Distributions and Sobolev Spaces Introduction

⚡ Key Takeaways

Distributions (generalized functions) extend the notion of a function so that every distribution is infinitely differentiable, while Sobolev spaces Wk,pW^{k,p} measure the integrability of a function together with its weak (distributional) derivatives up to order kk. Together they form the analytic backbone of modern PDE theory: weak formulations, existence/uniqueness via Hilbert-space methods, and regularity estimates. They apply wherever derivatives must be interpreted past the limits of classical calculus — shocks, point sources, finite elements, quantum mechanics. Foundational work by Sergei Sobolev (1930s) and Laurent Schwartz (1940s, Fields Medal 1950).

💡 The Core Insight

Differentiation is a chore for functions but trivial for distributions. Classical calculus forbids differentiating non-smooth functions; distribution theory dodges this by defining the derivative through the identity ⟨u′,φ⟩=−⟨u,φ′⟩\langle u', \varphi\rangle = -\langle u, \varphi'\rangle, which always makes sense because the test function φ\varphi is smooth. Sobolev spaces then quantify how many such weak derivatives an object has and how integrable they are — turning "regularity" into a measurable, topological property and converting PDE problems into geometry in Banach/Hilbert spaces.

Formal Statement

DefinitionTest Functions and Distributions

Let Ω⊆Rn\Omega \subseteq \mathbb{R}^n be open. The space of test functions is

1
D(Ω)=Cc∞(Ω)={φ∈C∞(Ω):supp⁡φ is compact, supp⁡φ⊂Ω}.\quad \mathcal{D}(\Omega) = C_c^\infty(\Omega) = \{ \varphi \in C^\infty(\Omega) : \operatorname{supp}\varphi \text{ is compact}, \ \operatorname{supp}\varphi \subset \Omega\}.

Derivation hint: A function is in Cc∞C_c^\infty iff it is infinitely differentiable and vanishes outside a compact set; the standard bump φ(x)=e−1/(1−∣x∣2)1∣x∣<1\varphi(x)=e^{-1/(1-|x|^2)}\mathbf 1_{|x|<1} exhibits non-emptiness. A sequence φj→φ\varphi_j \to \varphi in D(Ω)\mathcal{D}(\Omega) iff there is a single compact KK containing all supp⁡φj\operatorname{supp}\varphi_j and ∂αφj→∂αφ\partial^\alpha \varphi_j \to \partial^\alpha \varphi uniformly for every multi-index α\alpha. A distribution uu is a continuous linear functional u:D(Ω)→Ru : \mathcal{D}(\Omega) \to \mathbb{R} (or C\mathbb{C}); the space of all distributions is D′(Ω)\mathcal{D}'(\Omega). Continuity is equivalent to: for each compact K⊂ΩK \subset \Omega there exist C>0C>0 and N∈NN \in \mathbb{N} with

2
∣⟨u,φ⟩∣≤C∑∣α∣≤Nsup⁡x∈K∣∂αφ(x)∣∀ φ∈D(Ω), supp⁡φ⊂K.\quad |\langle u, \varphi\rangle| \le C \sum_{|\alpha|\le N} \sup_{x\in K} |\partial^\alpha \varphi(x)| \qquad \forall\, \varphi \in \mathcal{D}(\Omega),\ \operatorname{supp}\varphi\subset K.

Derivation hint: This seminorm bound is the explicit form of sequential continuity on the LF-space D(Ω)\mathcal{D}(\Omega); NN is the local order of uu.

DefinitionDistributional (Weak) Derivative

For u∈D′(Ω)u \in \mathcal{D}'(\Omega) and multi-index α=(α1,…,αn)\alpha = (\alpha_1,\dots,\alpha_n), the derivative ∂αu∈D′(Ω)\partial^\alpha u \in \mathcal{D}'(\Omega) is defined by

3
⟨∂αu,φ⟩=(−1)∣α∣⟨u,∂αφ⟩,∣α∣=α1+⋯+αn.\quad \langle \partial^\alpha u, \varphi\rangle = (-1)^{|\alpha|}\langle u, \partial^\alpha \varphi\rangle, \qquad |\alpha| = \alpha_1+\cdots+\alpha_n.

