<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dcterms="http://purl.org/dc/terms/">
<rdf:Description rdf:about="https://omeka.ihes.fr/document/P_98_50.pdf">
    <dcterms:title><![CDATA[A New solar system population of WIMP dark matter]]></dcterms:title>
    <dcterms:subject><![CDATA[SYSTEME SOLAIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE SOMBRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[KRAUSS]]></dcterms:creator>
    <dcterms:source><![CDATA[P/98/50]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[06/1998]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[3 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_98_50.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1998]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[KRAUSS]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_98_54.pdf">
    <dcterms:title><![CDATA[Big Bang nucleosynthesis and tensor-scalar gravity]]></dcterms:title>
    <dcterms:subject><![CDATA[BIG BANG]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCUL TENSORIEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[FUSION NUCLEAIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS GRAVITATIONNELS]]></dcterms:subject>
    <dcterms:subject><![CDATA[BARYONS]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[PICHON]]></dcterms:creator>
    <dcterms:source><![CDATA[P/98/54]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/1998]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[15 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_98_54.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1998]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[PICHON]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_98_55.pdf">
    <dcterms:title><![CDATA[A New WIMP population in the solar system and new signals for dark-matter detectors]]></dcterms:title>
    <dcterms:subject><![CDATA[SYSTEME SOLAIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE SOMBRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DETECTEURS DE RAYONNEMENT]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[KRAUSS]]></dcterms:creator>
    <dcterms:source><![CDATA[P/98/55]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/1998]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[20 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_98_55.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1998]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[KRAUSS]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_98_74.pdf">
    <dcterms:title><![CDATA[Effective one-body approach to general relativistic two-body dynamics]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PROBLEME A DEUX CORPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES DOUBLES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE STELLAIRE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BUONANNO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/98/74]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/1998]]></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>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_98_74.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1998]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[BUONANNO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_26.pdf">
    <dcterms:title><![CDATA[k-Inflation]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTROPHYSIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[INFLATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[MECANIQUE ANALYTIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[ARMENDARIZ-PICON]]></dcterms:creator>
    <dcterms:creator><![CDATA[MUKAHNOV]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/26]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/1999]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[11 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_26.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[ARMENDARIZ-PICON]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[MUKHANOV]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_28.pdf">
    <dcterms:title><![CDATA[Equivalence principle and clocks]]></dcterms:title>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[HORLOGES]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS SCALAIRES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/28]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/1999]]></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_99_28.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>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_31.pdf">
    <dcterms:title><![CDATA[Experimental tests of relativistic gravity]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[TESTS]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/31]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/1999]]></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_99_31.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>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_39.pdf">
    <dcterms:title><![CDATA[Implications of a new solar system population of neutralinos on indirect detection rates]]></dcterms:title>
    <dcterms:subject><![CDATA[SYSTEME SOLAIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES]]></dcterms:subject>
    <dcterms:subject><![CDATA[NEUTRALINOS]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE SOMBRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[TRAITEMENT DU SIGNAL]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BERGSTROM]]></dcterms:creator>
    <dcterms:creator><![CDATA[EDSJO]]></dcterms:creator>
    <dcterms:creator><![CDATA[KRAUSS]]></dcterms:creator>
    <dcterms:creator><![CDATA[ULLIO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/39]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/1999]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[10 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_39.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[BERGSTROM]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EDSJO]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[KRAUSS]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[ULLIO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_54.pdf">
    <dcterms:title><![CDATA[Self-gravitating fundamental strings and black holes]]></dcterms:title>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[VENEZIANO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/54]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/1999]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[15 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_54.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[VENEZIANO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_90.pdf">
    <dcterms:title><![CDATA[Transition from inspiral to plunge in binary black hole coalescences]]></dcterms:title>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[ORBITES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MOMENT ANGULAIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[EQUATIONS DIFFERENTIELLES]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BUONANNO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/90]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1999]]></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>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_99_90.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[BUONANNO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_94.pdf">
    <dcterms:title><![CDATA[Strings and black holes]]></dcterms:title>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/94]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1999]]></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_99_94.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>
</rdf:Description><rdf:Description rdf:about="https://omeka.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://omeka.ihes.fr/document/P_00_03.pdf">
    <dcterms:title><![CDATA[Frequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binaries]]></dcterms:title>
    <dcterms:subject><![CDATA[MECANIQUE CELESTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[DETECTEURS]]></dcterms:subject>
