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<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>
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    <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>
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</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>
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</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>
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    <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>
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    <dcterms:date><![CDATA[03/2000]]></dcterms:date>
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    <dcterms:format><![CDATA[3 f.]]></dcterms:format>
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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_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>
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    <dcterms:creator><![CDATA[VILENKIN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/32]]></dcterms:source>
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    <dcterms:date><![CDATA[04/2000]]></dcterms:date>
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    <dcterms:format><![CDATA[3 f.]]></dcterms:format>
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</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>
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    <dcterms:format><![CDATA[14 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <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>
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    <dcterms:format><![CDATA[7 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[HENNEAUX]]></dcterms:rightsHolder>
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    <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>
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    <dcterms:format><![CDATA[23 f.]]></dcterms:format>
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    <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>
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    <dcterms:format><![CDATA[8 f.]]></dcterms:format>
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    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
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    <dcterms:rightsHolder><![CDATA[BOULANGER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GUALTIERI]]></dcterms:rightsHolder>
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</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>
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    <dcterms:format><![CDATA[6 f.]]></dcterms:format>
    <dcterms:language><![CDATA[FR]]></dcterms:language>
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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_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>
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    <dcterms:format><![CDATA[10 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <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>
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    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/74]]></dcterms:source>
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</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>
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    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
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    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
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    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
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    <dcterms:format><![CDATA[3 f.]]></dcterms:format>
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</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>
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    <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>
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    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[02/2001]]></dcterms:date>
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    <dcterms:format><![CDATA[9 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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</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>
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    <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>
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    <dcterms:date><![CDATA[03/2001]]></dcterms:date>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:title><![CDATA[Hyperbolic Kac-Moody algebras and chaos in Kaluza-Klein models]]></dcterms:title>
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    <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>
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    <dcterms:date><![CDATA[03/2001]]></dcterms:date>
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</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>
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    <dcterms:subject><![CDATA[ASTROPHYSIQUE]]></dcterms:subject>
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    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[VILENKIN]]></dcterms:creator>
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    <dcterms:date><![CDATA[04/2001]]></dcterms:date>
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    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <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>
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    <dcterms:date><![CDATA[05/2001]]></dcterms:date>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[SCHAFFER]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Questioning the equivalence principle]]></dcterms:title>
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    <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>
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    <dcterms:date><![CDATA[09/2001]]></dcterms:date>
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    <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>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <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>
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    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:creator><![CDATA[RENDALL]]></dcterms:creator>
    <dcterms:creator><![CDATA[WEAVER]]></dcterms:creator>
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    <dcterms:date><![CDATA[02/2002]]></dcterms:date>
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    <dcterms:format><![CDATA[29 f.]]></dcterms:format>
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    <dcterms:rightsHolder><![CDATA[HENNEAUX]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[RENDALL]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Implications of a solar-system population of massive 4th generation neutrinos for underground searches of monochromatic neutrinos-annihilation signals]]></dcterms:title>
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    <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>
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    <dcterms:title><![CDATA[Violations of the equivalence principle in a dilaton-runaway scenario]]></dcterms:title>
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    <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>
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    <dcterms:format><![CDATA[17 f.]]></dcterms:format>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[PIAZZA]]></dcterms:rightsHolder>
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    <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>
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    <dcterms:format><![CDATA[11 f.]]></dcterms:format>
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    <dcterms:coverage><![CDATA[2002]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <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:Description rdf:about="https://omeka.ihes.fr/document/P_02_72.pdf">
    <dcterms:title><![CDATA[Billiard dynamics of Einstein-matter systems near a spacelike singularity]]></dcterms:title>
    <dcterms:subject><![CDATA[MOUVEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[BILLARD]]></dcterms:subject>
