Published May 2, 2023 | Version 1.0.0
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SEVN parameter file from the paper "Binary neutron star populations in the Milky Way" by Sgalletta et al., 2023

Authors/Creators

  • 1. SISSA
  • 2. University of Padova
  • 3. Universidad Andres Bello
  • 4. Cardiff University
  • 5. INAF-Ossrrvatorio Astronomico di Cagliari
  • 6. Università di Pisa

Description

The repository contains the runtime parameters used in the SEVN simulations analysed in the paper "Binary neutron star populations in the Milky Way" by  Sgalletta et al., 2023.

Repository content: 

- used_params_Sgalletta2023.txt
  The file contains all the runtime parameters used in the SEVN simulations. The parameters that have been varied in different runs are        indicated with **** and the explored values are reported in the comment. See the SEVN userguide (https://gitlab.com/sevncodes/sevn/-/blob/SEVN/resources/SEVN_userguide.pdf) for the description of each parameter 

 

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used_params_Sgalletta2023.txt

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Additional details

Funding

European Commission
DEMOBLACK - Demography of black hole binaries in the era of gravitational wave astronomy 770017