Large Scale Behavior of Generalized Stochastic Magnetohydrodynamic Turbulence with Mirror Symmetry Breaking

Author(s):  
Michal Hnatič ◽  
Georgii Kalagov ◽  
Tomáš Lučivjanský ◽  
Peter Zalom
2021 ◽  
Author(s):  
Ohjin Kwon ◽  
Xiaoqian Cai ◽  
Azhar Saeed ◽  
Feng Liu ◽  
Silvio Poppe ◽  
...  

Achiral multi-chain (polycatenar) compounds based on the 2,7-diphenyl substituted [1]benzothieno[3,2-b]benzothiophene (BTBT) unit and a 2,6-dibromo-3,4,5-trialkoxybenzoate end group lead to materials forming bicontinuous cubic liquid crystaline phases with helical network structures...


2021 ◽  
Author(s):  
Iris K. Schneider ◽  
Angela Rachael Dorrough ◽  
Celine Frank

The COVID-19 pandemic poses one of the largest behavioral change challenges in the last decades. Because currently, there is no widely available pharmaceutical treatment available to contain the spread of infection, governments worldwide rely – at least to some extent – on behavioral recommendations aimed at reducing spread. The success of this strategy is dependent on the number of people that follow the recommendations. Most recommendations need people to change their behavior or adopt a new behavior. We propose that such behavioral change, with direct costs and delayed benefits, is a source of conflict and mixed feelings. This ambivalence negatively affects adherence to such recommendations. We present three studies that support our hypotheses: the more ambivalent people are about the recommendations, the less they follow them. We also examined the effect of the mixed emotions of hope and worry on adherence and find that it positively relates to adherence. Our findings replicated both in a U.S. sample as well as a representative German sample. Our work is the first to investigate the role of ambivalence in large-scale behavior change and highlight the importance of understanding the conflict that comes with changing behavior. We discuss implications for policy and communication.


2021 ◽  
Vol 2021 ◽  
pp. 1-10
Author(s):  
Zhenyu Wang ◽  
Junsheng Yang ◽  
Xinghua Wang

Generally, the surrounding rock at the entrance of a mountain tunnel is loose, and the entrance has more slopes due to topography, which causes the tunnel entrance section to be easily destroyed under an earthquake. Based on the established slope model with a single free surface, this paper adopted the elastic wave theory to derive the analytical solution of the strain at the entrance of the mountain tunnel when the SH wave is incident perpendicularly to the bottom of the tunnel; besides, the factors affecting strain were also analyzed. The tangential strain curve at each point of the entrance section takes the centre of the elliptical tunnel as the centre of symmetry, forming symmetry between the left and right sides and mirror symmetry between the top and bottom sides. Then, large-scale shaking table model experiments were conducted to model the actual working conditions, and the correctness of the analytical solution was verified. The research can provide a theoretical reference for the seismic design of the entrance section of the high-speed railway tunnel and greatly improve the understanding of its seismic response.


1997 ◽  
Vol 163 ◽  
pp. 190-200
Author(s):  
Christopher A. Tout

AbstractWe review those processes associated with accretion discs that are probably influenced by magnetic fields, specifically, accretiondisc viscosity, energy dissipation and jet formation. We consider how magnetic instabilities in the disc can lead to a self-sustaining dynamical dynamo and how this is manifested as magnetohydrodynamic turbulence in numerical simulations. We show that currently these models do not fit with observational constraints imposed by dwarf-nova outbursts. We also show that the drop in ionisation fraction does not lead to the apparently necessary drop in viscosity in quiescent cataclysmic variable discs. Large-scale magnetic fields are required to launch and collimate jets form discs. We describe an inverse cascade process that can construct sufficient large-scale field from small-scale field generated by a dynamo.


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