Numerical modeling of differential problem
Definitions
Ω to denote a domain → subset of ℝd Ω d = 1, 2, 3. Ω is an open domain, ∞ people is exhausted, but we set Ω bounded. Ω is also connected; if you take 2 points inside the domain, you can connect them with a line inside of the domain. This is a differential problem on Ω. Normally we divide the forced domain from time variations Q = Ω x I where I = (t0, T], often t0 = ∅. True variation is a cylinder. Ω is a spatial domain, no time variations.
Differential problems
Elliptic Problem - ∇ · (μ ∇u) + β∇u + δu = f. u : Ω → ℝ. ∇ denotes divergence, ∇u denotes gradient, and u is a scalar function. μ(x) = ℝ β is a vector Ω → ℝd and can still be a function β(x) ∈ ℝd. β represents T, ∇, only a convective field, like velocity. d(β ∇u) = ∑ βi i=1 δu / ∂xi.
Let's get some physical meaning: -∇(μ∇u) is a diffusion term, for example, a thermal problem where u = Temperature and μ = Conductivity.
Numerical modeling of differential problem
Definitions
Ω to denote a domain → subset of ℝ Ω ⊂ ℝd d = 1, 2, 3. Ω is an open domain; ∂ purple is unbounded, but we set Ω bounded. Ω is connected; if you take 2 points inside the domain, you can connect them with a line inside of the domain. This is a differential problem on Ω. Normally we divide the forced domain from true variations Q = Ω × I where I = (τ0, τ) , often τ0 = ∅. Ω is a spatial domain, no time variations.
Differential problems
Elliptic Problem - ∇⋅(μ∇u) + β⋅∇u + δu = f in Ω. u : Ω → k. ∇ denotes divergence, ∇u denotes gradient, and u is a scalar function. μ(x) ∈ ℝ. β is a vector Ω → ℝd and can still be a function β(x) ∈ ℝd. β represents Vi, often a convective field, like velocity. (β⋅∇)u = Σi=1d βi 𝔡⁄dxi. -∇⋅(μ∇u) is a diffusion term, for example, a thermal problem where u = temperature and μ = conductivity.
In every elliptic problem, μ(x) > μ0 > 0 ∀x ∈ Ω. μ must be everywhere greater than zero; it is always bounded away from 0. -∇ · (μ∇u) + (β∇)u + cδu = f in Ω where β is a velocity field. (β∇)u is a convective field or an advective field. cδu is a reaction term, but it can be 0. f is called a source term or forcing term.
Example (membrane) - linearity u = displacement, μ = elastic coefficient, c = 0, β = 0, f = external forces.
To define a differential problem, it is not enough to write a differential equation; we must add boundary conditions. In an elliptic problem, we need to specify conditions on all the boundary of Ω (∂Ω).
Kinds of boundary conditions
- Dirichlet Boundary Condition (essential condition): In Dirichlet Boundary Condition, we impose the value u = g on M0 ⊂ ∂Ω. The condition is the knowledge of the value of the boundary.
- Neumann Boundary Condition (natural condition): μ ∂u/n = h, ∂u/n = t ∂u/n = in the flux across MN. With this condition, we don't know the value of the boundary.
- Robin Boundary Condition: μf ∂u/∂n + αu = h on Γf. The important thing is to fill the whole boundary Γu ∪ Γf ∪ Γn = ∂Ω.
Let's write our elliptic problem in the form L u = f where L is our differential operator L = -∇・(μ∇) + (β∇) + σ.
Classification of PDE's
The differential equations can be classified based on their mathematical formulation in 3 different families: elliptic, parabolic, and hyperbolic. L u = A∂²u/∂x1² + B∂²u/∂x2² + C∂²u/∂x1∂x2 + D∂u/∂x1 + ε∂u/∂x2 + F u = G. Coeffs A, B, C, D, E, F, ∈ R, the classification is made on the region of the △ = B²-4AC. If △ < 0.
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