    <dcterms:subject><![CDATA[GEOMETRIE HYPERBOLIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[ESPACE-TEMPS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:creator><![CDATA[NICOLAI]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/72]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/2002]]></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_72.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:Description rdf:about="https://omeka.ihes.fr/document/P_02_75.pdf">
    <dcterms:title><![CDATA[String theory, cosmology and varying constants]]></dcterms:title>
    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CONSTANTES DE COUPLAGE]]></dcterms:subject>
    <dcterms:subject><![CDATA[EXPERIENCES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/75]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/2002]]></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_02_75.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_77.pdf">
    <dcterms:title><![CDATA[A comparison of search templates for gravitational waves from binary inspiral -3.5PN update]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:subject><![CDATA[APPROXIMATION DE PADE]]></dcterms:subject>
    <dcterms:subject><![CDATA[LASERS]]></dcterms:subject>
    <dcterms:subject><![CDATA[TRAITEMENT DU SIGNAL]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:creator><![CDATA[SATHYAPRAKASH]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/77]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/2000]]></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_02_77.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[SATHYAPRAKASH]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.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://omeka.ihes.fr/document/P_64_03.pdf">
    <dcterms:title><![CDATA[Non-positivity of the energy density in quantized field theories]]></dcterms:title>
    <dcterms:subject><![CDATA[DENSITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[ENERGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:description><![CDATA[Abstract : It is shown that a positive definite local energy density is incompatible with the usual postulates of local field theory. The question whether it can be bounded below is briefly discussed but not solved.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[GLASER]]></dcterms:creator>
    <dcterms:creator><![CDATA[JAFFE]]></dcterms:creator>
    <dcterms:source><![CDATA[P/64/03]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1964]]></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_64_03.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1964]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GLASER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JAFFE]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_72_10.pdf">
    <dcterms:title><![CDATA[Renormalization of non polynomial Lagrangians in Jaffe&#039;s class]]></dcterms:title>
    <dcterms:subject><![CDATA[RESEAUX CEREBRAUX]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE STATISTIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[SYSTEMES COMPLEXES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIES NON LINEAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[INFORMATIQUE QUANTIQUE]]></dcterms:subject>
    <dcterms:description><![CDATA[Abstract : t, It is shown how a renormalized perturbation series can be defined for a<br />
theory with strictly locaI, non-polynomial, interacting Lagrangian<br />
:A(x)r: 2e(x) = )__, t,-----<br />
r=O r!<br />
so as to preserve locality at every order. ]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[GLASER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/72/10]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[1972]]></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_72_10.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1972]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GLASER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JAFFE]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_73_41.pdf">
    <dcterms:title><![CDATA[Remarks on two theorems of E. Lieb]]></dcterms:title>
    <dcterms:subject><![CDATA[RESEAUX CEREBRAUX]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE STATISTIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[SYSTEMES COMPLEXES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIES NON LINEAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[INFORMATIQUE QUANTIQUE]]></dcterms:subject>
    <dcterms:description><![CDATA[Abstract : The concavity of two functions of a positive matrixA, Tr exp(B + logA) and TrA r KA p K* (whereB=B* andK are fixed matrices), recently proved by Lieb, can also be obtained by using the theory of Herglotz functions.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/73/41]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[02/1973]]></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_73_41.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1973]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_73_60.pdf">
    <dcterms:title><![CDATA[Quelques Aspects globaux des problèmes d&#039;Edge-of-the-wedge]]></dcterms:title>
    <dcterms:subject><![CDATA[HYPERFONCTIONS]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:description><![CDATA[Contribution au Colloque sur les Hyperfonctions et leurs applications, Nice, mai 1973<br />
Abstract : Cet exposé décrit birèvement quelques résultats obtenus entre 1961et 1963. Certains d&#039;entre eux ont été publiés dans [1], [2], [3]. D&#039;autres n&#039;ont pas encore été publiés. L&#039;accent est mis sur l&#039;aspect global des problèmes du typ d&#039;edge-of-the-wedge.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[BROS]]></dcterms:creator>
    <dcterms:creator><![CDATA[GLASER]]></dcterms:creator>
    <dcterms:creator><![CDATA[STORA]]></dcterms:creator>
    <dcterms:source><![CDATA[P/73/60]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[08/1973]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[36 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_73_60.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1973]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[BROS]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GLASER]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[STORA]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_78_227.pdf">
    <dcterms:title><![CDATA[Time-ordered products and Schwinger functions]]></dcterms:title>
    <dcterms:subject><![CDATA[RESEAUX CEREBRAUX]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[SYSTEMES COMPLEXES]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE STATISTIQUE]]></dcterms:subject>
    <dcterms:description><![CDATA[Abstract : It is shown that every system of time-ordered products for a local field theory determines a related system of Schwinger functions possessing an extended form of Osterwalder-Schrader positivity and that the converse is true provided certain growth conditions are satisfied. This is applied to the ? 3 4 theory and it is shown that the time-ordered functions andS-matrix elements admit the standard perturbation series as asymptotic expansions.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[ECKMANN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/78/227]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[1978]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[35 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_78_227.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1978]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[ECKMANN]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_79_255.pdf">
    <dcterms:title><![CDATA[Borel summability of the mass and the s-matrix in ?4 models]]></dcterms:title>
    <dcterms:subject><![CDATA[PHYSIQUE THEORIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[SOMMABILITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MODELES MATHEMATIQUES]]></dcterms:subject>
    <dcterms:description><![CDATA[Abstract : We show that in the ?{2/4} theory, the physical mass and the two-body S-matrix are Borel summable in the coupling constant ? at ?=0.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[ECKMANN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/79/255]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[02/1979]]></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_79_255.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1979]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[ECKMANN]]></dcterms:rightsHolder>
</rdf:Description></rdf:RDF>