Derivation hint: Repeated integration by parts on a smooth uu, with boundary terms killed by compact support of φ\varphi, forces the sign (−1)∣α∣(-1)^{|\alpha|}; one then promotes this identity to a definition for arbitrary uu. A locally integrable u∈Lloc1(Ω)u \in L^1_{\mathrm{loc}}(\Omega) is identified with the distribution φ↦∫Ωuφ dx\varphi \mapsto \int_\Omega u\varphi\,dx. When ∂αu\partial^\alpha u (distributional) is again represented by an Lloc1L^1_{\mathrm{loc}} function gg, we call gg the weak derivative:

4
∫Ωg φ dx=(−1)∣α∣∫Ωu ∂αφ dx∀φ∈Cc∞(Ω).\quad \int_\Omega g\,\varphi\,dx = (-1)^{|\alpha|}\int_\Omega u\,\partial^\alpha\varphi\,dx \qquad \forall \varphi\in C_c^\infty(\Omega).

Derivation hint: Specialize [3] to a regular distribution and demand that the result be represented by an Lloc1L^1_{\mathrm{loc}} kernel.

DefinitionSobolev Spaces

Fix k∈N0k \in \mathbb{N}_0 and 1≤p≤∞1 \le p \le \infty. The Sobolev space is

5
Wk,p(Ω)={u∈Lp(Ω):∂αu∈Lp(Ω) for all ∣α∣≤k},\quad W^{k,p}(\Omega) = \{ u \in L^p(\Omega) : \partial^\alpha u \in L^p(\Omega)\ \text{for all } |\alpha| \le k\},

with norm

6
∥u∥Wk,p(Ω)=(∑∣α∣≤k∥∂αu∥Lp(Ω)p)1/p(1≤p<∞),∥u∥Wk,∞=max⁡∣α∣≤k∥∂αu∥L∞.\quad \|u\|_{W^{k,p}(\Omega)} = \Big(\sum_{|\alpha|\le k} \|\partial^\alpha u\|_{L^p(\Omega)}^p\Big)^{1/p} \quad (1\le p<\infty), \qquad \|u\|_{W^{k,\infty}} = \max_{|\alpha|\le k}\|\partial^\alpha u\|_{L^\infty}.

Derivation hint: Each ∂αu\partial^\alpha u is the weak derivative from [4]; the norm is the ℓp\ell^p-aggregate of the component LpL^p norms, making Wk,pW^{k,p} a closed subspace-style construction. When p=2p=2 we write Hk(Ω):=Wk,2(Ω)H^k(\Omega) := W^{k,2}(\Omega), a Hilbert space with inner product

7
⟨u,v⟩Hk=∑∣α∣≤k∫Ω∂αu ∂αv‾ dx.\quad \langle u, v\rangle_{H^k} = \sum_{|\alpha|\le k} \int_\Omega \partial^\alpha u\,\overline{\partial^\alpha v}\,dx.

Derivation hint: Polarize the p=2p=2 norm; completeness follows from completeness of L2L^2 on each derivative component. Define W0k,p(Ω)W^{k,p}_0(\Omega) as the closure of Cc∞(Ω)C_c^\infty(\Omega) in the Wk,pW^{k,p} norm (zero boundary trace), and H−k(Ω)=(H0k(Ω))′H^{-k}(\Omega) = (H^k_0(\Omega))' for negative-order spaces.

TheoremCompleteness, Embedding, Density

1. (Banach/Hilbert) Wk,p(Ω)W^{k,p}(\Omega) is a Banach space for 1≤p≤∞1 \le p \le \infty; Hk(Ω)H^k(\Omega) is a separable Hilbert space for 1≤p<∞1\le p<\infty. 2. (Meyers–Serrin, "H=WH=W") For 1≤p<∞1\le p<\infty, C∞(Ω)∩Wk,p(Ω)C^\infty(\Omega)\cap W^{k,p}(\Omega) is dense in Wk,p(Ω)W^{k,p}(\Omega). 3. (Sobolev Embedding, Ω=Rn\Omega=\mathbb{R}^n, kp<nkp<n) With p∗=npn−kpp^* = \frac{np}{n-kp} (the Sobolev conjugate),

8
Wk,p(Rn)↪Lp∗(Rn),∥u∥Lp∗≤C(n,k,p) ∥u∥Wk,p.\quad W^{k,p}(\mathbb{R}^n) \hookrightarrow L^{p^*}(\mathbb{R}^n), \qquad \|u\|_{L^{p^*}} \le C(n,k,p)\,\|u\|_{W^{k,p}}.

