How to Install and Uninstall mpgrafic Package on Ubuntu 21.10 (Impish Indri)

Last updated: November 26,2024

1. Install "mpgrafic" package

This guide let you learn how to install mpgrafic on Ubuntu 21.10 (Impish Indri)


    
        
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                sudo apt update
            
                    
    
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                sudo apt install
            
                        
                mpgrafic
            
                    
    
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2. Uninstall "mpgrafic" package

This tutorial shows how to uninstall mpgrafic on Ubuntu 21.10 (Impish Indri):


    
        
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                sudo apt remove
            
                        
                mpgrafic
            
                    
    
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                sudo apt autoclean && sudo apt autoremove
            
                    
    
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3. Information about the mpgrafic package on Ubuntu 21.10 (Impish Indri)

Package: mpgrafic
Architecture: amd64
Version: 0.3.19-1
Priority: optional
Section: universe/science
Origin: Ubuntu
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astro Team
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Installed-Size: 147
Depends: fftw2, libc6 (>= 2.29), libgfortran5 (>= 10), libgsl25 (>= 2.6), libopenmpi3 (>= 4.0.3), mpi-default-bin
Recommends: gnudatalanguage
Filename: pool/universe/m/mpgrafic/mpgrafic_0.3.19-1_amd64.deb
Size: 48016
MD5sum: 193b3ce6ebf7827b750eda4f9d39f526
SHA1: 921a4b54e64092b93b611e23f67b8eaa60784b17
SHA256: 63107323b998ae28f4de797243ddd5ed6ca2f0ba28a55207b627de0868539db2
SHA512: 0432417f45def5c403886cdd1488e4e19382571502c4a8a09044415337f49f90ce334f98ba5a7eab23ef60afbfc69182df78852537db4a887697ae00bd0cf0a0
Homepage: http://www2.iap.fr/users/pichon/mpgrafic.html
Description-en: MPI version of N-body initial conditions grafic package
mpgrafic produces initial conditions files for N-body simulations of
cosmological large-scale structure formation. It is a free-licensed,
MPI-parallelised, rewritten version of Ed Bertschinger's grafic-1
program, producing output files in the grafic format. It includes
options for an Eisenstein and Hu baryonic wiggles power spectrum, for
using a low-resolution map for large-scale modes in the spirit of
grafic-2, and together with constrfield, can be used for generating
constrained initial conditions. Details are given in Prunet et al
(2008) http://cdsads.u-strasbg.fr/abs/2008ApJS..178..179P.
Description-md5: 058d545128c1281fd9f68f462c6d197d