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Title: Full transport model of GW170817-like disk produces a blue kilonova

Journal Article · · Physical Review D

The 2017 detection of the inspiral and merger of two neutron stars in gravitational waves and gamma rays was accompanied by a quickly reddening transient. Such a transient was predicted to occur following a rapid neutron capture (r-process) nucleosynthesis event, which synthesizes neutron-rich, radioactive nuclei and can take place in both dynamical ejecta and in the wind driven off the accretion torus formed after a neutron star merger. In this study, we present the first three-dimensional general relativistic, full transport neutrino radiation magnetohydrodynamics simulations of the black hole-accretion disk-wind system produced by the GW170817 merger. We show that the small but non-negligible optical depths lead to neutrino transport globally coupling the disk electron fraction, which we capture by solving the transport equation with a Monte Carlo method. The resulting absorption drives up the electron fraction in a structured, continuous outflow, with electron fraction as high as Ye ~ 0.4 in the extreme polar region. Finally, we show via nuclear reaction network and radiative transfer calculations that nucleosynthesis in the disk wind will produce a blue kilonova.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)
Grant/Contract Number:
89233218CNA000001; SC0018297; 20170508DR
OSTI ID:
1570643
Alternate ID(s):
OSTI ID: 1546476
Report Number(s):
LA-UR-19-22623; PRVDAQ; TRN: US2100146
Journal Information:
Physical Review D, Vol. 100, Issue 2; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 116 works
Citation information provided by
Web of Science

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Cited By (5)

Kilonovae journal December 2019
Gamma Rays from Kilonova: A Potential Probe of r -process Nucleosynthesis journal February 2020
Can Kilonova Light Curves Be Standardized? journal November 2019
Spiral-wave Wind for the Blue Kilonova journal November 2019
Gamma-rays from kilonova: a potential probe of r-process nucleosynthesis text January 2019

Figures / Tables (8)