Rapid population synthesis of double neutron stars
Alejandro Vigna-Gómez avignagomez@nbi.ku.dk
Bonn 2020 14th Bonn workshop on the formation and evolution of neutron stars
Rapid population synthesis of double neutron stars Alejandro - - PowerPoint PPT Presentation
Rapid population synthesis of double neutron stars Alejandro Vigna-Gmez avignagomez@nbi.ku.dk Bonn 2020 14th Bonn workshop on the formation and evolution of neutron stars 1 Double Neutron Stars (DNSs): Observations Data as presented in
Alejandro Vigna-Gómez avignagomez@nbi.ku.dk
Bonn 2020 14th Bonn workshop on the formation and evolution of neutron stars
See Tauris+2017 and references therein.
2.00 2.25 2.50 2.75 3.00 3.25 3.50 3.75 4.00
mtot (M)
2 4 6 8 10
Probability density
χ < 0.89 χ < 0.05 Galactic BNS
* GW170817: Abbott+2017 (arXiv:1710.05832) ^GW190425 : Abbott+2019 (arXiv:2001.01761) Data as presented in Vigna-Gómez+2018 (arXiv:1805.07974)
^GW190425 *GW170817: mtot=2.74, 2.82 Msol
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Vigna-Gómez+2020 (arXiv:2001.09829) https://zenodo.org/record/3593844 Period-eccentricity (P-e) diagram Hertzsprung-Russell diagram
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https://compas.science/ compas-user@googlegroups.com 3
p(M1,q,e,a)ZAMS p(M1,q,e,a)DNS Common Envelope Supernovae Mass Transfer Winds Vkick Mrem λ α facc γ fWR fLBV Initial Distributions Final Distributions
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Data: https://zenodo.org/record/3593844 5
Data: https://zenodo.org/record/3593844 5
Credit: T. Rebagliato & A. Vigna-Gómez Plots: https://zenodo.org/record/3634498 (69% of all DNSs) 6
Credit: T. Rebagliato & A. Vigna-Gómez Plots: https://zenodo.org/record/3634498 (20% of all DNSs) 7
Neutron star – Giant donor Single-core common-envelope episode Channel I (~70%) Giant donor – Giant companion Double-core common-envelope episode Channel II (~20%)
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Vigna-Gómez+2020 (arXiv:2001.09829) 9
Vigna-Gómez+2020 (arXiv:2001.09829) https://zenodo.org/record/3593844 BLUE: single-core RED: double-core
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Fryer Delayed, Z=0.0142
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Two formation channels:
^“Similar” results with MOBSE, ComBiNe, StarTrack, etc.
DNS merger rates (Gpc^3 yr^−1):
110–3840
250–2810
240–280
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