From e19c0bdaafa74ce6b3a2f773d2087b84d373628b Mon Sep 17 00:00:00 2001 From: Michael Zingale Date: Thu, 14 Mar 2024 15:54:10 -0400 Subject: [PATCH] add a readme for subchandra (#2776) also fix a typo and formatting in the flame_wave readme --- Exec/science/flame_wave/README.md | 26 ++++++++++++++++---------- Exec/science/subchandra/README.md | 24 ++++++++++++++++++++++++ 2 files changed, 40 insertions(+), 10 deletions(-) create mode 100644 Exec/science/subchandra/README.md diff --git a/Exec/science/flame_wave/README.md b/Exec/science/flame_wave/README.md index 8deea3ff37..d062c58f61 100644 --- a/Exec/science/flame_wave/README.md +++ b/Exec/science/flame_wave/README.md @@ -1,19 +1,23 @@ # flame_wave -This is the XRB flame setup. I has been used for several -papers, including: +This is the XRB flame setup. It has been used for several papers, +including: -* Eiden et al. 2020 (https://ui.adsabs.harvard.edu/abs/2020ApJ...894....6E) +* Eiden et al. 2020 + (https://ui.adsabs.harvard.edu/abs/2020ApJ...894....6E) This modeled pure He flames and used "boosted" flames, which were artificially sped up. -* Harpole et al. 2021 (https://ui.adsabs.harvard.edu/abs/2021ApJ...912...36H/abstract) +* Harpole et al. 2021 + (https://ui.adsabs.harvard.edu/abs/2021ApJ...912...36H/abstract) - This also modeled pure He flames, but without any boosting. A variety of - rotation rates were explored. The inputs files for this are in `inputs_He/` + This also modeled pure He flames, but without any boosting. A + variety of rotation rates were explored. The inputs files for this + are in `inputs_He/` -* Zingale et al. 2023 (https://ui.adsabs.harvard.edu/abs/2023ApJ...952..160Z/abstract) +* Zingale et al. 2023 + (https://ui.adsabs.harvard.edu/abs/2023ApJ...952..160Z/abstract) This explored both 2D and 3D pure He flames. Another change was in the lower boundary condition -- a reflecting boundary was used an @@ -21,8 +25,10 @@ papers, including: `inputs_He/` and also available on Zenodo: https://zenodo.org/record/7692201 -* Chen et al. 2023 (https://ui.adsabs.harvard.edu/abs/2023ApJ...955..128C/abstract) +* Chen et al. 2023 + (https://ui.adsabs.harvard.edu/abs/2023ApJ...955..128C/abstract) - This looked at 2D pure He flames and explored different reaction networks. - The inputs files are available on Zenodo: https://zenodo.org/record/8117761 + This looked at 2D pure He flames and explored different reaction + networks. The inputs files are available on Zenodo: + https://zenodo.org/record/8117761 diff --git a/Exec/science/subchandra/README.md b/Exec/science/subchandra/README.md new file mode 100644 index 0000000000..d0f2c17c84 --- /dev/null +++ b/Exec/science/subchandra/README.md @@ -0,0 +1,24 @@ +# subchandra + +This is the double detonation Type Ia supernova setup. It takes a 1-d +initial model representing a sub-Chandra WD and a surface He layer and +initializes a small perturbation at the pole in the He layer. + +Initial models for this setup can be created via +https://github.com/AMReX-Astro/initial_models in the sub_chandra/ directory. + +This setup has been used in the following papers: + +* Zingale et al. 2022 + (https://ui.adsabs.harvard.edu/abs/2022ApJ...936....6Z/abstract) + + This paper introduced the simplified-SDC time-integration method and + used the double detonation setup as a test problem. + +* Zingale et al. 2024 + (https://ui.adsabs.harvard.edu/abs/2023arXiv230901802Z/abstract) + + This paper showed that the simplified-SDC method can model double + detonations without cutting the timestep or limiting the reaction + rates. It also explored disabling burning in shocks for this + problem.