Modeling the chemical composition of gas giants by accretion of pebbles, planetesimals and gas.
docs: WIKI
clone project:
git clone https://github.com/AaronDavidSchneider/chemcomp.git
move into directory:
cd chemcomp
Install conda environment:
conda create -n chemcomp numpy "astropy>=4.0" scipy matplotlib pyyaml jupyter parse h5py pip pytables
Install a development version chemcomp
:
pip install -e .
or install from pypi
pip install chemcomp
Adjust paths in chemcomp/helper/main_helper
if you need different directories for output and config.
-
Schneider & Bitsch (2021a)
How drifting and evaporating pebbles shape giant planets. I. Heavy element content and atmospheric C/O -
Schneider & Bitsch (2021b)
How drifting and evaporating pebbles shape giant planets. II. Volatiles and refractories in atmospheres -
Bitsch, Schneider & Kreidberg (2022)
How drifting and evaporating pebbles shape giant planets. III. The formation of WASP-77A b and$\tau$ Boötis b
Please cite Schneider & Bitsch(2021a), if you use chemcomp
in your work.
-
Bitsch et al. (2021)
Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line -
Hühn & Bitsch (2023)
How accretion of planet-forming disks influences stellar abundances -
Bitsch & Mah (2023)
Enriching inner discs and giant planets with heavy elements -
Mah & Bitsch (2023a)
Forming super-Mercuries: Role of stellar abundances -
Mah & Bitsch (2023b)
Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars -
Savvidou & Bitsch (2023)
How to make giant planets via pebble accretion -
Danti, Bitsch & Mah (2023)
Composition of giant planets: the roles of pebbles and planetesimals -
Chatziastros, Bitsch & Schneider (2023)
Constraining the formation history of the HAT-P-11 system by atmospheric abundances
And several more in preperation (last updated: 22.11.2023)
- I would like to thank Bertram Bitsch for his enormous support during the development of this code and for continuing to use the code together with his students.
- I would like to thank Cornelis Dullemond for providing the solver which (in adapted version) is used to solve the gas viscous disk equation and dust transport equation.
- I would like to thank everyone, who has already used chemcomp in their work and has contributed in fixing small bugs.