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  Material effects in binary neutron star inspiral waveforms

Markakis, C., Read, J., Baiotti, L., Creighton, J., Giacomazzo, B., Friedman, J., et al. (2011). Material effects in binary neutron star inspiral waveforms. Bulletin of the American Physical Society, 56(4): Y12.00005.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-000E-EF7E-B Version Permalink: https://hdl.handle.net/11858/00-001M-0000-000E-EF7F-9
Genre: Conference Paper

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 Creators:
Markakis, Charalampos, Author
Read, Jocelyn, Author
Baiotti, Luca, Author
Creighton, Jolien, Author
Giacomazzo, Bruno, Author
Friedman, John, Author
Rezzolla, Luciano1, Author           
Shibata, Masaru, Author
Taniguchi, Keisuke, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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 Abstract: Tidal effects due to the presence of matter in binary neutron star inspiral cause the gravitational wave phase to accumulate more rapidly than in binary black hole inspiral. We report a comparison of numerical waveforms from an extended set of simulations of inspiraling neutron-star binaries, computed by systematically varying the parameters of the equation of state above nuclear density. We calculate the signal strength of the difference between waveforms and obtain improved estimates of the accuracy with which second and third generation gravitational wave detectors can constrain the neutron-star equations of state. We also show how a observation of N events at varying distances improves the measurability.

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 Dates: 2011
 Publication Status: Published online
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Title: American Physical Society, APS April Meeting 2011
Place of Event: Anaheim, California
Start-/End Date: 2011-04-30 - 2011-05-03

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Title: Bulletin of the American Physical Society
Source Genre: Journal
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Pages: - Volume / Issue: 56 (4) Sequence Number: Y12.00005 Start / End Page: - Identifier: -