Search for Gravitational Waves from Binary Inspirals in S3 and S4 LIGO Data

Authors

• B. Abbott, California Institute of Technology
• R. Abbott, California Institute of Technology
• R. Adhikari, California Institute of Technology
• J. Agresti, California Institute of Technology
• P. Ajith, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
• B. Allen, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
• R. Amin, Louisiana State University
• S. B. Anderson, California Institute of Technology
• W. G. Anderson, University of Wisconsin-Milwaukee
• M. Arain, University of Florida
• M. Araya, California Institute of Technology
• H. Armandula, California Institute of Technology
• M. Ashley, The Australian National University
• S. Aston, University of Birmingham
• P. Aufmuth, Gottfried Wilhelm Leibniz Universität Hannover
• C. Aulbert, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
• S. Babak, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
• S. Ballmer, California Institute of Technology
• H. Bantilan, Carleton College, USA
• B. C. Barish, California Institute of Technology
• C. Barker, LIGO Hanford
• D. Barker, LIGO Hanford
• B. Barr, University of Glasgow
• P. Barriga, The University of Western Australia
• M. A. Barton, University of Glasgow
• K. Bayer, Massachusetts Institute of Technology
• K. Belczynski, Northwestern University
• J. Betzwieser, Massachusetts Institute of Technology
• P. T. Beyersdorf, San Jose State University
• B. Bhawal, California Institute of Technology
• I. A. Bilenko, Lomonosov Moscow State University
• Tiffany Z. Summerscales, Andrews UniversityFollow

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