CaltechAUTHORS
  A Caltech Library Service

Systematic Parameter Errors in Inspiraling Neutron Star Binaries

Favata, Marc (2014) Systematic Parameter Errors in Inspiraling Neutron Star Binaries. Physical Review Letters, 112 (10). Art. No. 101101. ISSN 0031-9007. https://resolver.caltech.edu/CaltechAUTHORS:20140422-143821253

[img]
Preview
PDF (arXiv) - Submitted Version
See Usage Policy.

599Kb
[img]
Preview
PDF - Published Version
See Usage Policy.

275Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20140422-143821253

Abstract

The coalescence of two neutron stars is an important gravitational wave source for LIGO and other detectors. Numerous studies have considered the precision with which binary parameters (masses, spins, Love numbers) can be measured. Here I consider the accuracy with which these parameters can be determined in the presence of systematic errors due to waveform approximations. These approximations include truncation of the post-Newtonian (PN) series and neglect of neutron star (NS) spin, tidal deformation, or orbital eccentricity. All of these effects can yield systematic errors that exceed statistical errors for plausible parameter values. In particular, neglecting spin, eccentricity, or high-order PN terms causes a significant bias in the NS Love number. Tidal effects will not be measurable with PN inspiral waveforms if these systematic errors are not controlled.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1103/PhysRevLett.112.101101DOIArticle
http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.112.101101PublisherArticle
http://arxiv.org/abs/1310.8288arXivWorking Paper
Additional Information:© 2014 American Physical Society. Published 10 March 2014; Received 30 October 2013. This work was supported by NSF Grants No. PHY- 0970074, No. PHY-1308527, and the UWM Research Growth Initiative. I thank Curt Cutler, Stephen Fairhurst, Jocelyn Read, Michele Vallisneri, and the referees for comments on this manuscript. I also thank Kent Yagi and Nicolás Yunes for helping me find a coding error that affected my results. Their complementary work [37] focuses on the systematic error in the tidal deformability using a modified version of the scheme discussed here.
Funders:
Funding AgencyGrant Number
NSFPHY-0970074
NSFPHY-1308527
UWM Research Growth InitiativeUNSPECIFIED
Issue or Number:10
Classification Code:PACS: 04.30.-w; 04.25.Nx; 04.30.Tv; 97.60.Jd
Record Number:CaltechAUTHORS:20140422-143821253
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140422-143821253
Official Citation:Favata, M. (2014). Systematic Parameter Errors in Inspiraling Neutron Star Binaries. Physical Review Letters, 112(10), 101101.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:45120
Collection:CaltechAUTHORS
Deposited By: Aucoeur Ngo
Deposited On:25 Apr 2014 16:52
Last Modified:03 Oct 2019 06:26

Repository Staff Only: item control page