scholarly journals Asymptotic stability of exogenous chemotaxis systems with physical boundary conditions

2021 ◽  
pp. 1
Author(s):  
Guangyi Hong ◽  
Zhi-an Wang
2015 ◽  
Vol 9 (2) ◽  
pp. 170-175 ◽  
Author(s):  
Otto Jusko ◽  
◽  
Michael Neugebauer ◽  
Helge Reimann ◽  
Ralf Bernhardt ◽  
...  

Form standards with different profile geometries were measured using 3- and 4-axis scanning on a 3D CMM prototype with a precision rotary table. Physical boundary conditions, including probing force, probe diameter, probe geometry, probe material, and scanning speed, were varied, and then the results were analyzed. Some results were found to be equivalent to those obtained using form measuring machines. Limitations of the current implementation of this technique are discussed.


Geophysics ◽  
2012 ◽  
Vol 77 (1) ◽  
pp. T11-T27 ◽  
Author(s):  
Kaushik Maji ◽  
Fuchun Gao ◽  
Sameera K. Abeykoon ◽  
Donald J. Kouri

We have developed a method of solving the Helmholtz equation based on a new way to generalize the “one-way” wave equation, impose correct boundary conditions, and eliminate exponentially growing evanescent waves. The full two-way nature of the Helmholtz equation is included, but the equation is converted into a pseudo one-way form in the framework of a generalized phase-shift structure consisting of two coupled first-order partial differential equations for wave propagation with depth. A new algorithm, based on the particular structure of the coupling between [Formula: see text] and [Formula: see text], is introduced to treat this problem by an explicit approach. More precisely, in a depth-marching strategy, the wave operator is decomposed into the sum of two matrices: The first one is a propagator in a reference velocity medium, whereas the second one is a perturbation term which takes into account the vertical and lateral variation of the velocity. The initial conditions are generated by solving the Lippmann-Schwinger integral equation formally, in a noniterative fashion. The approach corresponds essentially to “factoring out” the physical boundary conditions, thereby converting the inhomogeneous Lippmann-Schwinger integral equation of the second kind into a Volterra integral equation of the second kind. This procedure supplies artificial boundary conditions, along with a rigorous method for converting these solutions to those satisfying the correct, Lippmann-Scwinger (physical) boundary conditions. To make the solution numerically stable, the Feshbach projection operator technique is used to remove only the nonphysical exponentially growing evanescent waves, while retaining the exponentially decaying evanescent waves, along with all propagating waves. Suitable absorbing boundary conditions are implemented to deal with reflection or wraparound from boundaries. At the end, the Lippmann-Schwinger solutions are superposed to produce time snapshots of the propagating wave.


Author(s):  
Jose M. Chaquet ◽  
Roque Corral

Abstract Heat transfer problem is one of the main challenges in the design process of turbomachinery components for aeronautic applications. Good prediction capabilities are required to estimate metal temperatures, specially in those regions where the working fluid reaches temperatures near to the material melting point. In this context, it is common to perform multi-physics simulations involving different solvers. Special care must be taken at the interfaces between the several domains to avoid non-physical solutions. Concretely speaking, the coupling process between a thermal code (discretized heat diffusion equation solver) and a fluid network (low fidelity models representing air flows) is studied. Several non-physical boundary conditions examples are provided. The models are solved using an in-house thermal code called Saturn. The effects both in the results and in the convergence process are described. Non-physical boundary conditions provoke instabilities in the flow direction at some parts of the fluid network. A method to analyze the compatibility and convergence of the coupled problem is described and used in the examples. Also, some heuristics to achieve converge in the ill-posed models are commented.


2016 ◽  
Vol 96 ◽  
pp. 190-202 ◽  
Author(s):  
Zheshao Chang ◽  
Xin Li ◽  
Chao Xu ◽  
Chun Chang ◽  
Zhifeng Wang ◽  
...  

2011 ◽  
Vol 2011 ◽  
pp. 1-8 ◽  
Author(s):  
Andrea Lapi ◽  
Alfonso Cavaliere

We investigate the dynamical basis of the classic empirical models (specifically, Sérsic-Einasto and generalized NFW) that are widely used to describe the distributions of collisionless matter in galaxies. We submit that such a basis is provided by ourα-profiles, shown to constitute solutions of the Jeans dynamical equilibrium with physical boundary conditions. We show how to set the parameters of the empirical in terms of the dynamical models; we find the empirical models, and specifically Sérsic-Einasto, to constitute a simple and close approximation to the dynamical models. Finally, we discuss how these provide a useful baseline for assessing the impact of the small-scale dynamics that may modulate the density slope in the central galaxy regions.


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