We report on a search for gravitational waves from the coalescence of compact binaries during the third and fourth LIGO science runs. The search focused on gravitational waves generated during the inspiral phase of the binary evolution. In our analysis, we considered three categories of compact binary systems, ordered by mass: (i) primordial black hole binaries with masses in the range 0.35M⊙
Abbott, B., et al. “Search for Gravitational Waves from Binary Inspirals in S3 and S4 LIGO Data.” Physical Review D, vol. 77, no. 6, American Physical Society, Mar. 2008, p. 062002, doi:10.1103/PhysRevD.77.062002.
Physical Review D
©2008 American Physical Society. Original published version available at https://doi.org/10.1103/PhysRevD.77.062002