Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity

https://repo-archives.ihes.fr/FONDS_IHES/I_Prepublications/DAMOUR/1988-1993/P_89_59/P_89_59.pdf

Auteur(e.s) : DAMOUR

Date : 09/1989

Sujet(s) : ASTROPHYSIQUE

Source : P/89/59

©IHES

Mots-clés

1989, ARNOLD, ARNOWITT, ASTROPHYSIQUE, BAO, BLANCHET, BONAZZOLA, BURKE, CAPORALI, CARTER, CHANDRASEKHAR, DAMOUR, DESER, EINSTEIN, EN, ESPOSTITO, FINN, GAFFET, GRAVITATION, HAMILTON, HOLM, HYDRODYNAMIQUE, INFORMATIQUE, KIRILLOV, KOSTANT, KUNZLE, KUNZNETSOV, LAPLACE, LICHNEROWICZ, LIE, MARCK, MARSDEN, MINKOWSKI, MISNER, NAKAURA, NESTER, NEWTON, NUTKU, POISSON, PREPUBLICATION, PRIAN, RAYONNEMENT GRAVITATIONNEL, RELATIVITE, SCHAFER, STARK, THORNE, WALTON, ZAKHAROV

Citer ce document

DAMOUR, BLANCHET, et SCHAFER, “Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity,” Archives de l'IHES, consulté le 12 octobre 2026, https://archives.ihes.fr/document/P_89_59.pdf.

Formats de sortie

atom
dc-rdf
dcmes-xml
json
omeka-json
omeka-xml