LUTH - Observatoire de Paris https://luth.obspm.fr/ Laboratoire Univers et Théories fr SPIP - www.spip.net LUTH - Observatoire de Paris https://luthsp3.obspm.fr/local/cache-vignettes/L144xH14/siteon0-57ae6.png?1662990206 https://luth.obspm.fr/ 14 144 Codes Numériques https://luthsp3.obspm.fr/?Codes-Numeriques https://luthsp3.obspm.fr/?Codes-Numeriques 2019-03-21T10:26:01Z text/html fr webmaster <p>https://www.uv.es/coconut/ Coconut : General relativistic hydrodynamics code with dynamical space-time evolution. The main aim of this numerical code is the study of several astrophysical scenarios in which general relativity can play an important role, namely the collapse of rapidly rotating stellar cores and the evolution of isolated neutron stars. <br class='autobr' /> The code has two flavors : CoCoA, the axisymmetric (2D) magnetized version, and CoCoNuT, the 3D non-magnetized version. The CoCoA project (…)</p> - <a href="https://luthsp3.obspm.fr/?-ressources-numeriques-" rel="directory">Ressources numériques</a> <div class='rss_texte'><div id=tabart><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1035 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://www.uv.es/coconut/" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L500xH116/coconut-a3677.png?1663028837' width='500' height='116' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://www.uv.es/coconut/" class="spip_out" rel="external">Coconut</a> </i> : General relativistic hydrodynamics code with dynamical space-time evolution. The main aim of this numerical code is the study of several astrophysical scenarios in which general relativity can play an important role, namely the collapse of rapidly rotating stellar cores and the evolution of isolated neutron stars.<br class='autobr' /> The code has two flavors : CoCoA, the axisymmetric (2D) magnetized version, and CoCoNuT, the 3D non-magnetized version. The CoCoA project was started by Harald Dimmelmeier at the Max-Planck Institute for Astrophysics (Garching bei München, Germany) as part of his PhD thesis. It was extended to 3D (CoCoNuT) in collaboration with Jérôme Novak from the LUTH laboratory at the Observatoire de Paris (Meudon, France). This web page is intended to be a presentation of the numerical code and its scientific results. This code is not of public domain.</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1036 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://gyoto.obspm.fr" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L464xH623/gyoto-efb1c.png?1662994939' width='464' height='623' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://gyoto.obspm.fr" class="spip_out" rel="external">Gyoto</a> </i> : Provide a framework for computing orbits and ray-traced images in General relativity. It consists of a library (libgyoto), utility programs, and a plug-in for the Yorick programing language. Gyoto is known to run under Linux and Mac OS X. Please do tell us if you manage to run Gyoto under a different OS. It should compile and run with moderate effort on most UNIX-like systems</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1037 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://kadath.obspm.fr" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L500xH367/kappa-d72a9.jpg?1663028837' width='500' height='367' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://kadath.obspm.fr" class="spip_out" rel="external">Kadath</a> </i> : Blbiothèque pour la résolution des EDP de la relativité générale et de la théorie des champs, C++, parallelisé MPI, licence GPL</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1038 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://lorene.obspm.fr" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L500xH112/lorene-77f55.png?1663028837' width='500' height='112' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://lorene.obspm.fr" class="spip_out" rel="external">Lorene</a> </i> : Set of C++ classes to solve various problems arising in numerical relativity, and more generally in computational astrophysics. It provides tools to solve partial differential equations by means of multi-domain spectral methods. Scientific results obtained by means of LORENE are reported here.<br /> <br />LORENE classes implement basic structures such as arrays and matrices, but also abstract mathematical objects, such as tensors, and astrophysical objects, such as stars and black holes. Note that, as a research software, LORENE is under perpetual development</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1047 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://github.com/vreverdy/magrathea-pathfinder" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L220xH110/redshift-a0fdf.png?1662994939' width='220' height='110' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://github.com/vreverdy/magrathea-pathfinder" class="spip_out" rel="external">Magrathea-pathfinder</a> </i> : Code de lancer de rayon par intégration des équations géodésiques au sein de grilles adaptives. Calcul des effets de distortion dans l'espace des redshifts, des effets de lentilles gravitationnelles et de l'effet Sachs-Wolfe Intégré. C++ 2011, parallélisé MPI-Pthreads</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1049 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="http://www.projet-horizon.fr/rubrique64.html" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L150xH150/horizon-29432.jpg?1662994939' width='150' height='150' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="http://www.projet-horizon.fr/rubrique64.html" class="spip_out" rel="external">Mpgrafic</a> </i> : Code de génération des conditions initiales des simulations cosmologiques, Fortran 90, paralléllsation MPI<br class='autobr' /> <i>S.Prunet (IAP) et al., Développements LUTH</i> <br class='autobr' /> <i> <a href="http://www.projet-horizon.fr/rubrique64.html" class="spip_out" rel="external">Powergrid</a> </i> : Code de calcul du spectre de puissance de la distribution de matière, Fortran 90, parallélisation MPI<br class='autobr' /> <i>S.Prunet (IAP) et al., Développements LUTH</i></td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1040 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="http://homes.esat.kuleuven.be/~keppens" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L500xH346/amrvrac-07583.png?1663028837' width='500' height='346' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="http://homes.esat.kuleuven.be/~keppens" class="spip_out" rel="external">Mpi-Amrvac</a> </i> : MHD