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@@ -2,7 +2,28 @@ This is Nbody6++GPU - Beijing version, an N-body star cluster simulation code, m | |
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The code is an offspring of Sverre Aarseth's direct N-body codes see www.sverre.com . | ||
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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: | ||
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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] | ||
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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. | ||
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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 | ||
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------------------- | ||
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# For users | ||
## Installation | ||
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