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Institute of Physics - Rennes (IPR) - Open Access Repository

HAL-IPR is an open access repository providing access to the publication output of the IPR Research Unit.

Director: Jean-Christophe Sangleboeuf

Research teams:

Université Rennes 1, Institut de Physique de Rennes, UMR CNRS 6251 - Bât. 11 A, B, C, 263
av. Général Leclerc, 35042 Rennes cedex FRANCE

Latest Additions

                          OSUR
   

Full Text Publications

1 240

Bibliographic Records

3 935

Keywords

Temperature Kinetics Strain-induced crystallization Chemical physics Astrophysics Foams Viscoelasticity Membrane Line profiles Self-assembly Adsorption Spin crossover Chalcogenide glasses Astrochemistry X-ray diffraction Optical fibers Interface Stars fundamental parameters Chalcogenide glass Nanoparticles Integrated photonics Astrophysics laboratory Lysozyme Traitement thermique Propriété physicochimique Atomic and molecular physics AFM SAXS MCTDH Rheology LIGO DYNAMICS Indentation Protéine Molecular physics Density functional theory Foam Collisions Silicon Microscopie à force atomique Vibronic couplings Infrared thermography Charge transfer Thin films Magnetic properties Gravitational radiation Potential energy surfaces Gravitational radiation emission Low temperature chemical kinetics Water Rhéologie Microfluidics XPS Organic compounds Helium clusters Reaction kinetics and dynamics Elasticity Bubbles Interfaces Asteroseismology Densification Milieux granulaires Iron Natural rubber Atomic force microscopy Copper Ellipsometry Phase transitions Contact resistance Cold and ultra-cold collisions Quantum Monte Carlo Mousse Spectroscopy Models Optical fiber Fracture toughness Phase transition Granular media Diffusion Stars interiors Cavitands Mechanical properties Low temperature chemistry Gravitational radiation detector Lait Chemical kinetics Protein Surface tension Gravitational waves Liquid crystals Atomic and molecular collisions Digestion Density functional calculations CRESU Granular materials Confinement Glass Quantum dynamics Rubber Stars oscillations

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