scholarly journals A note on the inviscid limit of the Benjamin-Ono-Burgers equation in the energy space

2013 ◽  
Vol 141 (8) ◽  
pp. 2793-2798 ◽  
Author(s):  
Luc Molinet
2000 ◽  
Vol 417 ◽  
pp. 323-349 ◽  
Author(s):  
L. FRACHEBOURG ◽  
Ph. A. MARTIN

The one-dimensional Burgers equation in the inviscid limit with white noise initial condition is revisited. The one- and two-point distributions of the Burgers field as well as the related distributions of shocks are obtained in closed analytical forms. In particular, the large distance behaviour of spatial correlations of the field is determined. Since higher-order distributions factorize in terms of the one- and two- point functions, our analysis provides an explicit and complete statistical description of this problem.


2011 ◽  
Vol 228 (2) ◽  
pp. 647-677 ◽  
Author(s):  
Zihua Guo ◽  
Lizhong Peng ◽  
Baoxiang Wang ◽  
Yuzhao Wang

Author(s):  
Shenglan Yuan ◽  
Dirk Blömker ◽  
Jinqiao Duan

This work is devoted to investigating stochastic turbulence for the fluid flow in one-dimensional viscous Burgers equation perturbed by Lévy space-time white noise with the periodic boundary condition. We rigorously discuss the regularity of solutions and their statistical quantities in this stochastic dynamical system. The quantities include moment estimate, structure function and energy spectrum of the turbulent velocity field. Furthermore, we provide qualitative and quantitative properties of the stochastic Burgers equation when the kinematic viscosity [Formula: see text] tends towards zero. The inviscid limit describes the strong stochastic turbulence.


2020 ◽  
Vol 18 (6) ◽  
pp. 1477-1491
Author(s):  
Sona Akopian ◽  
Moon-Jin Kang ◽  
Alexis Vasseur

2010 ◽  
Vol 83 (2) ◽  
pp. 301-320
Author(s):  
HUA ZHANG ◽  
YUQIN KE

AbstractWe prove that the modified Benjamin–Ono–Burgers equation is globally well-posed in Hs for s>0. Moreover, we show that the solution of the modified Benjamin–Ono–Burgers equation converges to that of the modified Benjamin–Ono equation in the natural space C([0,T];Hs), s≥1/2, as the dissipative coefficient ϵ goes to zero, provided that the L2 norm of the initial data is sufficiently small.


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