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  5. DPI: Symplectic mapping for binary star systems for the Mercury software package
 
Title
DPI: Symplectic mapping for binary star systems for the Mercury software package
Date Issued
2015
Author(s)
TURRINI, Diego  
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. [Source code is in Astrophysics Source Code Library]
File(s)
DPI_Manual.pdf (79.91 KB)
Manuale Utente
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