Input files and numerical results for the paper "The Stellar Merger Scenario for Black Holes in the Pair-instability Gap". MESA_mergers.tar.gz contains separate work directories to run the pre-merger evolution, the merger relaxation process, and the post-merger evolution. The notebook init_merger.ipynb can be used to create input composition profiles for the merger relaxation. mix.tar.xz, primordial.tar.xz and pre-merger.tar.xz contain the numerical results used in the paper (selected profiles and history files). A git repository for this project is available on Bitbucket
In the cores of young dense star clusters, repeated stellar collisions involving the same object can...
The last few years have seen enormous progress in the field of galaxy formation and evolution. The l...
Data products and input files necessary to reproduce the results of the paper "The role of mass tran...
Data products and files to reproduce the results from du Buisson et al. (2020). MESA Calculations ...
This repository contains several data from the paper "Eccentric black hole mergers via three-body in...
The merger of 2 black holes is expected to be a common event in the universe. We perform a sta-tisti...
We have included the inlists, important run files, and selected simulation data accompanying Rui and...
We are grateful to the MESA developers for building and making available high-quality computational ...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
As galaxies merge in the standard hierarchical scenario of galaxy formation, their central Black Hol...
Inlists and initial models for simulating post-merger evolution of ONe WD + CO WD pairs. Folder in...
Rapid binary population synthesis codes are often used to investigate the evolution of compact-objec...
Inlists and initial models for simulating post-merger evolution of double ONe WD merger remnant (arX...
MESA inlists, run_star_extras, and data associated with Marchant et al. (2016). MESA version 8118. ...
The final outcome of white dwarf mergers across the entire merger parameter space is still relativel...
In the cores of young dense star clusters, repeated stellar collisions involving the same object can...
The last few years have seen enormous progress in the field of galaxy formation and evolution. The l...
Data products and input files necessary to reproduce the results of the paper "The role of mass tran...
Data products and files to reproduce the results from du Buisson et al. (2020). MESA Calculations ...
This repository contains several data from the paper "Eccentric black hole mergers via three-body in...
The merger of 2 black holes is expected to be a common event in the universe. We perform a sta-tisti...
We have included the inlists, important run files, and selected simulation data accompanying Rui and...
We are grateful to the MESA developers for building and making available high-quality computational ...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
As galaxies merge in the standard hierarchical scenario of galaxy formation, their central Black Hol...
Inlists and initial models for simulating post-merger evolution of ONe WD + CO WD pairs. Folder in...
Rapid binary population synthesis codes are often used to investigate the evolution of compact-objec...
Inlists and initial models for simulating post-merger evolution of double ONe WD merger remnant (arX...
MESA inlists, run_star_extras, and data associated with Marchant et al. (2016). MESA version 8118. ...
The final outcome of white dwarf mergers across the entire merger parameter space is still relativel...
In the cores of young dense star clusters, repeated stellar collisions involving the same object can...
The last few years have seen enormous progress in the field of galaxy formation and evolution. The l...
Data products and input files necessary to reproduce the results of the paper "The role of mass tran...