3.4.1: Ejemplos
- Page ID
- 117962
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)Ejemplo 3.4.1.1: Ecuaciones de Navier-Stokes
El sistema Navier-Stokes para un líquido viscoso incompresible es
\ begin {eqnarray*}
v_t+ (v\ cdot\ nabla_x) v&=&-\ frac {1} {\ rho}\ nabla_x p+\ gamma\ triangle_x v\
\ text {div} _x\ v&=&0,
\ end {eqnarray*}
donde
\(\rho\) es la densidad (constante y positiva) del líquido,
\(\gamma\) es la viscosidad (constante y positiva) del líquido, vector de
\(v=v(x,t)\) velocidad de las partículas líquidas,\(x\in\mathbb{R}^3\) o en\(\mathbb{R}^2\),
\(p=p(x,t)\) presión.
El problema es encontrar soluciones\(v,\ p\) al sistema anterior.
Ejemplo 3.4. 2.1: Elasticidad lineal
Considera el sistema
\ begin {ecuación}
\ label {elast}
\ rho\ frac {\ parcial^2u} {\ parcial t^2} =\ mu\ triangle_x u+ (\ lambda+\ mu)\ nabla_x (\ text {div} _x\ u) +f.
\ end {ecuación}
Aquí está, en el caso de un cuerpo elástico en\(\mathbb{R}^3\),
\(u(x,t)=(u_1(x,t),u_2(x,t),u_3(x,t))\)vector de desplazamiento,
\(f(x,t)\) densidad de fuerza externa, densidad
\(\rho\) (constante), constantes de Lamé
\(\lambda,\ \mu\) (positivas).
La ecuación característica es\(\det C=0\) donde las entradas de la matriz\(C\) están dadas por
$$
c_ {ij} =(\ lambda+\ mu)\ chi_ {x_i}\ chi_ {x_j} +\ delta_ {ij}\ left (\ mu|\ nabla_x\ chi|^2-\ rho\ chi_t^2\ right).
$$
La ecuación característica es
$$
\ left ((\ lambda+2\ mu) |\ nabla_x\ chi|^2-\ rho\ chi_t^2\ right)\ left (\ mu|\ nabla_x\ chi|^2-\ rho\ chi_t^2\ right) ^2=0.
$$ De
ello se deduce que son posibles dos velocidades diferentes\(P\) de superficies características\(\mathcal{S}(t)\)
\(\chi(x,t)=const.\), definidas por, a saber,
$$
P_1=\ sqrt {\ frac {\ lambda+2\ mu} {\ rho}},\\\ mbox {y}\\ P_2=\ sqrt {\ frac {\ mu} {\ rho}}.
$$ Eso
lo recordamos\(P=-\chi_t/|\nabla_x\chi|\).