chemcomp 1.0

planet formation model including pebbles and gas accretion

chemcomp

Modeling the chemical composition of gas giants by accretion of pebbles, planetesimals and gas.

docs: WIKI

install:

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.

Publications

Original Publications

• 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.

Publications using chemcomp

• 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

And several more in preperation (last updated: 22.11.2023)

Thanks:

• 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.