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spurzem authored May 11, 2023
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Expand Up @@ -2,7 +2,28 @@ This is Nbody6++GPU - Beijing version, an N-body star cluster simulation code, m

The code is an offspring of Sverre Aarseth's direct N-body codes see www.sverre.com .

This is the code suitable for parallel and GPU accelerated runs on supercomputers and workstations.
This is the code suitable for parallel and GPU accelerated runs on supercomputers and workstations. Before we give some more practical help, please read the following disambiguation; there is another github of Nbody6++GPU:

LW: https://github.com/nbodyx/ - if interested please contact and collaborate
with Long Wang [email protected]
RS: https://github.com/nbody6ppgpu - if interested please contact and
collaborate with Rainer Spurzem [email protected] [email protected]

Here is an example of current differences between the code version (May 2023), more changes and differences may occur in the future, if in doubt, ask the authors.

1. LW: implementation of Milky Way potential following the MWPotential2014 in
Galpy (Bovy 2015).
2. RS: implementation of spin and mass dependent recoil kicks after GW merger
(Arca Sedda et al. 2023 subm. MNRAS)
3. LW: implementation of python data reading interface for PeTar analysis tool.
4. RS: use of HDF5 output files with python data reading interfaces
5. RS: Namelist based input format, allowing also to read all stellar evolution
and binary / collision parameters.
5. LW and RS: Some bug fixes related to Roche and GR radiation, in both versions
slightly different ways.
6. LW and RS: implementation of BSE from Banerjee et al. 2019

-------------------

# For users
## Installation
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