Future prospects for constraining nuclear matter parameters with gravitational waves
Abstract
The gravitational wave emission from the merging binary neutron star system GW170817 arrived full of tidal information which can be used to probe the fundamental ultradense nuclear physics residing in these stars. In previous work, we used two-dimensional correlations between nuclear matter parameters and tidal deformabilities of neutron stars applying specifically to GW170817 to derive constraints on the former. Here, we extend this analysis by finding similar correlations for varying chirp masses, the dominant determining factor in the frequency evolution of the inspiral, such that one can apply the same method to future detections. We estimate how accurately one can measure nuclear parameters with future gravitational wave interferometers and show how such measurements can be improved by combining multiple events. We find that bounds on the nuclear parameters with future observations can improve from the current one with GW170817 only by ~30% due to the existence of systematic errors caused mainly by the remaining uncertainty in the equation of state near and just above the nuclear saturation density. As a result, we show that such systematic errors can be reduced by considering multidimensional correlations among nuclear parameters and tidal deformabilities with various neutron star masses.
- Authors:
-
[2];
- Univ. of Virginia, Charlottesville, VA (United States)
- Univ. of Tennessee, Knoxville, TN (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
- Publication Date:
- Research Org.:
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1560403
- Alternate Identifier(s):
- OSTI ID: 1545444
- Grant/Contract Number:
- AC05-00OR22725
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Volume: 100; Journal Issue: 2; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS
Citation Formats
Carson, Zack, Steiner, Andrew W., and Yagi, Kent. Future prospects for constraining nuclear matter parameters with gravitational waves. United States: N. p., 2019.
Web. doi:10.1103/PhysRevD.100.023012.
Carson, Zack, Steiner, Andrew W., & Yagi, Kent. Future prospects for constraining nuclear matter parameters with gravitational waves. United States. https://doi.org/10.1103/PhysRevD.100.023012
Carson, Zack, Steiner, Andrew W., and Yagi, Kent. Wed .
"Future prospects for constraining nuclear matter parameters with gravitational waves". United States. https://doi.org/10.1103/PhysRevD.100.023012. https://www.osti.gov/servlets/purl/1560403.
@article{osti_1560403,
title = {Future prospects for constraining nuclear matter parameters with gravitational waves},
author = {Carson, Zack and Steiner, Andrew W. and Yagi, Kent},
abstractNote = {The gravitational wave emission from the merging binary neutron star system GW170817 arrived full of tidal information which can be used to probe the fundamental ultradense nuclear physics residing in these stars. In previous work, we used two-dimensional correlations between nuclear matter parameters and tidal deformabilities of neutron stars applying specifically to GW170817 to derive constraints on the former. Here, we extend this analysis by finding similar correlations for varying chirp masses, the dominant determining factor in the frequency evolution of the inspiral, such that one can apply the same method to future detections. We estimate how accurately one can measure nuclear parameters with future gravitational wave interferometers and show how such measurements can be improved by combining multiple events. We find that bounds on the nuclear parameters with future observations can improve from the current one with GW170817 only by ~30% due to the existence of systematic errors caused mainly by the remaining uncertainty in the equation of state near and just above the nuclear saturation density. As a result, we show that such systematic errors can be reduced by considering multidimensional correlations among nuclear parameters and tidal deformabilities with various neutron star masses.},
doi = {10.1103/PhysRevD.100.023012},
journal = {Physical Review D},
number = 2,
volume = 100,
place = {United States},
year = {2019},
month = {7}
}
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Figures / Tables:
FIG. 1: The overall (statistical plus systematic) errors on Ksym,0 using priors in $\tilde{Λ}$ for single-event measurements, plotted as a function of the binary systems' chirp mass { applicable to any future binary NS merger. We fix the mass ratio as q = 0.9 consistent with GW170817 and choosemore »
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