Finite dimensional Feynman integrals In a sense this is a follow up question to The mathematical theory of Feynman integrals although by all rights it should precede that question.
Let $S$ be a polynomial with real coefficients in $n$ variables. Is there a criterion which would say when the integral $$\int_{\mathbf{R}^n}e^{iS(x)}dx$$ converges? Here $dx$ is the Lebesgue measure on $\mathbf{R}^n$ and the integral is understood as the limit of the integrals over the balls of radius $r$ centered at the origin (with respect to the standard metric) as $r\to\infty$.
Some obvious remarks:


*

*If $\deg S=2$, the integral converges if and only if the quadratic part of $S$ is nondegenerate.

*If $n=1$, the integral converges if and only if $\deg S>1$.

*The answer to the above question is probably classical (but it is unknown to me).
upd: Conjecture (inspired by Jeff's answer below). A sufficient condition for the integral to converge is as follows: let $S_i$ be the degree $i$ part of $S$ and let $V_i,i=1,\ldots,d=\deg S$ be the subvariety of the real projective space $\mathbf{P}^{n-1}(\mathbf{R})$ given by $S_i=0$. The integral converges if $V_2\cap\cdots\cap V_d={\emptyset}$. Here is how one can try to prove this: the above condition is equivalent to saying that the integral along any line converges, so one can try to first integrate along all half-lines emanating from the origin, get a continuous function on the sphere (hopefully) and then integrate it along the sphere. As remark 1. above shows, this condition may be sufficient but it is not necessary.
 A: Let $d=\deg S$. If $d\ge 2$ and $S$ is non-degenerate near infinity, in the sense that $|\nabla S(x)|^2 \ge c|x|^{2d-2}$ for $|x|\ge R$ for some positive $R$ and $c$ then the integral converges in a sense close to what you propose.  Namely, 
$$\lim_{r\rightarrow \infty} \int_{\mathbb R^n} \phi(|x|/r) e^{iS(x)} dx$$ exists where $\phi$ is any sufficiently smooth function with $\phi(t)\equiv 1$ for $0\le t\le 1$ and $\phi (t)\equiv 0$ for $t\ge 2$. 
To prove this use integration by parts.  Fix $r < r'$ and let
$$I_{r,r'} = \int_{\mathbb R^n} \phi_{r,r'}(x) e^{i S(x)}dx,$$where $\phi_{r,r'}(x)=\phi(|x|/r)-\phi(|x|/r')$.  Assume $r >R$. Multiply and divide by $|\nabla S(x)|^2$, noting that 
$$|\nabla S(x)|^2e^{i S(x)}= -i\nabla S(x)\cdot \nabla e^{i S(x)}.$$
So we have, after IBP,
$$I_{r,r'} = -i \int_{\mathbb R^n} \left [ \nabla \cdot \left ( \frac{\phi_{r,r'}(x)}{|\nabla S(x)|^2} \nabla S(x) \right ) \right ] e^{i S(x)} d x.$$
The integrand is supported in the region $r \le |x| \le 2 r'$, and you can check that it is bounded in magnitude by some constant times $|x|^{1-d}$.  (It is useful to note that an $m$-th derivative of $S$ is bounded from above by $|x|^{d-m}$ since it is a polynomial of degree $d-2$.)  If $d$ is large enough this may be enough to control the integral.  If not repeat the procedure as many times as necessary to produce a factor that is integrable and you can use to show that $I_{r,r'}$ is small for $r,r'$ sufficiently large.  Basically, each time you integrate by parts after multiplying and dividing by $|\nabla S(x)|^2$ you produce a an extra factor of size $|x|^{1-d}$.  
All of the above can be extended to integrals with $S$ not necessarily a polynomial, but sufficiently smooth in a neighborhood of infinity and with derivatives that satisfy suitable estimates.  The real difficulty with such integrals is not proving that they exist, but estimating their size.  Here stationary phase is useful, when applicable, but I don't know of much else.
A: That integral doesn't converge absolutely, so you'll have to choose some way of making sense of the sum.  The one you've chosen above -- taking a limit of integrals on compact sets -- is not so easy to control.  What physicists typically do is "analytic continuation":  They find a family $[0,\infty) \ni t \mapsto S_t$ of actions for which (a) $S_0 = S$, and (b) $Z_t = \int e^{iS_t(x)}dx$ is absolutely convergent for $t \neq 0$.  ($t$ is a real parameter.)  Then they define the integral of $e^{iS}$ as the boundary value $\lim_{t \to 0} Z_t$.
For some reason, the physicists speak about this process as if they were analytically continuing from $Z_0$ rather than to $Z_0$.
A: I would just like to add a note about this notion of "analytic continuation" that is often employed to make sense of such integrals. There are two dual ways of thinking about it,


*

*Often a "convergence factor" of $i\epsilon$ is added to the action and then the "path integration" done. At the end the $\epsilon \rightarrow 0$ limit is taken. Now there are lots of issues about why or when this limit will exist. I guess most often this limit does not exist and various methods are used to make sense of it like "Borel Resummation". This basically does kind of an asymptotic approximation but at low values of the "perturbation parameter". The series expansions of these integrals are generically divergent but a finite number of the terms sum to good approximations for low values of the perturbation parameter.

*The other way to look at analytic continuation is what is also called the "Feynman Prescription" by way of which one makes a complex analytic continuation of a real function by choosing a contour on which things are well-behaved. A part of this contour will include the region on the real axis where the actual interest is. Most often these functions have singularities on the real line and one has to infinitesimally deform the contour around them and take limits using what is called the Sokhotsky-Plemlj equation.
I haven't seen a rigorous proof of equivalence between these two points of view but on a case by case basis they work out equivalently. 
The simplest example where things work out easiest with no glitches is when the integration variables are on finite-dimensional vector spaces and the action is quadratic with no zero eigen values. One basically gets a determinant of the quadratic form. Now this is extrapolated to give "functional determinants" (determinants of differential operators) when the integration variables are Grassmann valued functions. Here open up a new possibility of trouble, i.e there being 0 modes. Some classical theorems assure that on compact manifolds this will not happen but Physics is more often than not done on non-compact manifolds. This invites the whole theory of "regularization". There is yet another beast that can make things go wild, what in physicists' parlance is called "short distance singularity". I would love to know what is the mathematical way of seeing their source and whether they are somehow related to there being 0 modes on non-compact manifolds. I guess these are related. 
