Evaluate $\int_{M}(F\cdot N)\,dS$ where $F=(e^{\cos z},x^2,z)$ and $M=\{(x,y,z):z=1-(x^2+y^2),x^2+y^2\leq 1\}$
I try to use Stokes' theorem:
We will evaluate it on the curve $(\cos\theta,\sin\theta,0)$.
Therefore $$\int_0^{2\pi}(e,\cos^2\theta,0)\cdot (-\sin\theta,\cos\theta,0)d\theta =\int_0^{2\pi}-e\sin\theta+\cos^3\theta d\theta=0$$
Is it correct?
I was waiting for Matthew's solution, but since he hasn't posted, here's a quick answer for you.
You can parametrize the surface and compute the surface integral directly. Polar coordinates is the easiest way to go. Let $\vec x(r,\theta) = (r\cos\theta,r\sin\theta,1-r^2)$, $0\le r\le 1$, $0\le\theta\le 2\pi$. Then \begin{align*} \int_S F\cdot N\,dS &= \int_0^{2\pi}\int_0^1 (e^{1-r^2},r^2\cos^2\theta,1-r^2)\cdot\left(\frac{\partial\vec x}{\partial r}\times\frac{\partial\vec x}{\partial\theta}\right)dr\,d\theta\\&=\int_0^{2\pi}\int_0^1 (e^{1-r^2},r^2\cos^2\theta,1-r^2)\cdot r(2r\cos\theta,2r\sin\theta,1)\,dr\,d\theta \\ &= \int_0^{2\pi}\int_0^1 r\big(e^{1-r^2}2r\cos\theta+ 2r^3\cos^2\theta\sin\theta+1-r^2\big)dr\,d\theta \\ &=\pi/2. \end{align*} (Note it's easier to actually do the $\theta$ integral first, as the first two terms integrate to $0$ by symmetry.) I've assumed that the surface $S$ is oriented with $N$ pointing upward, but you didn't state so explicitly in your question.
Much easier is to apply the Divergence Theorem by closing up the surface with the disk $D$ on the bottom. Now, since $N$ points upward on the paraboloid, it must point downward on $D$. I will emphasize this by writing $D^-$ to denote the downward orientation. Then $$\int_S F\cdot N\,dS + \int_{D^-} F\cdot N\,dS = \int_V \text{div}\,F\,dV = \int_V 1\,dV.$$ This means that $$\int_S F\cdot N\,dS = \int_V 1\,dV + \int_{D^+} F\cdot N\,dS.$$ This makes sense. What enters the bottom disk plus the net sources inside $V$ tell you what leaves the paraboloid. In this case, $F\cdot N = z = 0$ on $D$, so we just get $$\int_S F\cdot N\,dS = \int_V 1\,dV = \int_0^{2\pi}\int_0^1\int_0^{1-r^2}r\,dz\,dr\,d\theta = \frac{\pi}2;$$ indeed, this is precisely the same integral we had in the direct computation.