Gauss's Theorem and Divergence in R3

Prop:************ Let F=(P,Q,R):U⊆R3→R3 be C1on U, then we can define ∇⋅F as follows:

∇⋅F=∂P∂x+∂Q∂y+∂R∂z

Gauss’ Theorem

Let F=(P,Q,R):U⊆R3→R3 be C1on U, and Ω⊆U be Jordan measurable such that S=∂Ω be a piecewise surface and Ω∪S⊆U, then

∫Ω∇⋅F=∮S=∂ΩF⋅dσ

where σ is a simple parametrization of S that induce the normal vectors pointing “outward” of Ω.

General Gauss’ Theorem

Let F=(P,Q,R):U⊆R3→R3 be C1on U, and Ω⊆U be Jordan measurable such that ∂Ω=S0∪⋯∪Sk, where S0,…,Sk piecewise surfaces, and S0 being the most exterior and Ω∪S⊆U, then

∫Ω∇⋅F=∮S=∂ΩF⋅dσ=∑i=0k∮SiF⋅dσi

where σ0,…,σk is a simple parametrization of S0,…,Sk that induce the normal vectors pointing “outward”.

Divergence in R3

Def: Let F:U⊆R3→R3 be C1on U, x∈U and {Ωε}0<ε<c be a family of compact Jordan-measurable sets contained in U, such that Sε=∂Ωε is a surface, x∈intΩε, for all 0<ε<c∈R and limε→0diam(Ωε)=0 , then *divergence of F at x is defined as

divF(x):=limε→01J(Ωε)∮SεF⋅dσε

where σε is a parametrization of Sε that induce the normal vectors pointing “outward”. We know this must converge since we can use the Divergence Theorem to calculate the value and find it is independent of the choice of {Ωε}0<ε<c.

Prop: Let F=(P,Q):U⊆R2→R2 be C1on U, then we can simplify divF as follows:

divF=∇⋅F

Prop: Let F,G:U⊆R2→R2 such that divF and divG exists for every x∈U, and α,β∈R . Then div(αF+βG) exists for every x∈U, and

div(αF+βG)=αdivF+βdivG

Prop: Let F,G:U→R3 both being C1 on U, then ∇⋅(F×G) exists and

∇⋅(F×G)=(∇×F)⋅G−F⋅(∇×G)

Prop: Let ϕ:U⊆Rn→R be a scalar field and F:U→R3 both being C1 on U, then ∇⋅(ϕF) exists and

∇⋅(ϕF)=∇ϕ⋅F+ϕ∇⋅F

We can use this along with Gauss’ Theorem, and get the following

Let U be a open and connected set, let Ω⊆U be a Jordan-measurable, and ∂Ω=S be a piecewise surface, and Ω∪S⊆U, then

∫Ωϕ∇⋅F=∮S=∂ΩϕF⋅dσ−∫Ω∇ϕ⋅F

with σ be parametrization of S, that induces the normal vectors pointing upward.

This can be thought as formula of integration by parts of R3

Cor: Let F:U⊆R3→R3 be C2on U, then we get the following relation

∇⋅(∇×F)=0

Def:****** Let f:U⊆R2→R be C2on U, then we can consider the following

\nabla \cdot (\nabla f) = \nabla { #2} f=\Delta f = \frac{\partial^2 f }{\partial x^2} + \frac{\partial^2 f}{\partial y^2}+ \frac{\partial^2 f}{\partial z^2}

This is called the ************Laplacian of f

Def: Let f:U⊆R3→R be C2on U, if Δf=0, then f is called harmonic.