29 research outputs found

    Dynamics of axial separation in long rotating drums

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    We propose a continuum description for the axial separation of granular materials in a long rotating drum. The model, operating with two local variables, concentration difference and the dynamic angle of repose, describes both initial transient traveling wave dynamics and long-term segregation of the binary mixture. Segregation proceeds through ultra-slow logarithmic coarsening.Comment: 4 pages, 3 Postscript figures; submitted to PR

    Patterns and Collective Behavior in Granular Media: Theoretical Concepts

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    Granular materials are ubiquitous in our daily lives. While they have been a subject of intensive engineering research for centuries, in the last decade granular matter attracted significant attention of physicists. Yet despite a major efforts by many groups, the theoretical description of granular systems remains largely a plethora of different, often contradicting concepts and approaches. Authors give an overview of various theoretical models emerged in the physics of granular matter, with the focus on the onset of collective behavior and pattern formation. Their aim is two-fold: to identify general principles common for granular systems and other complex non-equilibrium systems, and to elucidate important distinctions between collective behavior in granular and continuum pattern-forming systems.Comment: Submitted to Reviews of Modern Physics. Full text with figures (2Mb pdf) avaliable at http://mti.msd.anl.gov/AransonTsimringReview/aranson_tsimring.pdf Community responce is appreciated. Comments/suggestions send to [email protected]

    The ubiquitous gp63-like metalloprotease from lower trypanosomatids: in the search for a function

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    Navigation Overview for the Mars Atmosphere and Volatile Evolution Mission

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    Study of habitability from Mars-NEXT

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    The question whether life exists or could have existed on other planets than Earth is not just limited to the search for life but it also requires an understanding of the habitable planetary environments. In its simplest form, habitability requires the stability of liquid water on the surface and/or subsurface of a planet. The factors that determine the stability of water and thus the habitability of a planet are multifaceted and include the internal dynamics, the presence or absence of a magnetosphere, the characteristics and evolution of a planet’s atmosphere, and the presence of energy sources. Those processes have a complex interplay and need to be studied in an interdisciplinary and comprehensive way. The future network-science Mars-NEXT mission addresses several of these objectives and will help to decipher how the key processes might have influenced the habitability on Mars and thus also on other terrestrial planets
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