Derivation hint: For k=1k=1 the Gagliardo–Nirenberg–Sobolev inequality follows from the fundamental theorem of calculus along each axis plus the generalized Hölder inequality; iterate for higher kk. 4. (Morrey, kp>nkp>n) Wk,p(Rn)↪C0,γ(Rn)W^{k,p}(\mathbb{R}^n) \hookrightarrow C^{0,\gamma}(\mathbb{R}^n) with Hölder exponent γ=k−n/p\gamma = k - n/p (mod 1), so functions become continuous (even Hölder). 5. (Rellich–Kondrachov) If Ω\Omega is bounded with Lipschitz boundary and kp<nkp<n, then Wk,p(Ω)↪↪Lq(Ω)W^{k,p}(\Omega) \hookrightarrow\hookrightarrow L^{q}(\Omega) compactly for all 1≤q<p∗1\le q<p^*.

Why It Holds

ProofSobolev Inequality for W1,1(Rn)W^{1,1}(\mathbb R^n) — the prototype

We prove the sharp scaling case p=1p=1, k=1k=1: ∥u∥Ln/(n−1)≤C∥∇u∥L1\|u\|_{L^{n/(n-1)}} \le C\|\nabla u\|_{L^1} for u∈Cc∞(Rn)u\in C_c^\infty(\mathbb R^n).

Step 1 — One-dimensional control. For each coordinate ii, the fundamental theorem of calculus gives

9
∣u(x)∣≤∫−∞∞∣∂iu(x1,…,t,…,xn)∣ dt=:gi(x^i),\quad |u(x)| \le \int_{-\infty}^{\infty} |\partial_i u(x_1,\dots,t,\dots,x_n)|\,dt =: g_i(\hat x_i),

Derivation hint: u(x)=∫−∞xi∂iu dtu(x)=\int_{-\infty}^{x_i}\partial_i u\,dt and uu has compact support, so bound the integral over all of R\mathbb R; gig_i does not depend on xix_i.

Step 2 — Multiply the nn estimates. Raise to the power 1/(n−1)1/(n-1) and multiply over ii:

10
∣u(x)∣nn−1≤∏i=1n(∫R∣∂iu∣ dt)1n−1.\quad |u(x)|^{\frac{n}{n-1}} \le \prod_{i=1}^n \Big(\int_{\mathbb R}|\partial_i u|\,dt\Big)^{\frac{1}{n-1}}.

Derivation hint: Each factor ∣u∣1/(n−1)≤gi1/(n−1)|u|^{1/(n-1)}\le g_i^{1/(n-1)}; multiplying all nn of them produces ∣u∣n/(n−1)|u|^{n/(n-1)} on the left.

Step 3 — Integrate iteratively with generalized Hölder. Integrate in x1x_1, pulling out the factor independent of x1x_1, and apply Hölder with n−1n-1 exponents each equal to n−1n-1. Repeating in x2,…,xnx_2,\dots,x_n yields

11
∫Rn∣u∣nn−1 dx≤∏i=1n(∫Rn∣∂iu∣ dx)1n−1.\quad \int_{\mathbb R^n}|u|^{\frac{n}{n-1}}\,dx \le \prod_{i=1}^n \Big(\int_{\mathbb R^n}|\partial_i u|\,dx\Big)^{\frac{1}{n-1}}.

Derivation hint: At each integration the term lacking the integration variable comes out; the remaining n−1n-1 terms are paired against each other via Hölder’s inequality with conjugate exponents (n−1,…,n−1)(n-1,\dots,n-1).

Step 4 — AM–GM finish. Take the (n−1)/n(n-1)/n power and apply the arithmetic–geometric mean inequality to the product:

12
∥u∥Ln/(n−1)≤∏i=1n∥∂iu∥L11/n≤1n∑i=1n∥∂iu∥L1≤∥∇u∥L1.\quad \|u\|_{L^{n/(n-1)}} \le \prod_{i=1}^n \|\partial_i u\|_{L^1}^{1/n} \le \frac1n \sum_{i=1}^n \|\partial_i u\|_{L^1} \le \|\nabla u\|_{L^1}.

