Metadata-Version: 2.1
Name: chemcomp
Version: 1.0
Summary: planet formation model including pebbles and gas accretion
Home-page: https://github.com/aarondavidschneider/chemcomp
Author: Aaron David Schneider
Author-email: aaron.schneider@nbi.ku.dk
License: MIT
Description: # chemcomp
        
        Modeling the chemical composition of gas giants by accretion of pebbles, planetesimals and gas.
        
        **docs: [WIKI](https://chemcomp.readthedocs.io/en/latest/ "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)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S)</br>
            How drifting and evaporating pebbles shape giant planets. I. Heavy element content and atmospheric C/O
        
        -   [Schneider & Bitsch (2021b)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..72SS)</br>
            How drifting and evaporating pebbles shape giant planets. II. Volatiles and refractories in atmospheres
        
        -   [Bitsch, Schneider & Kreidberg (2022)](https://ui.adsabs.harvard.edu/abs/2022A&A...665A.138B)</br>
            How drifting and evaporating pebbles shape giant planets. III. The formation of WASP-77A b and $\tau$ Boötis b
        
        Please cite [Schneider & Bitsch(2021a)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S), if you use `chemcomp` in your work.
        
        ### Publications using `chemcomp`
        
        -   [Bitsch et al. (2021)](https://ui.adsabs.harvard.edu/abs/2021A&A...649L...5B)</br>
            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)](https://ui.adsabs.harvard.edu/abs/2023A&A...676A..87H)</br>
            How accretion of planet-forming disks influences stellar abundances
        
        -   [Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230900509B)</br>
            Enriching inner discs and giant planets with heavy elements
        
        -   [Mah & Bitsch (2023a)](https://ui.adsabs.harvard.edu/abs/2023A&A...673A..17M)</br>
            Forming super-Mercuries: Role of stellar abundances
        
        -   [Mah & Bitsch (2023b)](https://ui.adsabs.harvard.edu/abs/2023A&A...677L...7M)</br>
            Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars
        
        -   [Savvidou & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230903807S)</br>
            How to make giant planets via pebble accretion
        
        -   [Danti, Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv231002886D)</br>
            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.
        
Platform: UNKNOWN
Description-Content-Type: text/markdown
