Lecture 23
Consider
Then locally (near \(z_0\)) \(\,f\) preserves
We say that \(f\) is conformal.
\(\Gamma_1 = f(C_1)\), \(\Gamma_2 = f(C_2)\).
Conformality \(\Rightarrow\) \(\beta = \alpha\).
If orientation (i. e., sense) is not necessarily preserved, but angle magnitude is, the map is called isogonal.
Consider \(f\) an analytic function with
\(f'(z_0) = 0\):
\(z_0\) is a critical point of
\(f\).
Angle will not be preserved. Can show: angle will be multiplied by \(m\), where \(m\) is the smallest integer such that \(\,f^{(m)}(z_0) \neq 0.\)
Conformality \(\Rightarrow\) locally one-to-one and
onto,
i. e. \(f\) has a local inverse.
This follows from MATH2400/2401: Inverse function theorem.
\(f:(x,y) \mapsto (u,v)\) sufficiently smooth is locally invertible if \[ \text{det}\left(J_f\right) = \left| \begin{array}{cc} u_x & u_y\\ v_x & v_y \end{array} \right| \neq 0. \]
In our case, \(f\) is analytic \(\Rightarrow u_x, u_y, v_x, v_y\) are continuous and
\(\text{det}\left(J_f\right) \) \( = u_x v_y - u_y v_x\) \( = u_x^2 + v_x^2\)
\( \quad \qquad = |u_x+iu_y|^2\) \( = \left|\,f'\right|^2\)
\( \quad \qquad \neq 0 \) at \(z_0\).
\(u: \Omega\subset \R^n \ra \R^n\) harmonic says:
\(\Omega \subseteq \R^2\),
\(U: \Omega \ra \R\) such that
\(\Delta U = 0\).
Laplacian or Laplace operator
\(\Delta U = U_{xx} + U_{yy}\)
In \(\R^3\) \(\Delta U = U_{xx} + U_{yy} + U_{zz}\)
In \(\R^n\) \(\Delta U = \sum_{j=1}^{n} U_{jj}\)
Models many physical situations in "steady state"
\(\Omega \subseteq \R^2\) or \(\R^3\)
\(\Lambda =\) sufficiently smooth subdomain of \(\Omega\) with external normal \(\mathbf v(\mathbf x)\) on \(\partial \Lambda\),
\(\mathbf v'\) unit exterior normal
\(U =\) density of something on equilibrium.
\(\mathbf F\): flux density of \(U\) in \(\Omega\) in equilibrium.
\[ \int_{\partial \Lambda} \mathbf F \cdot \mathbf v' dS = 0 \] \(dS=\) surface measure on \(\partial \Lambda\).
Gauss's divergence theorem:
\[ \int_{\Lambda} \text{div} \, \mathbf F \, \text{d} \mathbf x = 0 \]
\(\text{d}\mathbf x= dx \,dy\) in 2D \(\qquad\)
\(= dx \,dy\, dz\) in 3D
\(\text{d}\mathbf x= dx_1 \cdots dx_n\) in \(n\)-D
Since \(\Lambda\) is (essentially) arbitrary, there holds:
\[ \text{div} \, \mathbf F = 0 \;\text{ in } \;\Omega, \]
i. e. \(\ds \sum_{j=1}^{n} \partial_j F_j = 0\;\) in \(\;\Omega\quad (*)\)
In many physical situations, \[ \mathbf F = c \nabla U, \text{ with } c \text{ usually negative} \]
\((*) \Rightarrow\) \(c\left( \text{div}\, \nabla U\right) =0 \) i. e. \(\Delta U = 0\).