Published November 24, 2015 | Version Submitted
Journal Article Open

Application of artificial neural network to search for gravitational-wave signals associated with short gamma-ray bursts

  • 1. ROR icon Hanyang University
  • 2. ROR icon Syracuse University
  • 3. ROR icon California Institute of Technology
  • 4. ROR icon Pusan National University
  • 5. ROR icon National Institute for Mathematical Sciences

Abstract

We apply a machine learning algorithm, the artificial neural network, to the search for gravitational-wave signals associated with short gamma-ray bursts (GRBs). The multi-dimensional samples consisting of data corresponding to the statistical and physical quantities from the coherent search pipeline are fed into the artificial neural network to distinguish simulated gravitational-wave signals from background noise artifacts. Our result shows that the data classification efficiency at a fixed false alarm probability (FAP) is improved by the artificial neural network in comparison to the conventional detection statistic. Specifically, the distance at 50% detection probability at a fixed false positive rate is increased about 8%–14% for the considered waveform models. We also evaluate a few seconds of the gravitational-wave data segment using the trained networks and obtain the FAP. We suggest that the artificial neural network can be a complementary method to the conventional detection statistic for identifying gravitational-wave signals related to the short GRBs.

Additional Information

© 2015 IOP Publishing Ltd. Received 3 March 2015, revised 24 August 2015. Accepted for publication 2 October 2015. Published 24 November 2015. We thank the LIGO Scientific Collaboration and the Virgo Collaboration for the use of the data. We are also grateful for computational resources provided by the Leonard E Parker Center for Gravitation, Cosmology and Astrophysics at University of Wisconsin-Milwaukee (NSF-0923409). The authors would like to thank S Bose, K Cannon, T Dent, C Hanna, H M Lee, C Kim, and R Vaulin for helpful comments and useful discussions. KK would like to specially thank J Burguet-Castell, A Dietz, and N Fotopoulos for suggesting the initial motivation of this work. KK, YMK, CHL, HKL, JJO, SHO, and EJS were supported in part by the Global Research Network program of the National Research Foundation (NRF) funded by the Ministry of Science, ICT, and Future Planning of Korea (MSIP) (NRF-2011-220-C00029). KK, YMK, CHL, HKL, JJO, SHO, and EJS were also supported in part by the Global Science experimental Data hub Center (GSDC) at KISTI. The work of YMK and CHL was also supported by the NRF funded by the MSIP (NRF-2015R1A2A2A01004238).

Attached Files

Submitted - 1410.6878v2.pdf

Files

1410.6878v2.pdf

Files (2.2 MB)

Name Size
md5:5d696e97ccd0f92c4d572b3d8027353d
2.2 MB Preview Download

Additional details

Identifiers

Eprint ID
63446
DOI
10.1088/0264-9381/32/24/245002
Resolver ID
CaltechAUTHORS:20160107-105509801

Related works

Funding

NSF
0923409
ICT & Future Planning of Korea
National Research Foundation of Korea (NRF)
NRF-2011-220- C00029
KISTI Global Science Experimental Data Hub Center (GSDC)
National Research Foundation of Korea (NRF)
NRF-2015R1A2A2A01004238

Dates

Created
2016-01-08
Created from EPrint's datestamp field
Updated
2022-07-12
Created from EPrint's last_modified field