    <dcterms:subject><![CDATA[SPECTROMETRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[ONDES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:creator><![CDATA[SATHYAPRAKASH]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/03]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[01/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[26 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_03.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[IYER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SATHYAPRAKASH]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_19.pdf">
    <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>
    <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://omeka.ihes.fr/document/P_00_20.pdf">
    <dcterms:title><![CDATA[Chaos in Superstring Cosmology]]></dcterms:title>
    <dcterms:subject><![CDATA[THEORIE DES SYSTÈME]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAOS]]></dcterms:subject>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[SUPERCORDES]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE NUCLEAIRE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/20]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[3 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_20.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[HENNEAUX]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_32.pdf">
    <dcterms:title><![CDATA[Gravitational wave bursts from cosmic strings]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[CORDES COSMIQUES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[VILENKIN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/32]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[3 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_32.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[VILENKIN]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.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>
    <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://omeka.ihes.fr/document/P_00_47.pdf">
    <dcterms:title><![CDATA[Oscillatory behaviour in homogeneous string cosmology models]]></dcterms:title>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[SUPERCORDES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/47]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/2000]]></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_00_47.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[HENNEAUX]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_60.pdf">
    <dcterms:title><![CDATA[Inconsistency of interacting, multi-graviton theories]]></dcterms:title>
    <dcterms:subject><![CDATA[ESPACE-TEMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES ELEMENTAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[SPIN]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BOULANGER]]></dcterms:creator>
    <dcterms:creator><![CDATA[GUALTIERI]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/60]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[08/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[23 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_60.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[BOULANGER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GUALTIERI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[HENNEAUX]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_62.pdf">
    <dcterms:title><![CDATA[No Consistent cross-interactions for a collection of massless spin-2 fields]]></dcterms:title>
    <dcterms:subject><![CDATA[PHYSIQUE DES HAUTES ENERGIES]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE THEORIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES ELEMENTAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[SPIN]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BOULANGER]]></dcterms:creator>
    <dcterms:creator><![CDATA[GUALTIERI]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/62]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[09/2000]]></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_62.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[BOULANGER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GUALTIERI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[HENNEAUX]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_65.pdf">
    <dcterms:title><![CDATA[La Relativité générale]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[EINSTEIN]]></dcterms:subject>
    <dcterms:subject><![CDATA[ESPACE-TEMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[BIG BANG]]></dcterms:subject>
    <dcterms:subject><![CDATA[BIG CRUNCH]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/65]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[6 f.]]></dcterms:format>
    <dcterms:language><![CDATA[FR]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_00_65.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>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_67.pdf">
    <dcterms:title><![CDATA[A Comparison of search templates for gravitational waves from binary inspiral]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[SOMMABILITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE THEORIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:creator><![CDATA[SATHYAPRAKASH]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/67]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[10 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_67.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[IYER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SATHYAPRAKASH]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.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>
    <dcterms:rightsHolder><![CDATA[SCHAFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_83.pdf">
    <dcterms:title><![CDATA[E10, BE10 and arithmetical chaos in superstring cosmology]]></dcterms:title>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAOS]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MECANIQUE QUANTIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/83]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[3 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_83.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[HENNEAUX]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_01_05.pdf">
    <dcterms:title><![CDATA[The Fate of classical tensor inhomogeneities in pre-big-bang string cosmology]]></dcterms:title>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[BIG BANG]]></dcterms:subject>
    <dcterms:subject><![CDATA[TENSEUR]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BUONANNO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/01/05]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[02/2001]]></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_01_05.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[BUONANNO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_01_11.pdf">
    <dcterms:title><![CDATA[Coalescence of two spinning black holes : an Effective one-body approach]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTROPHYSIQUE RELATIVISTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[SYSTEME BANAIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/01/11]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/2001]]></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_01_11.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>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_01_12.pdf">
    <dcterms:title><![CDATA[Hyperbolic Kac-Moody algebras and chaos in Kaluza-Klein models]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTROPHYSIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[COSMOLOGIE QUANTIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[ALGEBRES DE KAC-MOODY]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIES DE KALUZA-KLEIN]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:creator><![CDATA[JULIA]]></dcterms:creator>
    <dcterms:creator><![CDATA[NICOLAI]]></dcterms:creator>
    <dcterms:source><![CDATA[P/01/12]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/2001]]></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_01_12.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[HENNEAUX]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JULIA]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[NICOLAI]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_01_15.pdf">
