Radiation hydrodynamics modelling of kilonovae with SNEC. Issue 1 (15th February 2022)
- Record Type:
- Journal Article
- Title:
- Radiation hydrodynamics modelling of kilonovae with SNEC. Issue 1 (15th February 2022)
- Main Title:
- Radiation hydrodynamics modelling of kilonovae with SNEC
- Authors:
- Wu, Zhenyu
Ricigliano, Giacomo
Kashyap, Rahul
Perego, Albino
Radice, David - Abstract:
- ABSTRACT: We develop a method to compute synthetic kilonova light curves that combine numerical relativity simulations of neutron star mergers and the SNEC radiation–hydrodynamics code. We describe our implementation of initial and boundary conditions, r-process heating, and opacities for kilonova simulations. We validate our approach by carefully checking that energy conservation is satisfied and by comparing the SNEC results with those of two semi-analytic light-curve models. We apply our code to the calculation of colour light curves for three binaries having different mass ratios (equal and unequal mass) and different merger outcome (short-lived and long-lived remnants). We study the sensitivity of our results to hydrodynamic effects, nuclear physics uncertainties in the heating rates, and duration of the merger simulations. We find that hydrodynamics effects are typically negligible and that homologous expansion is a good approximation in most cases. However, pressure forces can amplify the impact of uncertainties in the radioactive heating rates. We also study the impact of shocks possibly launched into the outflows by a relativistic jet. None of our models match AT2017gfo, the kilonova in GW170817. This points to possible deficiencies in our merger simulations and kilonova models that neglect non-LTE effects and possible additional energy injection from the merger remnant and to the need to go beyond the assumption of spherical symmetry adopted in this work.
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 512:Issue 1(2022)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 512:Issue 1(2022)
- Issue Display:
- Volume 512, Issue 1 (2022)
- Year:
- 2022
- Volume:
- 512
- Issue:
- 1
- Issue Sort Value:
- 2022-0512-0001-0000
- Page Start:
- 328
- Page End:
- 347
- Publication Date:
- 2022-02-15
- Subjects:
- hydrodynamics -- radiative transfer -- methods: numerical -- neutron star mergers
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/stac399 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 20735.xml