DPI: Symplectic mapping for binary star systems for the Merc

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Ada Coda
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DPI: Symplectic mapping for binary star systems for the Mercury software package

Post by Ada Coda » Tue Apr 28, 2015 12:33 am

DPI: Symplectic mapping for binary star systems for the Mercury software package

Abstract: DPI is a FORTRAN77 library that supplies the symplectic mapping method for binary star systems for the Mercury N-Body software package (ascl:1201.008). The binary symplectic mapping is implemented as a hybrid symplectic method that allows close encounters and collisions between massive bodies and is therefore suitable for planetary accretion simulations.

Credit: Turrini, D.

Site: http://arxes.iaps.inaf.it/DownloadSoftw ... 1_0.tar.gz
http://adsabs.harvard.edu/abs/2005MSAIS...6..172T

Bibcode: 2015ascl.soft04012T

ID: ascl:1504.012
Last edited by Ada Coda on Mon Feb 04, 2019 7:05 pm, edited 1 time in total.
Reason: Updated code entry.

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