<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_85_55.pdf">
    <dcterms:title><![CDATA[News proofs of the existence of the Feigenbaum functions]]></dcterms:title>
    <dcterms:subject><![CDATA[EQUATIONS FONCTIONNELLES]]></dcterms:subject>
    <dcterms:subject><![CDATA[SYSTEMES DYNAMIQUES]]></dcterms:subject>
    <dcterms:description><![CDATA[Abstract : A new proof of the existence of analytic, unimodal soutions of the Cvitanovic-Feigenbaum functional equation ?g (x) = -g(g-?x)), g(x) ? 1-const. |x| r at 0, walid for all ? in (0,1), is given, and the existence of the Eckmann-Wittwer functions [8] is recovered. The method also provides the existence of solutions for certain given values of r, and in particular, for r=2, a proof requiring no computer.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/85/55]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/1985]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[22 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_85_55.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1985]]></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_83_70.pdf">
    <dcterms:title><![CDATA[Scaling of Mandelbrot sets generated by critical point preperiodicity]]></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[THEORIES NON LINEAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE]]></dcterms:subject>
    <dcterms:description><![CDATA[Astract : Letz?f?(z) be a complex holomorphic function depending holomorphically on the complex parameter ?. If, for ?=0, a critical point off0 falls after a finite number of steps onto an unstable fixed point off0, then, in the parameter space, near 0, an infinity of more and more accurate copies of the Mandelbrot set appears. We compute their scaling properties.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[ECKMANN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/83/70]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/1983]]></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_83_70.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1983]]></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_81_27.pdf">
    <dcterms:title><![CDATA[Analyticity properties of the Feigenbaum function]]></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[THEORIES NON LINEAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[INFORMATIQUE QUANTIQUE]]></dcterms:subject>
    <dcterms:description><![CDATA[Absract : Analyticity properties of the Feigenbaum function [a solution ofg(x)=???1g(g(?x)) withg(0)=1,g?(0)=0,g?(0)&lt;0] are investigated by studying its inverse function which turns out to be Herglotz or anti-Herglotz on all its sheets. It is found thatg is analytic and uniform in a domain with a natural boundary.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[LASCOUX]]></dcterms:creator>
    <dcterms:source><![CDATA[P/81/27]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/1981]]></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_81_27.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1981]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[LASCOUX]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_80_35.pdf">
    <dcterms:title><![CDATA[On the existence of Fegeinbaum&#039;s fixed point]]></dcterms:title>
    <dcterms:subject><![CDATA[RESEAUX CEREBRAUX]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE STATISTIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[ANALYSE FONCTIONNELLE]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIES NON LINEAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE]]></dcterms:subject>
    <dcterms:description><![CDATA[Abstract : We give a proof of the existence of aC2, even solution of Feigenbaum&#039;s functional equation<br />
g(x)=???10g(g(??0x)),g(0) = 1,<br />
whereg is a map of [?1, 1] into itself. It extends to a real analytic function over ?.]]></dcterms:description>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[CAMPANINO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/80/35]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[1980]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[38 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_80_35.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1980]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[CAMPANINO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_80_32.pdf">
    <dcterms:title><![CDATA[On Feigenbaum&#039;s functional equation g°g (?x) + ?g (x) =0]]></dcterms:title>
    <dcterms:subject><![CDATA[EQUATIONS FONCTIONNELLES]]></dcterms:subject>
    <dcterms:creator><![CDATA[EPSTEIN]]></dcterms:creator>
    <dcterms:creator><![CDATA[RUELLE]]></dcterms:creator>
    <dcterms:creator><![CDATA[CAMPANINO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/80/32]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[07/1980]]></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_80_32.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1980]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[EPSTEIN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[RUELLE]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[CAMPANINO]]></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: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_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_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_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_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_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>
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    <dcterms:coverage><![CDATA[2002]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
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    <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_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>
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    <dcterms:format><![CDATA[3 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <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_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_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>
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    <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_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>
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    <dcterms:format><![CDATA[3 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <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_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_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_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_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_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_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_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>
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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[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[MATIERE]]></dcterms:subject>
    <dcterms:subject><![CDATA[SOLEIL]]></dcterms:subject>
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    <dcterms:creator><![CDATA[BELOTSKY]]></dcterms:creator>
    <dcterms:creator><![CDATA[KHLOPOV]]></dcterms:creator>
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    <dcterms:format><![CDATA[9 f.]]></dcterms:format>
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</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>
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    <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: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>
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    <dcterms:source><![CDATA[P/01/44]]></dcterms:source>
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    <dcterms:date><![CDATA[09/2001]]></dcterms:date>
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    <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[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>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFFER]]></dcterms:rightsHolder>
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    <dcterms:title><![CDATA[Gravitational wave bursts from cusps and kinks on cosmic strings]]></dcterms:title>
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    <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>
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    <dcterms:format><![CDATA[13 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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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>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/2001]]></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[Coalescence of two spinning black holes : an Effective one-body approach]]></dcterms:title>
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    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
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    <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:format><![CDATA[14 f.]]></dcterms:format>
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    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <dcterms:title><![CDATA[The Fate of classical tensor inhomogeneities in pre-big-bang string cosmology]]></dcterms:title>
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    <dcterms:subject><![CDATA[TENSEUR]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
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    <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>
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    <dcterms:format><![CDATA[9 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:coverage><![CDATA[2001]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
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    <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:creator><![CDATA[HENNEAUX]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/83]]></dcterms:source>
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    <dcterms:date><![CDATA[12/2000]]></dcterms:date>
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    <dcterms:format><![CDATA[3 f.]]></dcterms:format>
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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>
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    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
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    <dcterms:date><![CDATA[11/2000]]></dcterms:date>
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    <dcterms:language><![CDATA[EN]]></dcterms:language>
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    <dcterms:title><![CDATA[A Comparison of search templates for gravitational waves from binary inspiral]]></dcterms:title>
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    <dcterms:subject><![CDATA[SOMMABILITE]]></dcterms:subject>
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    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:creator><![CDATA[SATHYAPRAKASH]]></dcterms:creator>
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    <dcterms:format><![CDATA[10 f.]]></dcterms:format>
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    <dcterms:title><![CDATA[La Relativité générale]]></dcterms:title>
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    <dcterms:subject><![CDATA[EINSTEIN]]></dcterms:subject>
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    <dcterms:date><![CDATA[10/2000]]></dcterms:date>
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    <dcterms:format><![CDATA[6 f.]]></dcterms:format>
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    <dcterms:title><![CDATA[No Consistent cross-interactions for a collection of massless spin-2 fields]]></dcterms:title>
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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>
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    <dcterms:title><![CDATA[Oscillatory behaviour in homogeneous string cosmology models]]></dcterms:title>
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    <dcterms:subject><![CDATA[MODELES DES CORDES VIBRANTES]]></dcterms:subject>
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    <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>
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    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
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    <dcterms:title><![CDATA[Gravitational wave bursts from cosmic strings]]></dcterms:title>
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    <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>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/2000]]></dcterms:date>
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