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[![AMReX](https://amrex-codes.github.io/badges/powered%20by-AMReX-red.svg)](https://amrex-codes.github.io)

*an adaptive mesh, massively-parallel, cosmological simulation code*
*An adaptive mesh, massively-parallel, cosmological simulation code*

******

## About
### About

Nyx code solves equations of compressible hydrodynamics on an adaptive grid
hierarchy coupled with an N-body treatment of dark matter. The gasdynamics in
Expand All @@ -20,40 +20,52 @@ ionization equilibrium, the code calculates heating and cooling processes of the
primordial-composition gas in an ionizing ultraviolet background radiation field.
Additional physics capabilities are under development.

Nyx is parallelized with MPI + OpenMP, and has been run at parallel concurrency
of up to 2,097,152 (on NERSC's Cori).
While Nyx can run on any Linux system in general, we particularly focus on supercomputer systems.
Nyx is parallelized with MPI + X, where "X" can be OpenMP, Cuda, or HIP (DPC++ implementation
is ongoing). In the OpenMP regime, Nyx and has been successfully run at parallel concurrency
of up to 2,097,152 (on NERSC's Cori-KNL). With Cuda implementation, it was ran on up to
13,824 GPUs (on OLCF's Summit).

More information on Nyx can be found at
http://amrex-astro.github.io/Nyx/

## Getting Started

To compile the code, we require Fortran 2003 and C++11 compliant compilers that
support (if parallelism is sought) OpenMP 4.5 or better, and/or MPI-2 or higher
implementation.
### Standards and dependencies

To compile the code we require C++11 compliant compilers that support MPI-2 or
higher implementation. If threads or accelerators are used, we require
OpenMP 4.5 or higher, Cuda 9 or higher, or HIP-Clang.

To use Nyx, you also need AMReX:
https://github.com/AMReX-codes/amrex

For axample, this is what we currently do to compile Lyman alpha executable on Summit:
```sh
$ module load gcc/6.4.0 cuda/11.0.3

$ git clone https://github.com/AMReX-Codes/amrex.git
$ git clone https://github.com/AMReX-astro/Nyx.git

$ cd Nyx/Exec/LyA
$ make -j 12 USE_CUDA=TRUE
```


There is a User's Guide in `Nyx/UsersGuide/` (type `make` to build
from LaTeX source) that will guide you through running your first
problem.


## Development Model
### Development model

New features are committed to the `development` branch. We use nightly
The `development` branch in also the main branch. We use nightly
regression testing to ensure that no answers change (or if they do, that
the changes were expected). No changes should be pushed directly into
`master`. Approximately once a month, we perform a merge of `development`
into `master`.

Contributions are welcomed and should be done via pull requests.
the changes were expected). Contributions are welcomed and should be done via pull requests.
A pull request should be generated from your fork of Nyx and should target
the `development` branch.


## Physics
### Physics

For the description of the N-body and adiabatic hydro algorithms in Nyx, see
Almgren, Bell, Lijewski, Lukic & Van Andel (2013), ApJ, 765, 39:
Expand All @@ -72,7 +84,8 @@ http://adsabs.harvard.edu/abs/2017ApJ...837..106O
We have also implemented non-radiative transfer methods to model inhomogeneous reionization,
the paper is in preparation.

## Output

### Output

Nyx outputs certain global diagnostics at each timestep and plot files at regular
intervals, or at user-specified redshifts. Visualization packages
Expand All @@ -88,11 +101,11 @@ related to the Lyman-alpha forest science. These suites are fully MPI-parallel a
be run either "in situ" or "in-transit", or with a combination of both.


## License
### License
Nyx is released under the LBL's modified BSD license, see the [license.txt](license.txt) file for details.


## Contact
### Contact

For questions, comments, suggestions, contact Ann Almgren at [email protected]
or Zarija Lukic at [email protected] .

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