In mathematics, and in particular singularity theory, an singularity, where is an integer, describes a level of degeneracy of a function. The notation was introduced by V. I. Arnold.
Let
f:\Rn\to\R
\Omega(\Rn,\R)
\operatorname{diff}(\Rn)
\Rn\to\Rn,
\operatorname{diff}(\R)
\R\to\R.
\operatorname{diff}(\Rn) x \operatorname{diff}(\R)
\Omega(\Rn,\R)
\varphi:\Rn\to\Rn
\psi:\R\to\R
f:\Rn\to\R
(\varphi,\psi) ⋅ f:=\psi\circf\circ\varphi-1
orb(f)=\{\psi\circf\circ\varphi-1:\varphi\indiff(\Rn),\psi\indiff(\R)\} .
The members of a given orbit of this action have the following fact in common: we can find a diffeomorphic change of coordinate in and a diffeomorphic change of coordinate in such that one member of the orbit is carried to any other. A function is said to have a type -singularity if it lies in the orbit of
f(x1,\ldots,xn)=1+\varepsilon1x
2 | |
1 |
+ … +\varepsilonn-1
2 | |
x | |
n-1 |
\pm
k+1 | |
x | |
n |
\varepsiloni=\pm1
By a normal form we mean a particularly simple representative of any given orbit. The above expressions for give normal forms for the type -singularities. The type -singularities are special because they are amongst the simple singularities, this means that there are only a finite number of other orbits in a sufficiently small neighbourhood of the orbit of .
This idea extends over the complex numbers where the normal forms are much simpler; for example: there is no need to distinguish from .