Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: detectability of GW170817-like events

Rosalba Perna, M. Celeste Artale, Yi Han Wang, Michela Mapelli, Davide Lazzati, Cecilia Sgalletta, Filippo Santoliquido

Research output: Contribution to journalArticlepeer-review

14 Citations (Scopus)

Abstract

The association of GRB170817A with a binary neutron star (BNS) merger has revealed that BNSs produce at least a fraction of short gamma-ray bursts (SGRBs). As gravitational wave (GW) detectors push their horizons, it is important to assess coupled electromagnetic (EM)/GW probabilities and maximize observational prospects. Here, we perform BNS population synthesis calculations with the code mobse, seeding the binaries in galaxies at three representative redshifts, z = 0.01, 0.1, and 1 of the Illustris TNG50 simulation. The binaries are evolved and their locations numerically tracked in the host galactic potentials until merger. Adopting the microphysics parameters of GRB170817A, we numerically compute the broad-band light curves of jets from BNS mergers, with the afterglow brightness dependent on the local medium density at the merger site. We perform Monte Carlo simulations of the resulting EM population assuming either a random viewing angle with respect to the jet, or a jet aligned with the orbital angular momentum of the binary, which biases the viewing angle probability for GW-triggered events. We find a gamma-ray detection probability of ∼ 2 per cent,10 per cent, and 40 per cent for BNSs at z = 1, 0.1, and 0.01, respectively, for the random case, rising to ∼ 75 per cent for the z = 0.01, GW-triggered aligned case. Afterglow detection probabilities of GW-triggered BNS mergers vary in the range of ∼ 0.3 - 0.5 per cent, with higher values for aligned jets, and are comparable across the high- and low-energy bands, unlike gamma-ray-triggered events (cosmological SGRBs) which are significantly brighter at higher energies. We further quantify observational biases with respect to host galaxy masses.

Original languageEnglish
Pages (from-to)2654-2668
Number of pages15
JournalMonthly Notices of the Royal Astronomical Society
Volume512
Issue number2
DOIs
Publication statusPublished - 1 May 2022
Externally publishedYes

Keywords

  • (stars:) binaries (including multiple): close
  • (stars:) gamma-ray burst: general
  • galaxies: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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