What is the effect on the second fundametal form of asurface of applying an isometry of $\Bbb R^3$ ? Or a dilation?
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This answer is not understandable for me in general. Please is someone explains it, I'll be happy. Thank you.
What is the effect on the second fundametal form of asurface of applying an isometry of $\Bbb R^3$ ? Or a dilation?
I posted its answer.

This answer is not understandable for me in general. Please is someone explains it, I'll be happy. Thank you.
On
For the second part of the question, to understand the effect on the second fundamental form of applying a dilation, lets consider a hypersurface in $\mathbb{R}^n$ with the metric induced by the usual inner product $\langle \cdot , \cdot \rangle$.
Then we have a parameterisation $F$ of a surface in $\mathbb{R}^n$, and the dilation $\tilde{F} = \psi F$, where $\psi$ is a constant (independent of the spacial coordinates). We then notice that
\begin{equation} \frac{\partial \tilde{F}}{\partial x_i} = \psi\frac{\partial F}{\partial x_i}, \quad \mbox{and}\quad \frac{\partial^2 \tilde{F}}{\partial x_j\partial x_i} = \psi\frac{\partial^2 F}{\partial x_j\partial x_i}, \end{equation}
from which follows \begin{equation} \tilde{g}_{ij} = \left\langle \frac{\partial \tilde{F}}{\partial x_i} , \frac{\partial \tilde{F}}{\partial x_j} \right\rangle = \left\langle \psi \frac{\partial F}{\partial x_i} ,\psi \frac{\partial F}{\partial x_j} \right\rangle = \psi^2 g_{ij}. \end{equation}
Since the unit normal vector $\nu$ of the hypersurface $F$ is also a normal unit vector for the hypersurface $\tilde{F}$, we compute the second fundamental form as \begin{equation} \tilde{h}_{ij} = \left\langle \frac{\partial^2 \tilde{F}}{\partial x_j\partial x_i} , \nu\right\rangle = \psi \left\langle \frac{\partial^2 F}{\partial x_j\partial x_i} , \nu\right\rangle = \psi h_{ij}. \end{equation}
Let $r=r(u,v)$ be a parametrization of a given surface and let $n=n(u,v)$ denote the normal vector. We use the notation
$$II:=Ldu^2 + 2Mdudv + Ndv^2$$ where $L = r_{uu}\cdot n$; $M = r_{uv}\cdot n$; $N = r_{vv}\cdot n$ for the second fundamental form.
In this answer I proved that the first fundamental form is invariant under $r\mapsto r':= Or+b$, where $O$ is a $3\times 3$ orthogonal matrix and $b$ real. Note that $r'=r'(u,v)$. and
$$r'_j=\sum_{k=1}^3 O_{jk}r_k+b_j, $$
for all $j=1,2,3$.
Then $r'_u:=\frac{\partial r'}{\partial u}=O\frac{\partial r}{\partial u}$ and $r'_v:=\frac{\partial r'}{\partial v}=O\frac{\partial r}{\partial u}$, as $O$ does not depend on $(u,v)$; similarly $r'_{uu}=r_{uu}$ and $r'_{vv}=r_{vv}$. The normal vector w.r.t. $r'$ is then
$$n'=r'_u \times r'_v=\pm n,$$
as proved in the original reference (prop. A.1.6). It follows that
$$L'= r'_{uu}\cdot n'=\pm r_{uu}\cdot n=\pm L,$$ $$M' = r'_{uv}\cdot n'= \pm r_{uv}\cdot n=\pm M,$$
and similarly for the remaining coefficient of the second fundamental form, i.e. $N$.
The case of dilations is treated analogously. Please check this answer again for the explicit computations.