48 research outputs found
Friction and wear behavior of glasses and ceramics
Adhesion, friction, and wear behavior of glasses and ionic solids are reviewed. These materials are shown to behave in a manner similar to other solids with respect to adhesion. Their friction characteristics are shown to be sensitive to environmental constituents and surface films. This sensitivity can be related to a reduction in adhesive bonding and the changes in surficial mechanical behavior associated with Rehbinder and Joffe effects. Both friction and wear properties of ionic crystalline solids are highly anisotropic. With metals in contact with ionic solids the fracture strength of the ionic solid and the shear strength in the metal and those properties that determine these will dictate which of the materials undergoes adhesive wear. The chemical activity of the metal plays an important role in the nature and strength of the adhesive interfacial bond that develops between the metal and a glass or ionic solid
Cosmological Birefringence: an Astrophysical test of Fundamental Physics
We review the methods used to test for the existence of cosmological
birefringence, i.e. a rotation of the plane of linear polarization for
electromagnetic radiation traveling over cosmological distances, which might
arise in a number of important contexts involving the violation of fundamental
physical principles. The main methods use: (1) the radio polarization of radio
galaxies and quasars, (2) the ultraviolet polarization of radio galaxies, and
(3) the cosmic microwave background polarization. We discuss the main results
obtained so far, the advantages and disadvantages of each method, and future
prospects.Comment: To appear in the Proceedings of the JENAM 2010 Symposium "From
Varying Couplings to Fundamental Physics", held in Lisbon, 6-10 Sept. 201
An 84 microGauss Magnetic Field in a Galaxy at Redshift z=0.692
The magnetic field pervading our Galaxy is a crucial constituent of the
interstellar medium: it mediates the dynamics of interstellar clouds, the
energy density of cosmic rays, and the formation of stars. The field associated
with ionized interstellar gas has been determined through observations of
pulsars in our Galaxy. Radio-frequency measurements of pulse dispersion and the
rotation of the plane of linear polarization, i.e., Faraday rotation, yield an
average value B ~ 3 microGauss. The possible detection of Faraday rotation of
linearly polarized photons emitted by high-redshift quasars suggests similar
magnetic fields are present in foreground galaxies with redshifts z > 1. As
Faraday rotation alone, however, determines neither the magnitude nor the
redshift of the magnetic field, the strength of galactic magnetic fields at
redshifts z > 0 remains uncertain. Here we report a measurement of a magnetic
field of B ~ 84 microGauss in a galaxy at z =0.692, using the same
Zeeman-splitting technique that revealed an average value of B = 6 microGauss
in the neutral interstellar gas of our Galaxy. This is unexpected, as the
leading theory of magnetic field generation, the mean-field dynamo model,
predicts large-scale magnetic fields to be weaker in the past rather than
stronger
Stochastic upscaling of hydrodynamic dispersion and retardation factor in a physically and chemically heterogeneous tropical soil
[EN] Stochastic upscaling of flow and reactive solute transport in a tropical soil is performed using real data collected in the laboratory. Upscaling of hydraulic conductivity, longitudinal hydrodynamic dispersion, and retardation factor were done using three different approaches of varying complexity. How uncertainty propagates after upscaling was also studied. The results show that upscaling must be taken into account if a good reproduction of the flow and transport behavior of a given soil is to be attained when modeled at larger than laboratory scales. The results also show that arrival time uncertainty was well reproduced after solute transport upscaling. This work represents a first demonstration of flow and reactive transport upscaling in a soil based on laboratory data. It also shows how simple upscaling methods can be incorporated into daily modeling practice using commercial flow and transport codes.The authors thank the financial support by the Brazilian National Council for Scientific and Technological Development (CNPq) (Project 401441/2014-8). The doctoral fellowship award to the first author by the Coordination of Improvement of Higher Level Personnel (CAPES) is acknowledged. The first author also thanks the international mobility grant awarded by CNPq, through the Sciences Without Borders program (Grant Number: 200597/2015-9). The international mobility grant awarded by Santander Mobility in cooperation with the University of Sao Paulo is also acknowledged. DHI-WASI is gratefully thanked for providing a FEFLOW license.Almeida De-Godoy, V.; Zuquette, L.; Gómez-Hernández, JJ. (2019). Stochastic upscaling of hydrodynamic dispersion and retardation factor in a physically and chemically heterogeneous tropical soil. 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