A Nearly Minimum Redundant Correlator Interpolation Formula for Gravitational Wave Chirp Detection

An absolute lower bound on the number of templates needed to keep the fitting factor above a prescribed minimal value $\mathrm{\Gamma }$ in correlator bank detection of (newtonian) gravitational wave chirps from unknown inspiraling compact binary sources is derived, resorting to the theory of quasi-bandlimited functions in the $L^{\mathrm{\infty }}$ norm. An explicit nearly-minimum redundant cardinal-interpolation formula for the (reduced, noncoherent) correlator is introduced. Its computational burden and statistical properties are compared to those of the plain lattice of (reduced, noncoherent) correlators, for the same $\mathrm{\Gamma }$. Extension to post-newtonian models is outlined.