<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
<dc:title>Study of the linear ablation growth rate for the quasi-isobaric model of Euler equations with thermal conductivity</dc:title>
<dc:creator>Olivier Lafitte</dc:creator>
<dc:subject>34B99</dc:subject><dc:subject>76N</dc:subject><dc:subject>hydrodynamics instabilities</dc:subject><dc:subject>Evans functions</dc:subject><dc:subject>Rayleigh-Taylor</dc:subject><dc:subject>semiclassical analysis</dc:subject><dc:subject>asymptotic analysis</dc:subject><dc:subject>compressible fluids</dc:subject>
<dc:description>In this paper, we study a linear system related to the 2d system of Euler equations with thermal conduction in the quasi-isobaric approximation of Kull-Anisimov (H.J. Kull, \emph{Theory of the Rayleigh-Taylor instability}, Physical Report \textbf{206} (1991), 197--325). This model is used for the study of the ablation front instability, which appears in the problem of inertial confinement fusion. The heat flux $\vec{Q}$ is given by the Fourier law $T^{-\nu}\vec{Q}$ proportional to $\nabla T$, where $\nu &gt; 1$ is the thermal conduction index, and the external force is a gravity field $\vec{g} = -g\vec{e}_x$. This physical system contains a mixing region, in which the density of the gaz varies quickly, and one denotes by $L_0$ an associated characteristic length. The fluid velocity in the denser region is denoted by $V_a$.  The system of equations is linearized around a stationary solution, and each perturbed quantity $\tilde{u}$ is written using the normal modes method \[ \tilde{u}(x,z,t) = \text{Re}(\bar{u}(x,k,\gamma)e^{ikz + \gamma \sqrt{gk}t}) \] in order to take into account an increasing solution in time.  The resulting linear system is a non self-adjoint fifth order system. Its coefficients depend on $x$ and on physical parameters $\alpha$, $\beta$, $\alpha$ and $\beta$ being two dimensionless physical constants, given by $\alpha\beta = kL_0$ and $\alpha/\beta = gL_0/V_a^2$ (introduced in C. Cherfils-Cl\&#39;erouin, P. Lafitte, and P.A. Raviart, \emph{Asymptotic Results for the Rayleigh-Taylor Instability}, Birkhauser, Boston, 2001). We study the existence of bounded solutions of this system in the limit $\alpha \to 0$, under the condition $\beta \in [\beta_0, 1/\beta_0]$, and the assumption $\text{Re}\gamma \in [0, 1/\beta_0]$, $|\gamma| \leq 1/\beta_0$ (regime that we studied for a simpler model in ibid.) calculating the Evans function $\text{Ev}(\alpha,\beta,\gamma)$ associated with this linear system.  Using rigorous constructions of decreasing at $\pm\infty$ solutions of systems of ODE, we prove that, for any $\beta_0 &gt; 0$, there exists $\alpha_1(\beta_0)$ such that, for all $\beta \in [\beta_0, 1/\beta_0]$, $0 &lt; \alpha \leq \alpha_1$, there is no bounded solution of the linearized system such that $\text{Re}\gamma \in [0, 1/\beta_0]$, $|\gamma| \leq 1/\beta_0$.  In other terms, for any $M &gt; 0$ and $\beta_0 &gt; 0$ there exists $\alpha_1 &gt; 0$ such that, for $0 &lt; \alpha \leq \alpha_1$ and $\beta \in [\beta_0, 1/\beta_0]$, an admissible value $\gamma(\alpha,\beta)$ such that there exists a bounded solution of the linearized system satisfying $|\gamma| \leq M$ is such that $\text{Re}\gamma \notin [0,M]$.</dc:description>
<dc:publisher>Indiana University Mathematics Journal</dc:publisher>
<dc:date>2008</dc:date>
<dc:type>text</dc:type>
<dc:format>pdf</dc:format>
<dc:identifier>10.1512/iumj.2008.57.3172</dc:identifier>
<dc:source>10.1512/iumj.2008.57.3172</dc:source>
<dc:language>en</dc:language>
<dc:relation>Indiana Univ. Math. J. 57 (2008) 945 - 1018</dc:relation>
<dc:coverage>state-of-the-art mathematics</dc:coverage>
<dc:rights>http://iumj.org/access/</dc:rights>
</oai_dc:dc>