Tension mécanique | EPFL Graph Search

En physique, la tension mécanique d'un solide linéaire, exprimée en newtons () — ce qui correspond à des dans les unités SI — est l'effort qu'il subit quand il est soumis, à ses extrémités, à deux forces dirigées vers l'extérieur du solide. En résistance des matériaux, cet effort résulte d'une contrainte appelée traction. Lors du calcul de forces centripètes, on peut utiliser m\frac{v^2}{r} pour trouver la force de tension d'un fil, ou de quelque chose qui fait office de corde. Catégorie:Mécanique Catégorie:Résistance des matériaux

Mechanical properties of tailored nanostructured alloys produced by electrodeposition

Juri Aljoscha Wehrs

The studies presented in this thesis aim to extend the current knowledge and understanding of the mechanical behavior of nanocrystalline materials with respect to temperature- and time dependence. Free standing electrodeposited nanocrystalline nickel specimen with mean grain sizes in the order of 40nm are synthesized and investigated. A miniaturized in situ test rig is developed, capable of performing uniaxial tensile tests on dedicated miniaturized specimen. A novel displacement controlled in situ high temperature indentation system is presented, capable of performing sharp tip indentation and uniaxial micropillar compression experiments up to 600°C. Elevated temperature micropillar strain rate jump tests are performed to extract the strain rate sensitivity factor, apparent activation volume and activation energy. The results suggest grain boundary diffusion to be the rate controlling deformation mechanism. Post deformation imaging also indicates the activity of dislocation based mechansims. To compare the results to established techniques, micro specimen are tested under three different load cases: uniaxial tension, uniaxial compression and hydrostatic pressure. The results compare well to the previous, suggesting the rate controlling mechanism to be the same for all three load cases. A transient load relaxation tests is developed to assess time dependent plasticity on short and intermediate time scales. The results suggest grain boundary mediated processes to be rate controlling. To enhance the identification of specific deformation mechanisms, elevated temperature micropillar strain rate jump- and load relaxation tests are also conducted on an inert gas condensated nanocrystalline palladium-gold model alloy. Distinct features of this material are extremely high chemical purity and small, homogeneous grain sizes in the order of ~10nm. Shear transformation mediated plasticity is observed, similar to the deformation of metallic glasses. The demonstrated methods are relevant for the Swiss watch industry. A series of mechanical tests on standard watch materials are compared. An approach for the electrodeposition of a nickel-tungsten alloy for watch applications with improved thermal stability and less pronounced time dependent plastic behavior is presented.

EPFL2017

Embrittlement induced by the synergistic effects of radiation damage and helium in structural steels

Kun Wang

Ferritic/martensitic steels are candidate materials for fusion reactor structural components, liquid metal containers of spallation neutron sources, and accelerator driven systems, with good radiation resistance and thermo-mechanical properties. However, embrittlement resulting from the combined effects of radiation induced displacement damage (measured in dpa = displacement per atom) and transmutation products, especially helium gas, is one of the key issues. Four different steels were selected for mechanical and microstructural studies to understand the mechanisms of embrittlement induced by the combined effects of displacement damage and helium after irradiation in SINQ, the Swiss spallation source. The irradiations conditions were in the range: 10.7 ¿ 20.4 dpa with 850-1750 appm He at 160-300 °C. The evolution of the mechanical properties after irradiation was investigated by tensile and hardness tests. Radiation-induced defect clusters and helium bubbles were quantified by transmission electron microscopy (TEM). Emphasis was put on the deformation mechanisms under the different observed fracture mode, (ductile, quasi-cleavage and intergranular), whose occurrence depends on the irradiation conditions (dpa, He content and irradiation temperature). The tensile stress-strain curves and the scanning electron microscopy images of fracture surfaces showed distinct fracture mechanisms under different irradiation and test conditions. The tensile tests showed a yielding stress increase and loss of ductility of irradiated specimens. Hardness was measured on the specimens before tensile testing. The hardness results demonstrated an increasing trend with irradiation dose and helium content. TEM observations were done for all irradiated fractured specimens. Small defect clusters were observed in the 12.3 dpa specimen, but large defect clusters with loop-shape were very few. In the specimens of 17.2, 17.7 and 20.4 dpa, many large dislocation loops were detected besides small clusters. In addition, helium bubbles were observed in all specimens. The average size of defect clusters increased from 4.2 nm to 11.8 nm with dose increasing from 12.3 dpa to 20.4 dpa, whereas the number density did not change significantly. Meanwhile, the average size of visible helium bubbles increased from 1.03 nm to 1.93 nm. The microstructures in deformed area of irradiated specimens were observed and defect free channels with {110} and {112} slip planes were found in some specimens, indicating plastic flow localization. The average width of the channels is about 100 nm. Regarding the brittle samples, the TEM-lamella were extracted directly below intergranular fracture surfaces or cleavage surfaces by focused ion beam. Strikingly, deformation twinning was observed as the main feature in three irradiated specimens at high dose. Only twins with {112} planes were observed in all of these samples. The average thickness of twins is about 34 nm. Twins started from a fracture surface became gradually thinner with distance away from the fracture surface and stopped in the matrix finally. Features such as twin-precipitates interaction, twin-grain boundary and/or lath boundary interaction were observed. Twinning bands were seen to be arrested by grain boundaries or large precipitates, but could penetrate martensitic lath boundaries. Unlike the case of defect free channels, inside twins small defect-clusters, dislocation loops and dense small helium bubbles were observed.

EPFL2015

Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies

Richard Irving Anderson, Hsin-Yu Chen, Frédéric Courbin, Fabio Finelli, Mikhail Ivanov, Melissa Joseph, Suresh Kumar, Julien Lesgourgues, Florian Niedermann, Emre Ozulker

The standard Lambda Cold Dark Matter (Lambda CDM) cosmological model provides a good description of a wide range of astrophysical and cosmological data. However, there are a few big open questions that make the standard model look like an approximation to a more realistic scenario yet to be found. In this paper, we list a few important goals that need to be addressed in the next decade, taking into account the current discordances between the different cosmological probes, such as the disagreement in the value of the Hubble constant H-0, the sigma(8)-S-8 tension, and other less statistically significant anomalies. While these discordances can still be in part the result of systematic errors, their persistence after several years of accurate analysis strongly hints at cracks in the standard cosmological scenario and the necessity for new physics or generalisations beyond the standard model. In this paper, we focus on the 5.0 sigma tension between the Planck CMB estimate of the Hubble constant H-0 and the SH0ES collaboration measurements. After showing the H-0 evaluations made from different teams using different methods and geometric calibrations, we list a few interesting new physics models that could alleviate this tension and discuss how the next decade's experiments will be crucial. Moreover, we focus on the tension of the Planck CMB data with weak lensing measurements and redshift surveys, about the value of the matter energy density Omega(m), and the amplitude or rate of the growth of structure (sigma(8), f sigma(8)). We list a few interesting models proposed for alleviating this tension, and we discuss the importance of trying to fit a full array of data with a single model and not just one parameter at a time. Additionally, we present a wide range of other less discussed anomalies at a statistical significance level lower than the H-0-S-8 tensions which may also constitute hints towards new physics, and we discuss possible generic theoretical approaches that can collectively explain the non-standard nature of these signals. Finally, we give an overview of upgraded experiments and next-generation space missions and facilities on Earth that will be of crucial importance to address all these open questions. (C) 2022 The Author(s). Published by Elsevier B.V.

ELSEVIER2022