    <dcterms:title><![CDATA[Gravitational wave bursts from cusps and kinks on cosmic strings]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[ASTROPHYSIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES  DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[VILENKIN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/01/15]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/2001]]></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_01_15.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[VILENKIN]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.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://omeka.ihes.fr/document/P_01_44.pdf">
    <dcterms:title><![CDATA[Questioning the equivalence principle]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MASSE]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/01/44]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[09/2001]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[8 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_01_44.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>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_06.pdf">
    <dcterms:title><![CDATA[Kasner-like behaviour for subcritical Einstein-matter systems]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[COSMOLOGIE QUANTIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE DES HAUTES ENERGIES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:creator><![CDATA[RENDALL]]></dcterms:creator>
    <dcterms:creator><![CDATA[WEAVER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/06]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[02/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[29 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_06.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[HENNEAUX]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[RENDALL]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[WEAVER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_08.pdf">
    <dcterms:title><![CDATA[Implications of a solar-system population of massive 4th generation neutrinos for underground searches of monochromatic neutrinos-annihilation signals]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTROPHYSIQUE DES NEUTRINOS]]></dcterms:subject>
    <dcterms:subject><![CDATA[GEOPHYSIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE]]></dcterms:subject>
    <dcterms:subject><![CDATA[SOLEIL]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BELOTSKY]]></dcterms:creator>
    <dcterms:creator><![CDATA[KHLOPOV]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/08]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[02/2002]]></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_02_08.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[BELOTSKY]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[KHLOPOV]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_09.pdf">
    <dcterms:title><![CDATA[Violations of the equivalence principle in a dilaton-runaway scenario]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MASSE]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE QUANTIQUE DES CHAMPS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[PIAZZA]]></dcterms:creator>
    <dcterms:creator><![CDATA[VENEZIANO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/09]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[17 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_09.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[PIAZZA]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[VENEZIANO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_10.pdf">
    <dcterms:title><![CDATA[Circular orbits of corotating binary black holes : comparison between analytical and numerical results]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[GOURGOULHON]]></dcterms:creator>
    <dcterms:creator><![CDATA[GRANDCLEMENT]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/10]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[11 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_10.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[GOURGOULHON]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GRANDCLEMENT]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_22.pdf">
    <dcterms:title><![CDATA[String cosmology and chaos]]></dcterms:title>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAOS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/22]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/2002]]></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_02_22.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>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_27.pdf">
    <dcterms:title><![CDATA[Runaway dilaton and equivalence principle violations]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MASSE]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE SOMBRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[ENERGIE SOMBRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE QUANTIQUE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:subject><![CDATA[EXPERIENCES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[PIAZZA]]></dcterms:creator>
    <dcterms:creator><![CDATA[VENEZIANO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/27]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[3 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_27.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[PIAZZA]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[VENEZIANO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_34.pdf">
    <dcterms:title><![CDATA[Non-Linear bigravity and cosmic acceleration]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIES DE KALUZA-KLEIN]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[COMPACTIFICATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITE QUANTIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[KOGAN]]></dcterms:creator>
    <dcterms:creator><![CDATA[PAPAZOGLOU]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/34]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[06/2002]]></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>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_02_34.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[KOGAN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[PAPAZOGLOU]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_35.pdf">
    <dcterms:title><![CDATA[Effective Lagrangians and universality classes of nonlinear bigravity]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[UNIVERS]]></dcterms:subject>
    <dcterms:subject><![CDATA[BIG BANG]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[KOGAN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/35]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[06/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[21 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_35.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[KOGAN]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_43.pdf">
    <dcterms:title><![CDATA[Einstein billiards and overextensions of finite-dimensional simple Lie algebras]]></dcterms:title>
    <dcterms:subject><![CDATA[THEORIE DE LA GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[SUPERGRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[ALGEBRES DE LIE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[DE BUYL]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHOMBLOND]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/43]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[06/2002]]></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_02_43.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[DE BUYL]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[HENNEAUX]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHOMBLOND]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_48.pdf">
    <dcterms:title><![CDATA[E10 and a &quot;small tension expansion&#039;&#039; of M theory]]></dcterms:title>
    <dcterms:subject><![CDATA[SUPERGRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[INVARIANCE DE JAUGE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE SOMBRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[SUPERCODRES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:creator><![CDATA[NICOLAI]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/48]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[3 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_48.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[HENNEAUX]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[NICOLAI]]></dcterms:rightsHolder>
</rdf:Description></rdf:RDF>