M
Mathieu Renzo
Researcher at York University
Publications - 74
Citations - 3181
Mathieu Renzo is an academic researcher from York University. The author has contributed to research in topics: Stars & Supernova. The author has an hindex of 24, co-authored 63 publications receiving 2143 citations. Previous affiliations of Mathieu Renzo include Programme for International Student Assessment & University of Amsterdam.
Papers
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Journal ArticleDOI
On the formation history of Galactic double neutron stars
Alejandro Vigna-Gómez,Alejandro Vigna-Gómez,Coenraad J. Neijssel,Simon Stevenson,Simon Stevenson,Jim W. Barrett,Krzysztof Belczynski,Stephen Justham,Selma E. de Mink,Bernhard Müller,Philipp Podsiadlowski,Philipp Podsiadlowski,Mathieu Renzo,Dorottya Szécsi,Ilya Mandel,Ilya Mandel,Ilya Mandel +16 more
TL;DR: In this paper, the authors perform rapid population synthesis of massive binary stars and discuss model predictions, including DNS formation rates, mass distributions, and delay time distributions, varying assumptions and parameters of physical processes such as mass transfer stability criteria.
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Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
TL;DR: In this article, the location of the lower edge of the mass gap at 45$M_\odot$ is remarkably robust against variations in the metallicity, the treatment of internal mixing, and stellar wind mass loss.
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Light Curves of Core-Collapse Supernovae with Substantial Mass Loss using the New Open-Source SuperNova Explosion Code (SNEC)
Viktoriya S. Morozova,Anthony L. Piro,Mathieu Renzo,Mathieu Renzo,Christian D. Ott,Drew Clausen,Sean M. Couch,Justin A. Ellis,Luke F. Roberts +8 more
TL;DR: The SuperNova Explosion Code (SNEC) as discussed by the authors is an open-source Lagrangian code for the hydrodynamics and equilibrium-diffusion radiation transport in the expanding envelopes of supernovae.
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Mind the Gap: The Location of the Lower Edge of the Pair-instability Supernova Black Hole Mass Gap
Robert Farmer,Mathieu Renzo,S. E. de Mink,S. E. de Mink,Pablo Marchant,Stephen Justham,Stephen Justham +6 more
TL;DR: In this article, the location of the lower edge of the mass gap at 45 M is remarkably robust against variations in the metallicity, the treatment of internal mixing, and stellar wind mass loss, making it the most robust predictor for the final stages of the evolution of massive stars.
Journal ArticleDOI
Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
Emmanouil Zapartas,S. E. de Mink,Robert G. Izzard,Sung-Chul Yoon,Carles Badenes,Y. Götberg,A. de Koter,A. de Koter,Coenraad J. Neijssel,Mathieu Renzo,A. Schootemeijer,Tushar Shrotriya +11 more
TL;DR: In this article, a population synthesis study was conducted to compute the delay-time distribution of core-collapse supernovae, that is, the supernova rate versus time following a starburst, taking into account binary interactions.