Common-envelope episodes that lead to double neutron star formation
Alejandro Vigna-Gómez
Lund 2020 Compact Objects For All
Common-envelope episodes that lead to double neutron star - - PowerPoint PPT Presentation
Common-envelope episodes that lead to double neutron star formation Alejandro Vigna-Gmez Lund 2020 Compact Objects For All 1 Population Synthesis Initial Distributions p(M 1 ,q,e,a) ZAMS f acc V kick Mass M rem Supernovae Transfer
Alejandro Vigna-Gómez
Lund 2020 Compact Objects For All
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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Credit: Philip D. Hall
ejection merger time
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https://compas.science/ compas-user@googlegroups.com 3
Credit: T. Rebagliato & A. Vigna-Gómez https://zenodo.org/record/3634498 (69% of all DNSs) 4
Credit: T. Rebagliato & A. Vigna-Gómez https://zenodo.org/record/3634498 (20% of all DNSs) 5
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) 7
https://zenodo.org/record/3593844 8
Summary of Uncertainties Two formation channels:
DNS merger rates (Gpc^3 yr^−1):
110–3840
250–2810
240–280
^“Similar” results with MOBSE, ComBiNe, StarTrack, etc.
Wild Extrapolations Wide DNSs:
Close DNSs:
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Author arXiv Binary Physics BBHs DNSs Statistics Cosmic History Rates Data Only Barrett+2017 1704.03781 X X Barrett+2018 1711.06287 X X X Bavera+2019 1906.12257 X X X X X Broekgaarden+2019 1905.00910 X X X Chattopadhyay+2019 1912.02415 X X Howitt+2019 1912.07771 X Lau+2019 1910.12422 X X X Neijssel+2019 1906.08136 X X X Schrøder+2019 1906.04189 X X Stevenson+2017 1704.01352 X X Stevenson+2019 1904.02821 X X X Vigna-Gomez+2018 1805.07974 X X X X X Vigna-Gomez+2020 2001.09829 X X X
https://compas.science/ compas-user@googlegroups.com