Document Type
Article
Publication Date
3-7-2008
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
Journal Title
Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume
77
Issue
6
DOI
https://doi.org/10.1103/PhysRevD.77.062002
First Department
Physics
Recommended Citation
Abbott, B.; Abbott, R.; Adhikari, R.; Agresti, J.; Ajith, P.; Allen, B.; Amin, R.; Anderson, S. B.; Anderson, W. G.; Arain, M.; Araya, M.; Armandula, H.; Ashley, M.; Aston, S.; Aufmuth, P.; Aulbert, C.; Babak, S.; Ballmer, S.; Bantilan, H.; Barish, B. C.; Barker, C.; Barker, D.; Barr, B.; Barriga, P.; Barton, M. A.; Bayer, K.; Belczynski, K.; Betzwieser, J.; Beyersdorf, P. T.; Bhawal, B.; Bilenko, I. A.; and Summerscales, Tiffany Z., "Search for Gravitational Waves from Binary Inspirals in S3 and S4 LIGO Data" (2008). Faculty Publications. 1994.
https://digitalcommons.andrews.edu/pubs/1994
Acknowledgements
Retrieved March 8, 2021 from https://arxiv.org/pdf/0704.3368.pdf