Gravitational lensing of gravitational waves from merging neutron star binaries
Abstract
We discuss the gravitational lensing of gravitational waves from merging neutron star binaries, in the context of advanced LIGO type gravitational wave detectors. We consider properties of the expected observational data with cut on the signal-to-noise ratio \rho, i.e., \rho>\rho_0. An advanced LIGO should see unlensed inspiral events with a redshift distribution with cut-off at a redshift z_{\rm max} < 1 for h \leq 0.8. Any inspiral events detected at z>z_{\rm max} should be lensed. We compute the expected total number of events which are present due to gravitational lensing and their redshift distribution for an advanced LIGO in a flat Universe. If the matter fraction in compact lenses is close to 10\%, an advanced LIGO should see a few strongly lensed events per year with \rho >5.
- Authors:
-
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Princeton Univ., Princeton, NJ (United States)
- Publication Date:
- Research Org.:
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1155593
- Report Number(s):
- FERMILAB-PUB-96-091-A
Journal ID: ISSN 0031-9007; PRLTAO
- DOE Contract Number:
- AC02-07CH11359
- Resource Type:
- Journal Article
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Volume: 77; Journal Issue: 14; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Wang, Yun, Stebbins, Albert, and Turner, Edwin L. Gravitational lensing of gravitational waves from merging neutron star binaries. United States: N. p., 1996.
Web. doi:10.1103/PhysRevLett.77.2875.
Wang, Yun, Stebbins, Albert, & Turner, Edwin L. Gravitational lensing of gravitational waves from merging neutron star binaries. United States. https://doi.org/10.1103/PhysRevLett.77.2875
Wang, Yun, Stebbins, Albert, and Turner, Edwin L. 1996.
"Gravitational lensing of gravitational waves from merging neutron star binaries". United States. https://doi.org/10.1103/PhysRevLett.77.2875. https://www.osti.gov/servlets/purl/1155593.
@article{osti_1155593,
title = {Gravitational lensing of gravitational waves from merging neutron star binaries},
author = {Wang, Yun and Stebbins, Albert and Turner, Edwin L.},
abstractNote = {We discuss the gravitational lensing of gravitational waves from merging neutron star binaries, in the context of advanced LIGO type gravitational wave detectors. We consider properties of the expected observational data with cut on the signal-to-noise ratio \rho, i.e., \rho>\rho_0. An advanced LIGO should see unlensed inspiral events with a redshift distribution with cut-off at a redshift z_{\rm max} < 1 for h \leq 0.8. Any inspiral events detected at z>z_{\rm max} should be lensed. We compute the expected total number of events which are present due to gravitational lensing and their redshift distribution for an advanced LIGO in a flat Universe. If the matter fraction in compact lenses is close to 10\%, an advanced LIGO should see a few strongly lensed events per year with \rho >5.},
doi = {10.1103/PhysRevLett.77.2875},
url = {https://www.osti.gov/biblio/1155593},
journal = {Physical Review Letters},
issn = {0031-9007},
number = 14,
volume = 77,
place = {United States},
year = {Wed May 01 00:00:00 EDT 1996},
month = {Wed May 01 00:00:00 EDT 1996}
}