Derivation hint: Geometric mean ≤\le arithmetic mean of the nn quantities ∥∂iu∥L1\|\partial_i u\|_{L^1}; absorb constants. Density of Cc∞C_c^\infty extends the inequality to all of W1,1W^{1,1}. The general W1,pW^{1,p} case applies this to ∣u∣γ|u|^{\gamma} with γ=(n−1)pn−p\gamma=\frac{(n-1)p}{n-p} and uses Hölder once more. ■\qquad\blacksquare

∎
LS
Laurent Schwartz
1915–2002

Schwartz unified decades of "improper" objects — Heaviside’s operational calculus, Dirac’s delta, Hadamard’s finite parts — into the rigorous theory of distributions in Théorie des distributions (1950–51). His decisive idea was duality: define generalized functions as continuous linear functionals on a carefully topologized space of test functions, so that operations on the singular object are dual to operations on smooth functions. For this he received the Fields Medal (1950). He emphasized that the "trick" was less in the objects than in choosing the right test-function topology, the inductive-limit space D\mathcal D, whose dual is large enough to host delta and its derivatives.

Building Intuition

🧠 Intuition

Think of a distribution as a measuring device, not a pointwise object. You never ask "what is u(x)u(x)?"; you ask "what is the weighted average ⟨u,φ⟩\langle u,\varphi\rangle against this smooth probe φ\varphi?" The Dirac delta is the device that returns φ(0)\varphi(0) — it reads a value, not an average, which no ordinary function can do. Differentiation works by passing the derivative to the probe. Since you can’t differentiate uu directly, you let the smooth φ\varphi absorb the derivative, paying a sign (−1)∣α∣(-1)^{|\alpha|} as the price of integration by parts. Because φ\varphi is infinitely smooth, this never fails — hence every distribution is infinitely differentiable. Sobolev spaces add a bookkeeping ledger: not just "does the derivative exist as a distribution," but "is it integrable to power pp?" The number kk counts derivatives; pp counts integrability. The Sobolev embedding theorem is the exchange rate: spend enough derivatives (large kpkp relative to dimension nn) and you buy back classical continuity. The competition is always against dimension nn — high dimension makes regularity expensive.

Figure
Duality of differentiation: the weak derivative passes d/dxd/dx onto the smooth test function
⟨u′, φ⟩ = −⟨u, φ′⟩ x u = Heaviside step (jump) φ ∈ C∞_c (smooth probe) u′ = δ (point mass) Classical u′ undefined at jump — but ⟨u′,φ⟩ = −∫u φ′ dx = φ(0) is perfectly defined.

Worked Examples

example[Weak derivative of the Heaviside step] Given: the Heaviside function H(x)=1H(x)=1 for x>0x>0, 00 for x<0x<0 on R\mathbb R. Find H′H' in D′(R)\mathcal D'(\mathbb R).

Step 1. Apply [3] with ∣α∣=1|\alpha|=1:

⟨H′,φ⟩=−⟨H,φ′⟩=−∫RH(x)φ′(x) dx=−∫0∞φ′(x) dx.\langle H', \varphi\rangle = -\langle H,\varphi'\rangle = -\int_{\mathbb R} H(x)\varphi'(x)\,dx = -\int_0^\infty \varphi'(x)\,dx.

Step 2. Compute the elementary integral; φ\varphi has compact support so φ(∞)=0\varphi(\infty)=0:

−∫0∞φ′(x) dx=−[φ(∞)−φ(0)]=φ(0).-\int_0^\infty \varphi'(x)\,dx = -\big[\varphi(\infty)-\varphi(0)\big] = \varphi(0).

Step 3. The functional φ↦φ(0)\varphi\mapsto\varphi(0) is by definition the Dirac delta δ0\delta_0.

H′=δ0in D′(R).\boxed{H' = \delta_0 \quad\text{in } \mathcal D'(\mathbb R).}

Consequence (Sobolev): H∈Wloc1,pH \in W^{1,p}_{\mathrm{loc}}? No — δ0∉Lp\delta_0\notin L^p for any pp. So H∉W1,pH \notin W^{1,p}. But H∈W0,p=LpH \in W^{0,p}=L^p locally. The jump costs all regularity beyond L∞L^\infty.

ExampleIs u(x)=∣x∣−su(x)=|x|^{-s} in H1H^1 of the unit ball in R3\mathbb R^3?

