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    <dcterms:subject><![CDATA[CHAMPS GRAVITATIONNELS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BLANCHET]]></dcterms:creator>
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    <dcterms:date><![CDATA[03/1989]]></dcterms:date>
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    <dcterms:format><![CDATA[22 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:language><![CDATA[FR]]></dcterms:language>
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    <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>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_89_59.pdf">
    <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>
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    <dcterms:date><![CDATA[09/1989]]></dcterms:date>
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    <dcterms:format><![CDATA[27 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:identifier><![CDATA[P_89_59.pdf]]></dcterms:identifier>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_03.pdf">
    <dcterms:title><![CDATA[Dark matter, time-varying G and a dilaton field]]></dcterms:title>
    <dcterms:subject><![CDATA[MATIERE NOIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CONSTANTE COSMOLOGIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[GIBBONS]]></dcterms:creator>
    <dcterms:creator><![CDATA[GUNDLACH]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/03]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/1990]]></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_90_03.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[GIBBONS]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GUNDLACH]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_32.pdf">
    <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>
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    <dcterms:date><![CDATA[05/1990]]></dcterms:date>
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    <dcterms:format><![CDATA[13 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <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>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_41.pdf">
    <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>
    <dcterms:source><![CDATA[P/90/41]]></dcterms:source>
    <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>
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    <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>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_59.pdf">
    <dcterms:title><![CDATA[Multipole analysis for electromagnetism and linearized gravity with irreducible Cartesian tensors]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS ELECTROMAGNETIQUES]]></dcterms:subject>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/59]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[19 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_59.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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</rdf:Description><rdf:Description rdf:about="https://omeka.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>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_82.pdf">
    <dcterms:title><![CDATA[A New approach to the general relativistic N-body problem]]></dcterms:title>
    <dcterms:subject><![CDATA[EQUATIONS DU MOUVEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SOFFEL]]></dcterms:creator>
    <dcterms:creator><![CDATA[XU]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/82]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/1990]]></dcterms:date>
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    <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_82.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[XU]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_85.pdf">
    <dcterms:title><![CDATA[Post-Newtonian generation of gravitational waves II. The Spin moments]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[SPIN]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS GRAVITATIONNELS]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCUL TENSORIEL]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/85]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[32 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_90_85.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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</rdf:Description><rdf:Description rdf:about="https://omeka.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>
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    <dcterms:rightsHolder><![CDATA[SOFFEL]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[XU]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_88.pdf">
    <dcterms:title><![CDATA[Nucleosynthesis constraints on an extended Jordan-Brans-Dicke theory]]></dcterms:title>
    <dcterms:subject><![CDATA[NUCLEOSYNTHESE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS SCALAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE SOMBRE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[GUNDLACH]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/88]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[9 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_88.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[GUNDLACH]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.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>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_91_63.pdf">
    <dcterms:title><![CDATA[Strong-field tests of relativistic gravity and binary pulsars]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PULSARS]]></dcterms:subject>
    <dcterms:subject><![CDATA[SYSTEMES BINAIRES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[TAYLOR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/91/63]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[09/1991]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[33 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_63.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
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    <dcterms:rightsHolder><![CDATA[TAYLOR]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.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>
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    <dcterms:creator><![CDATA[WEISBERG]]></dcterms:creator>
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    <dcterms:title><![CDATA[General relativity and experiment : a brief review]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[EXPERIENCES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <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>
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    <dcterms:date><![CDATA[10/1991]]></dcterms:date>
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    <dcterms:format><![CDATA[40 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:identifier><![CDATA[P_91_72.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_91_82.pdf">
    <dcterms:title><![CDATA[Theoretical problems in nonsymmetric gravitational theory]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[ENERGIE NEGATIVE]]></dcterms:subject>
    <dcterms:subject><![CDATA[FORMALISME]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[DESER]]></dcterms:creator>
    <dcterms:creator><![CDATA[MC CARTHY]]></dcterms:creator>
    <dcterms:source><![CDATA[P/91/82]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1991]]></dcterms:date>
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    <dcterms:format><![CDATA[4 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
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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>
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    <dcterms:format><![CDATA[49 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[ESPOSITO-FARESE]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_92_25.pdf">
    <dcterms:title><![CDATA[Testing the Lorentz invariance of gravity with binary-pulsar data]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PULSARS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[ESPOSITO-FARESE]]></dcterms:creator>
    <dcterms:source><![CDATA[P/92/25]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/1992]]></dcterms:date>
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    <dcterms:format><![CDATA[7 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[1992]]></dcterms:coverage>
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    <dcterms:title><![CDATA[Nonsymmetric gravity theories : inconsistencies and a cure]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[DESER]]></dcterms:creator>
    <dcterms:creator><![CDATA[MC CARTHY]]></dcterms:creator>
    <dcterms:source><![CDATA[P/92/36]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[06/1992]]></dcterms:date>
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    <dcterms:format><![CDATA[18 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[1992]]></dcterms:coverage>
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    <dcterms:title><![CDATA[Hereditary effects in gravitational radiation]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BLANCHET]]></dcterms:creator>
    <dcterms:source><![CDATA[P/92/42]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/1992]]></dcterms:date>
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    <dcterms:coverage><![CDATA[1992]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:title><![CDATA[General relativistic celestial mechanics. III - Rotational equations of motion]]></dcterms:title>
    <dcterms:subject><![CDATA[MECANIQUE CELESTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[EQUATIONS DU MOUVEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SOFFEL]]></dcterms:creator>
    <dcterms:creator><![CDATA[XU]]></dcterms:creator>
    <dcterms:source><![CDATA[P/92/87]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/1992]]></dcterms:date>
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    <dcterms:format><![CDATA[13 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[1992]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_92_93.pdf">
    <dcterms:title><![CDATA[On some Links between mathematical physics and physics in the context of general relativity]]></dcterms:title>
    <dcterms:subject><![CDATA[PHYSIQUE MATHEMATIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/92/93]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1992]]></dcterms:date>
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    <dcterms:format><![CDATA[5 f.]]></dcterms:format>
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    <dcterms:identifier><![CDATA[P_92_93.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1992]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:title><![CDATA[General relativity as a cosmological attractor of tensor-scalar theories]]></dcterms:title>
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    <dcterms:subject><![CDATA[SCALARS]]></dcterms:subject>
    <dcterms:subject><![CDATA[TENSEURS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[NORDTVEDT]]></dcterms:creator>
    <dcterms:source><![CDATA[P/92/94]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1992]]></dcterms:date>
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    <dcterms:format><![CDATA[4 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[1992]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[NORDTVEDT]]></dcterms:rightsHolder>
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