论文标题
稀疏波的非线性稳定性,用于粘性辐射和反应性气体,并具有较大的初始扰动
Nonlinear stability of rarefaction waves for a viscous radiative and reactive gas with large initial perturbation
论文作者
论文摘要
We investigate the time-asymptotically nonlinear stability of rarefaction waves to the Cauchy problem of an one-dimensional compressible Navier-Stokes type system for a viscous, compressible, radiative and reactive gas, where the constitutive relations for the pressure $p$, the specific internal energy $e$, the specific volume $v$, the absolute temperature $θ$, and the specific entropy $s$ are given by $p=Rθ/v +aθ^4/3 $,$ e =c_vθ+avθ^4 $,$ s = c_v \lnθ+4avθ^3/3+r \ ln v $,$ r> 0 $,$ c_ {v}> 0 $,$ a> 0 $是完美的气体常数,特定的热量和辐射常量和辐射常数,分别为辐射常数。 对于这种特定的气体运动,一个令人惊讶的事实是,概括地说,压力$ \ widetilde {p}(v,s)$不是特定卷$ v $和特定熵$ s $的凸功能。即便如此,我们在本文中表明,如果辐射常数$ a $和稀有波的强度足够小,那么对于大初始扰动而言,稀疏波是稳定的。我们分析的关键点是在特定体积和绝对温度上推断出正的下限和上限,相对于空间和时间变量是均匀的,但与辐射常数$ a $无关。
We investigate the time-asymptotically nonlinear stability of rarefaction waves to the Cauchy problem of an one-dimensional compressible Navier-Stokes type system for a viscous, compressible, radiative and reactive gas, where the constitutive relations for the pressure $p$, the specific internal energy $e$, the specific volume $v$, the absolute temperature $θ$, and the specific entropy $s$ are given by $p=Rθ/v +aθ^4/3$, $e=C_vθ+avθ^4$, and $s=C_v\ln θ+ 4avθ^3/3+R\ln v$ with $R>0$, $C_{v}>0$, and $a>0$ being the perfect gas constant, the specific heat and the radiation constant, respectively. For such a specific gas motion, a somewhat surprising fact is that, general speaking, the pressure $\widetilde{p}(v,s)$ is not a convex function of the specific volume $v$ and the specific entropy $s$. Even so, we show in this paper that the rarefaction waves are time-asymptotically stable for large initial perturbation provided that the radiation constant $a$ and the strength of the rarefaction waves are sufficiently small. The key point in our analysis is to deduce the positive lower and upper bounds on the specific volume and the absolute temperature, which are uniform with respect to the space and the time variables, but are independent of the radiation constant $a$.