Given: Ω=B(0,1)⊂R3\Omega = B(0,1)\subset\mathbb R^3 (n=3n=3), u(x)=∣x∣−su(x)=|x|^{-s}, s>0s>0. Determine the threshold ss for which u∈H1(Ω)=W1,2u\in H^1(\Omega)=W^{1,2}.

Step 1 — L2L^2 condition. Using spherical coordinates dx=4πr2 drdx = 4\pi r^2\,dr:

∫Ω∣u∣2 dx=4π∫01r−2s r2 dr=4π∫01r2−2s dr,\int_\Omega |u|^2\,dx = 4\pi\int_0^1 r^{-2s}\,r^2\,dr = 4\pi\int_0^1 r^{2-2s}\,dr,

finite iff 2−2s>−12-2s>-1, i.e. s<3/2s < 3/2.

Step 2 — Gradient. ∣∇u∣=s ∣x∣−s−1|\nabla u| = s\,|x|^{-s-1}, so

∫Ω∣∇u∣2 dx=4πs2∫01r−2s−2 r2 dr=4πs2∫01r−2s dr,\int_\Omega |\nabla u|^2\,dx = 4\pi s^2\int_0^1 r^{-2s-2}\,r^2\,dr = 4\pi s^2\int_0^1 r^{-2s}\,dr,

finite iff −2s>−1-2s>-1, i.e. s<1/2s < 1/2.

Step 3 — Intersect. The binding constraint is the gradient:

u=∣x∣−s∈H1(B1⊂R3)  ⟺  0<s<12.\boxed{u=|x|^{-s}\in H^1(B_1\subset\mathbb R^3) \iff 0 < s < \tfrac12.}

Cross-check with embedding. Here kp=1⋅2=2<n=3kp = 1\cdot 2 = 2 < n=3, so H1H^1 does not embed into L∞L^\infty in 3D — unbounded functions like ∣x∣−s|x|^{-s}, s<1/2s<1/2, are legitimately in H1H^1. The Sobolev conjugate is p∗=3⋅23−2=6p^*=\frac{3\cdot2}{3-2}=6; indeed ∣x∣−s∈L6|x|^{-s}\in L^6 iff 6s<36s<3 iff s<1/2s<1/2, consistent.

Common Misconceptions

⚠️ Common mistake

"Weak derivative = classical derivative wherever the function is differentiable." False in general. The weak derivative is determined by behavior on sets of positive measure plus singular structure. The Cantor–Lebesgue (devil's staircase) function c(x)c(x) has classical derivative 00 almost everywhere, yet its distributional derivative is the singular Cantor measure, not the zero function. So c∉W1,1c \notin W^{1,1} even though c′=0c'=0 a.e. — the pointwise-a.e. derivative ignores the measure concentrated on a null set.

⚠️ Common mistake

"Sobolev functions have pointwise values." Generally false. Elements of Wk,pW^{k,p} are equivalence classes modulo a.e. equality. A "value at a point" makes sense only after the trace theorem (on lower-dimensional sets) or Morrey embedding (when kp>nkp>n gives a continuous representative). Asking u(0)u(0) for u∈H1(R3)u\in H^1(\mathbb R^3) is meaningless without further structure.

CounterexampleMultiplication of distributions is impossible in general

There is no associative product on D′(R)\mathcal D'(\mathbb R) extending pointwise multiplication and the usual calculus (Schwartz's impossibility). Naively, δ⋅H\delta \cdot H would need to satisfy contradictory rules. Consider, with H2=HH^2 = H and H′=δH' = \delta:

δ=(H)′=(H2)′=2HH′=2Hδ  ⟹  δ=2Hδ.\delta = (H)' = (H^2)' = 2HH' = 2H\delta \implies \delta = 2H\delta.

Yet also H3=HH^3=H gives δ=(H3)′=3H2H′=3Hδ\delta = (H^3)' = 3H^2 H' = 3H\delta, so 2Hδ=3Hδ2H\delta = 3H\delta, forcing Hδ=0H\delta=0 and hence δ=0\delta=0 — absurd. Moral: products like δ2\delta^2 or HδH\delta are undefined; one needs Colombeau algebras or microlocal wavefront-set conditions to multiply selectively.

