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<rdf:Description rdf:about="https://archives.ihes.fr/document/P_95_100.pdf">
    <dcterms:title><![CDATA[A Tighter test of the local Lorentz invariance of gravity using PSR J2317+1439]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[TESTS]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE RESTREINTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[LORENTZ]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[PULSARS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BELL]]></dcterms:creator>
    <dcterms:creator><![CDATA[CAMILO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/95/100]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1995]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[4 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:identifier><![CDATA[P_95_100.pdf]]></dcterms:identifier>
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    <dcterms:rightsHolder><![CDATA[CAMILO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_95_25.pdf">
    <dcterms:title><![CDATA[Conservation laws for sysmems of extended  bodies in the first post-Newtonian approximation]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MOMENTS QUADRUPOLAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MASSE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[VOKROUHLICKY]]></dcterms:creator>
    <dcterms:source><![CDATA[P/95/25]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/1995]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[7 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:identifier><![CDATA[P_95_25.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1995]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[VOKROUHLICKY]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_01_19.pdf">
    <dcterms:title><![CDATA[Dimensional regularization of the gravitational interaction of point masses]]></dcterms:title>
    <dcterms:subject><![CDATA[SYSTEMES BINAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[EQUATIONS DU MOUVEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MASSE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/01/19]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/2001]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[5 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_01_19.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2001]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_99_95.pdf">
    <dcterms:title><![CDATA[Dynamical invariants for general relativistic two-body systems at the third post-Newtonian approximation]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[INVARIANTS]]></dcterms:subject>
    <dcterms:subject><![CDATA[MASSE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/95]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1999]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[12 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_99_95.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1999]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_00_74.pdf">
    <dcterms:title><![CDATA[Equivalence between the ADM-Hamiltonian and the harmonic-coordinates approaches to the third post-Newtonian dynamics of compact binaries]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTRONOMIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES A NEUTRONS]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE STATISTIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/74]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[8 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_00_74.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
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</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_91_65.pdf">
    <dcterms:title><![CDATA[Experimental constraints on strong-field relativistic gravity]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMP GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[EXPERIENCES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[TAYLOR]]></dcterms:creator>
    <dcterms:creator><![CDATA[WOLSZCZAN]]></dcterms:creator>
    <dcterms:creator><![CDATA[WEISBERG]]></dcterms:creator>
    <dcterms:source><![CDATA[P/91/65]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/1991]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[8 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_91_65.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[TAYLOR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[WOLSZCZAN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[WEISBERG]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_90_87.pdf">
    <dcterms:title><![CDATA[General relativistic celestial mechanics. I - Method and definition of reference systems]]></dcterms:title>
    <dcterms:subject><![CDATA[MECANIQUE CELESTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[METHODOLOGIE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SOFFEL]]></dcterms:creator>
    <dcterms:creator><![CDATA[XU]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/87]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[41 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_90_87.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SOFFEL]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[XU]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_91_72.pdf">
    <dcterms:title><![CDATA[General relativistic celestial mechanics. II - Translational equations of motion]]></dcterms:title>
    <dcterms:subject><![CDATA[MECANIQUE CELESTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[EQUATIONS DU MOUVEMENT]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SOFFEL]]></dcterms:creator>
    <dcterms:creator><![CDATA[XU]]></dcterms:creator>
    <dcterms:source><![CDATA[P/91/72]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/1991]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[40 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_91_72.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SOFFEL]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[XU]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_02_78.pdf">
    <dcterms:title><![CDATA[Gravitational waves from black hole binary inspiral and merger : The span of third post-Newtonian effective-one-body templates]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE QUANTIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[DETECTEURS DE RAYONNEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[SPECTROMETRES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:creator><![CDATA[SATHYAPRAKASH]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/78]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[13 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_02_78.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2002]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[IYER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SATHYAPRAKASH]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_90_60.pdf">
    <dcterms:title><![CDATA[Levi-Civita and the general relativistic problem of motion]]></dcterms:title>
    <dcterms:subject><![CDATA[LEVI-CIVITA]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MECANIQUE ANALYTIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MOUVEMENT]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/60]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[7 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_90_60.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_91_31.pdf">
    <dcterms:title><![CDATA[New tests of the strong equivalence principle using binary-pulsar data]]></dcterms:title>
    <dcterms:subject><![CDATA[PULSARS]]></dcterms:subject>
    <dcterms:subject><![CDATA[EXPLORATION DE DONNEES]]></dcterms:subject>
    <dcterms:subject><![CDATA[INTERACTIONS GRAVITATIONNELLES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/91/31]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/1991]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[6 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_91_31.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://archives.ihes.fr/document/P_00_37.pdf">
    <dcterms:title><![CDATA[On the Determination of the last stable orbit for circular general relativistic binaries at the third post-Newtonian approximation]]></dcterms:title>
    <dcterms:subject><![CDATA[ORBITES]]></dcterms:subject>
    <dcterms:subject><![CDATA[ANALYSE NUMERIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[INVARIANTS]]></dcterms:subject>
    <dcterms:subject><![CDATA[INVARIANCE DE JAUGE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/37]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[14 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_00_37.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:title><![CDATA[On the Orbital period change of the binary pulsar PSR 1913+16]]></dcterms:title>
    <dcterms:subject><![CDATA[ETOILES BINAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[PULSARS]]></dcterms:subject>
    <dcterms:subject><![CDATA[VOIE LACTEE]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE STELLAIRE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[TAYLOR]]></dcterms:creator>
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    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[18 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_90_41.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
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    <dcterms:rightsHolder><![CDATA[TAYLOR]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Poincaré invariance in the ADM Hamiltonian approach to the general relativistic two-body problem]]></dcterms:title>
    <dcterms:subject><![CDATA[MECANIQUE CELESTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[ONDES]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES A NEUTRONS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/19]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[5 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_00_19.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
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    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFFER]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Post-Newtonian generation of gravitational waves]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVIATATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS GRAVITATIONNELS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BLANCHET]]></dcterms:creator>
    <dcterms:source><![CDATA[P/89/18]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/1989]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[22 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:language><![CDATA[FR]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_89_18.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1989]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
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    <dcterms:rightsHolder><![CDATA[BLANCHET]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTROPHYSIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[INFORMATIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[HYDRODYNAMIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BLANCHET]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/89/59]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[09/1989]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[27 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
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    <dcterms:identifier><![CDATA[P_89_59.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1989]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
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    <dcterms:rightsHolder><![CDATA[BLANCHET]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Redefinition of position variables and the reduction of higher-order Lagrangians]]></dcterms:title>
    <dcterms:subject><![CDATA[EQUATIONS DU MOUVEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[VARIABLES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/32]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[13 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_90_32.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
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    <dcterms:rightsHolder><![CDATA[SCHAFER]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Tensor-multi-scalar theories of gravitation]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[SCALARS]]></dcterms:subject>
    <dcterms:subject><![CDATA[TENSEURS]]></dcterms:subject>
    <dcterms:subject><![CDATA[PROBLEME DES N CORPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS GRAVITATIONNELS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[ESPOSITO-FARESE]]></dcterms:creator>
    <dcterms:source><![CDATA[P/91/93]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1991]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[49 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_91_93.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[ESPOSITO-FARESE]]></dcterms:rightsHolder>
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