 3323-3332 (2006).

Physics

2

Scientific paper

In this work, we present the analytic treatment of the Fourier transform (FT) of the gravitational wave (GW) signal from a pulsar in a parametrized model discussed by Brady et al (1998 Phys. Rev. D 57 2101). The formalism lends itself to a development of the FT that accounts for the corrections due to the orbital eccentricity, and the Jovian and lunar perturbations in terms of well-known special functions.

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