relativiste, transfert de rayonnement, Fortran 2003 / Perl, parallélisé MPI (run max = 4000 procs)</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1050 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://gitlab.obspm.fr/roy/pFoF" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L470xH199/pfof-0c9c1.png?1662994939' width='470' height='199' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://gitlab.obspm.fr/roy/pFoF" class="spip_out" rel="external">PFof</a> </i> : Code de détection des halos cosmologiques par la méthode de percolation Friends-of-Friends et de post-traitement de toutes les (lourdes) sorties du code de simulation cosmologique, Fortran 90, parallélisation</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1045 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://bitbucket.org/rteyssie/ramses" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L220xH262/ramses-df373.jpg?1662994939' width='220' height='262' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://bitbucket.org/rteyssie/ramses" class="spip_out" rel="external">Ramses</a> </i> : Code de simulations cosmologiques avec grille adaptative, Fortran 90, parallélisation MPI<br class='autobr' /> <i>R.Teyssier (UZH) et al.. Développements LUTH</i></td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1039 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://sagemanifolds.obspm.fr" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L350xH314/sage-5bea0.png?1662994939' width='350' height='314' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://sagemanifolds.obspm.fr" class="spip_out" rel="external">SageManifolds</a> </i> : implementing differential geometry and tensor calculus in the modern computer algebra system SageMath</td></tr> </tbody> </table></div></div> Bases de données https://luthsp3.obspm.fr/?Bases-de-donnees-832 https://luthsp3.obspm.fr/?Bases-de-donnees-832 2019-03-01T13:12:49Z text/html fr webmaster <p>https://compose.obspm.fr Compose : The online service CompOSE provides data tables for different state of the art equations of state (EoS) ready for further usage in astrophysical applications, nuclear physics and beyond http://www.deus-consortium.org/deuvo/ Deus-Data : This project aims at investigating the imprints of dark energy on cosmic structure formation through very high resolution cosmological simulations https://cosmo.obspm.fr/deus-pur-spectra/ Deus-Pur : Database of (…)</p> - <a href="https://luthsp3.obspm.fr/?-ressources-numeriques-" rel="directory">Ressources numériques</a> <div class='rss_texte'><div id=tabart><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1044 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://compose.obspm.fr" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L151xH142/compose-ad863.png?1662989144' width='151' height='142' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://compose.obspm.fr" class="spip_out" rel="external">Compose</a> </i> : The online service CompOSE provides data tables for different state of the art equations of state (EoS) ready for further usage in astrophysical applications, nuclear physics and beyond</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1042 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="http://www.deus-consortium.org/deuvo/" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L99xH83/deus-0b819-383eb.png?1662989144' width='99' height='83' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="http://www.deus-consortium.org/deus-data" class="spip_out" rel="external">Deus-Data</a> </i> : This project aims at investigating the imprints of dark energy on cosmic structure formation through very high resolution cosmological simulations</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1046 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://cosmo.obspm.fr/deus-pur-spectra/" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L500xH468/deus_pur_sims-f0415.png?1663028838' width='500' height='468' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://cosmo.obspm.fr/deus-pur-spectra/" class="spip_out" rel="external">Deus-Pur</a> </i> : Database of matter power spectra of the Dark Energy Universe Simulation-Parallel Universe Run simulations</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1041 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="http://exoplanet.eu/" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L362xH112/exoplanet-5c584.png?1662989144' width='362' height='112' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="http://exoplanet.eu/" class="spip_out" rel="external">Exoplanets</a> </i> : Encyclopédie des planètes extrasolaires<br class='autobr' /> Projet démarré au Luth, développé et maintenu par <a href="http://exoplanet.eu/team/" class="spip_out" rel="external">Exoplanet TEAM</a></td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1043 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://gradsvp.obspm.fr" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L500xH83/gradsvp-99656.png?1663028838' width='500' height='83' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://gradsvp.obspm.fr" class="spip_out" rel="external">Gradsvp</a> </i> : Calculation of radiative accelerations in stars</td></tr> </tbody> </table><table class='table spip'> <tbody> <tr class='row_odd odd'> <td><p></p> <div class='spip_document_1048 spip_document spip_documents spip_document_image spip_documents_left spip_document_left'> <figure class="spip_doc_inner"> <a href="https://cosmo.obspm.fr/raygalgroupsims-relativistic-halo-catalogs/" class="spip_out spip_doc_lien"> <img src='https://luthsp3.obspm.fr/local/cache-vignettes/L500xH759/raygal.pngraygal-20b6e.jpg?1663028838' width='500' height='759' alt='' /></a> </figure> </div> <p></p> <p></p> </td> <td><i> <a href="https://cosmo.obspm.fr/raygalgroupsims-relativistic-halo-catalogs/" class="spip_out" rel="external">RayGalGroupSims</a> </i> : The RayGalGroupSims suite consists of a set of N-body simulations of different cosmological models, which have been specifically designed to generate high resolution halo catalogs in redshift-space (light-cone) taking into account for all observable relativistic effects to first order in the weak field approximation</td></tr> </tbody> </table></div></div>