Connections

connection

Distributions and Sobolev spaces sit at the crossroads of analysis:

  • <a class="wiki-link" href="/wiki/fourier-transform">Fourier Transform</a> — On Rn\mathbb R^n, HsH^s is characterized by ∫(1+∣ξ∣2)s∣u^(ξ)∣2 dξ<∞\int (1+|\xi|^2)^s |\hat u(\xi)|^2\,d\xi<\infty, defining fractional and negative order spaces HsH^s for all real ss. The transform turns differentiation into multiplication by iξi\xi, making smoothness a decay condition on u^\hat u.
  • <span class="wiki-link-missing">Lp Spaces</span> — Sobolev spaces are built on top of LpL^p; the embedding theorems trade derivative count kk against integrability pp and dimension nn.
  • <span class="wiki-link-missing">Weak Solutions of PDEs</span> — The Lax–Milgram theorem on H01H^1_0 produces unique weak solutions of elliptic equations; this is the payoff of the whole machinery.
  • <a class="wiki-link" href="/wiki/hilbert-spaces">Hilbert Spaces</a> — HkH^k inherits orthogonality, projections, and the Riesz representation theorem, enabling variational methods.
  • <span class="wiki-link-missing">Tempered Distributions</span> — The dual S′\mathcal S' of the Schwartz space S\mathcal S is the natural home for the Fourier transform, intermediate between D′\mathcal D' and finite-energy spaces.
  • <span class="wiki-link-missing">Measure Theory</span> — Radon measures are exactly the distributions of order 00, linking the abstract dual to classical integration.

Real-World Applications

🔬 Where this appears

Historical Development

⏳ History
- 1822 — Fourier introduces what becomes the delta as a limit of his integral kernel, used freely but without rigor.
- 1894–1920s — Heaviside develops operational calculus; physicists differentiate discontinuities pragmatically, drawing criticism from rigorists.
- 1908 — Hadamard introduces finite parts (parties finies) of divergent integrals — an early regularization that foreshadows distributions.
- 1926–1927 — Dirac formalizes the delta "function" δ\delta in quantum mechanics; mathematically illegitimate but operationally indispensable.
- 1935–1938 — Sergei Sobolev (Leningrad/Moscow) defines generalized functions and the spaces Wl,pW^{l,p} (now bearing his name) to solve the wave/Cauchy problem; proves the embedding inequality. This is the genuine first rigorous theory.
- 1936 — Bochner & Friedrichs develop related notions of generalized derivatives and mollification ("Friedrichs mollifiers").
- 1944–1948 — Laurent Schwartz crystallizes the duality framework, choosing the topology on D\mathcal D and identifying D′\mathcal D'.
- 1950–1951 — Schwartz publishes Théorie des distributions (2 vols); receives the Fields Medal (1950). Tempered distributions S′\mathcal S' and the distributional Fourier transform follow.
- 1955 — Lax / Sobolev-Kondrachov / Rellich mature compact embeddings; Meyers–Serrin (1964) prove "H=WH=W", unifying two historical definitions of Sobolev spaces.
- 1960s–70s — Hörmander founds microlocal analysis and the wavefront set, refining where distributions can be multiplied and how singularities propagate.

Subtleties & Limits

open-problem

Multiplication and nonlinearity. Distribution theory is linear by design; nonlinear PDEs (Navier–Stokes, nonlinear wave/Schrödinger, stochastic PDEs) require multiplying rough objects, which is generically forbidden (see the impossibility counterexample). Partial resolutions — Colombeau algebras, paraproducts (Bony), rough paths (Lyons), and regularity structures (Hairer, Fields Medal 2014) — provide self-consistent calculi for specific equations, but no universal nonlinear theory of distributions exists.

Global regularity of Navier–Stokes (Clay Millennium) is the headline open question framed entirely in Sobolev language: do 3D weak (Leray–Hopf) solutions in Lt2Hx1L^2_t H^1_x remain smooth for all time, or can the H1H^1 norm blow up?

Optimal constants and rigidity. The sharp constant in the Sobolev inequality [8] and the classification of extremizers (Aubin–Talenti functions) connect to the Yamabe problem in conformal geometry; sharp traces, fractional analogues (HsH^s, Ws,pW^{s,p} via Gagliardo seminorms), and stability of these inequalities remain active.

See Also

Fourier Transform · Tempered Distributions · Lax-Milgram Theorem · Rellich-Kondrachov Theorem · Bounded Variation Functions · Sobolev Embedding Theorem · Green's Functions · Finite Element Method