Search for gravitational waves from binary inspirals in S3 and S4 LIGO data

Authors

B. P. Abbott
R. Abbott
Mario C. Diaz, The University of Texas Rio Grande ValleyFollow
R. Grosso
Soumya Mohanty, The University of Texas Rio Grande ValleyFollow
Soma Mukherjee, The University of Texas Rio Grande ValleyFollow
Cristina V. Torres, The University of Texas Rio Grande Valley

Document Type

Article

Publication Date

2008

Abstract

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⊙

Comments

©2008 American Physical Society. Original published version available at https://doi.org/10.1103/PhysRevD.77.062002

Recommended Citation

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.

Publication Title

Physical Review D

DOI

10.1103/PhysRevD.77.062002