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En deuxième partie, ce cours présente l'application de la méthode McKenzie aux articulations du membre supérieur (épaule, coude, poignet, main) ainsi qu'au management des tendinopathies du …
arxiv.org arXiv
arxiv.org › abs › 1106.4567v1
The frequency distributions of sizes and fluxes of supra-arcade downflows (SADs) provide information about the process of their creation. For example, a fractal creation process may be expected to yie...
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L'Institut McKenzie International a développé un examen de compétence il y a quelques années. En France, il est proposé depuis 2010. L’examen de compétence McKenzie est axé sur la clinique. I...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0409223v2
We present time-domain Monte Carlo simulations of radio emission from cosmic ray air showers in the scheme of coherent geosynchrotron radiation. Our model takes into account the important air shower c...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0305141v1
We discuss the various post-main sequence phases of massive stars, focusing on Wolf-Rayet stars, Luminous Blue Variables, plus connections with other early-type and late-type supergiants. End states f...
arxiv.org arXiv
arxiv.org › abs › 2303.05913v1
Mack's distribution-free chain ladder reserving model belongs to the most popular approaches in non-life insurance mathematics. Proposed to determine the first two moments of the reserve, it does not ...
arxiv.org arXiv
arxiv.org › abs › 1211.6334v1
A coupled cell network describes interacting (coupled) individual systems (cells). As in networks from real applications, coupled cell networks can represent inhomogeneous networks where different typ...
arxiv.org arXiv
arxiv.org › abs › 2503.13774v1
Elastoviscoplastic (EVP) fluid flows are driven by a non-trivial interplay between the elastic, viscous, and plastic properties, which under certain conditions can transition the otherwise laminar flo...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0410327v1
Using Monte Carlo codes, we follow the collisional evolution of clusters in a variety of scenarios. We consider the conditions under which a cluster of main sequence stars may undergo rapid core colla...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0305140v1
We discuss the determination of fundamental parameters of `normal' hot, massive OB-type stars, namely temperatures, luminosities, masses, gravities and surface abundances. We also present methods used...
arxiv.org arXiv
arxiv.org › abs › 2203.12962v2
To simulate elastic turbulence, where viscoelasticity dominates, numerical solvers introduce an artificial stress diffusivity term to handle the steep polymer stress gradients that ensue. This has rec...
arxiv.org arXiv
arxiv.org › abs › 1012.1373v1
Massive stars are powerful sources of radiation, stellar winds, and supernova explosions. The radiative and mechanical energies injected by massive stars into the interstellar medium (ISM) profoundly ...