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The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: A Case Study on GW190425

Journal Article · · The Astrophysical Journal
 [1];  [2];  [3];  [4];  [5];  [6];  [3];  [7];  [8];  [9];  [10];  [11];  [12];  [13];  [14]
  1. Univ. of Amsterdam (Netherlands); Univ. of Amsterdam (Netherlands)
  2. Univ. of Amsterdam (Netherlands); Nikhef Theory Group, Amsterdam (Netherlands)
  3. Univ. of New Hampshire, Durham, NH (United States)
  4. California Institute of Technology (CalTech), Pasadena, CA (United States)
  5. Stockholm Univ. (Sweden)
  6. Univ. of Alberta, Edmonton, AB (Canada)
  7. Univ. of Amsterdam (Netherlands); Utrecht University (Netherlands)
  8. Univ. of Tokyo (Japan)
  9. Univ. of Amsterdam (Netherlands)
  10. Univ. of California, Santa Barbara, CA (United States); Institute for Advanced Study, Princeton, NJ (United States); Tata Inst. of Fundamental Research, Bangalore (India)
  11. Centre National de la Recherche Scientifique (CNRS), Paris (France); Univ. of Paris (France)
  12. Univ. of Minnesota, Minneapolis, MN (United States)
  13. Univ. of Potsdam (Germany); Max Planck Institute for Gravitational Physics, Potsdam (Germany)
  14. Univ. of Amsterdam (Netherlands); Stockholm Univ. (Sweden)

In recent years, there have been significant advances in multimessenger astronomy due to the discovery of the first, and so far only confirmed, gravitational wave event with a simultaneous electromagnetic (EM) counterpart, as well as improvements in numerical simulations, gravitational wave (GW) detectors, and transient astronomy. This has led to the exciting possibility of performing joint analyses of the GW and EM data, providing additional constraints on fundamental properties of the binary progenitor and merger remnant. Here, in this work, we present a new Bayesian framework that allows inference of these properties, while taking into account the systematic modeling uncertainties that arise when mapping from GW binary progenitor properties to photometric light curves. We extend the relative binning method presented in Zackay et al. to include extrinsic GW parameters for fast analysis of the GW signal. The focus of our EM framework is on light curves arising from r-process nucleosynthesis in the ejected material during and after merger, the so-called kilonova, and particularly on black hole–neutron star systems. As a case study, we examine the recent detection of GW190425, where the primary object is consistent with being either a black hole or a neutron star. We show quantitatively how improved mapping between binary progenitor and outflow properties, and/or an increase in EM data quantity and quality are required in order to break degeneracies in the fundamental source parameters.

Research Organization:
Univ. of New Hampshire, Durham, NH (United States)
Sponsoring Organization:
USDOE Office of Science (SC); National Aeronautics and Space Administration (NASA); National Science Foundation (NSF)
Grant/Contract Number:
SC0020435
OSTI ID:
1981230
Journal Information:
The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 922; ISSN 0004-637X
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English

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