BS I c Gabriel Nagy
Banach Spaces I: Normed Vector Spaces Notes from the Functional Analysis Course (Fall 07 - Spring 08)
Banach spaces are the most manageable among all types of topological vector spaces, particularly due to their metric structure. Before we start treating them, we will first treat their natural precursors to which this section is devoted. Convention. Throughout this note K will be one of the fields R or C, and all vector spaces are over K. A. Normable and Normed Vector Spaces
The starting point of our discussion is Exercise 17 from LCVS III, which we recall here as the following: Remark 1. For a locally convex topological vector space (X , T), the following are equivalent: (i) There exists a bounded neighborhood of 0;
(ii) There exists some neighborhood V of 0, such that {εV}ε>0 is a basic neighborhood system for 0. (iii) There exists one seminorm p, so that T = T(p). Moreover, any seminorm with this property is a norm, i.e. one has the implication: p(x) = 0 ⇒ x = 0. Definition. A locally convex vector space, satisfying (one of) these three equivalent conditions, is declared normable. Of course, a normable topological vector space is metrizable, by the results from LCVS III. Notations. Norms on vector spaces will be typically denoted using the symbol k . k, that is, kxk stands for (the old) p(x). On occasion the norm notation will be accompanied by subscripts or superscripts.
Remark 2. Suppose X1 and X2 are normable spaces, with their topologies defined by norms k . k1 and k . k2, respectively. For a linear map T : X1 → X2, the following conditions are equivalent: (i) T is continuous; (i’) T is continuous at 0; (ii) there exists a constant C ≥ 0, such that
kT xk2 ≤ Ckxk1, ∀ x ∈ X1.
1 This statement follows directly from Theorem 4 from LCVS V.
Remarks 3-4. Suppose k . k1 and k . k2 are two norms on a vector space X , and let T1 and T2 be the locally convex topologies defined by them.
3. The condition that T2 is weaker than T1 is equivalent to the existence of a constant C > 0, such that: kxk2 ≤ Ckxk1, ∀ x ∈ X .
This follows from the preceding Remark, since the condition T2 ⊂ T1 is equivalent to the continuity of the identity map I :(X , T1) → (X , T2). 4. The condition that the two topologies coincide is equivalent to the existence of two constants C, D > 0, such that
Dkxk1 ≤ kxk2 ≤ Ckxk1, ∀ x ∈ X . (1)
Two norms satisfying condition (1) are said to be equivalent. Comment. From the topological point of view, to define a normable topology on a vector space X is the same as identifying an equivalence class (in the sense defined above) in the set of all norms. When a (distinguished) norm is identified, that is, when a pair (X , k . k) is considered, we call the pair a normed vector space. Therefore, the difference between “normable” and “normed” lies in the possibility that two different norms might produce the same topology. Example 1. On a finite dimensional vector space X there exists a unique Hausdorff linear topology. Moreover, this topology is normable, so on X any two norms are equivalent. For instance, in the case when X = Kn, this unique topology is the product topology, which can be defined by the norm
n kxk∞ = max{|x1|,..., |xn|}, ∀ x = (x1, . . . , xn) ∈ K . Q If S is an infinite set, then neither the product space K (equipped with the product L S topology), nor the direct sum S K (equipped with the locally convex sum topology) is normable. (In the product space every neighborhood of 0 contains an infinite dimensional linear space, so it cannot be bounded. The direct sum is not even metrizable.) Definition. Given a normed vector space (X , k . k), the (locally convex) topology defined by the k . k is referred to as the norm topology. In terms of convergence, the condition k . k xλ −−→ x is equivalent to the condition kxλ − xk → 0. We denote (with k . k fixed), for any r > 0, the closed ball {x ∈ X : kxk ≤ r} by (X )r. Using this notation, the collection (X )r r>0 constitutes a basic neighborhood system for 0 in the norm topology. B. Methods of Constructing Norms
In this section we outline three methods for constructing norms. The first one is simply a restatement of well known fact from the theory of metric spaces (see also Remark 1 from TVS IV).
2 Remark 5. If (X , k . k) is a normed vector space and T denotes its norm topology, then for every linear subspace Y ⊂ X , the restriction of k . k to Y is a norm, and furthermore, the corresponding norm topology on Y coincides with the induced topology T Y . The second method is an easy application of Exercise 2 from LCVS III (or Lemma 2 from TVS IV). Proposition-Definition 1. Suppose (X , k . k) is a normed space and Y ⊂ X is a linear subspace, which is closed in the norm topology. If we consider the quotient space X /Y and we denote by π : X → X /Y the quotient map, then the map k . kˆ: X /Y → [0, ∞) given by
kvkˆ= inf{kxk : x ∈ X , π(x) = v}, v ∈ X /Y defines a norm on X /Y. Moreover, the norm topology defined by k . kˆ coincides with the quotient topology. The norm k . kˆis referred to as the quotient norm. Proof. From Exercise 2 in LCVS III we know that k . kˆ is a seminorm, which defines the quotient topology. Since the quotient topology is Hausdorff, it follows that k . kˆis in fact a norm. The third method is a bit more elaborate, but quite effective, as shown by the examples below. It uses dual pairs, as introduced in DT I. Proposition-Definition 2. Suppose X and Y are in a dual pairing, defined by means of two injective linear maps1
#: X 3 x 7−→ x# ∈ Y0 #: Y 3 y 7−→ y# ∈ X 0 satisfying: x#(y) = y#(x), ∀ x ∈ X , y ∈ Y. Suppose M ⊂ Y is some non-empty absorbing set, and define the map k . kM : X → [0, ∞] by
# kxkM = sup |x (y)|. y∈M
(i) The set XM = {x ∈ X : kxkM < ∞} is a linear subspace in X .
(ii) k . kM is a norm, when restricted to XM.
2 # (iii) If we consider the absolute polar M = {x ∈ X : |x (y)| ≤ 1, ∀ y ∈ M}, then we
S have the equalities: XM = span(M ) = t>0 tM .
(iv) The unit ball (XM)1 coincides with M.
# (v) The norm topology on XM is stronger than the induced w -topology.
Proof. Before we prove each of the statements (i)-(v) we first show that k . kM has the following properties3
1 Here X 0 and Y0 denote the algebraic duals of X and Y. 2 # From DT I we know that M is convex, balanced, and closed in the w -topology. 3 We use the usual conventions: number + ∞ = ∞ + ∞ = ∞ and (positive number) · ∞ = ∞.
3 (a) kx1 + x2kM ≤ kx1kM + kx2kM, ∀ x1, x2 ∈ M;
(b) if α ∈ K, α 6= 0, then kαxkM = |α| · kxkM, ∀ x ∈ X ;
(c) for x ∈ X , one has the equivalence kxkM = 0 ⇔ x = 0.
Property (a) is quite trivial, since for every y ∈ M we have the inequalities
# # # # # |(x1 + x2) (y)| = |x1 (y) + x2 (y)| ≤ |x1 (y)| + |x2 (y)| ≤ kx1kM + kx2kM.
For property (b), we first notice that, for every y ∈ M we have the inequality |(αx)#(y)| = # # |α · x (y)| = |α| · |x (y)| ≤ |α| · kxkM, so taking supremum yields
kαxkM ≤ |α| · kxkM, ∀ x ∈ X , α 6= 0. (2)
If we use the above inequality with α−1 in place of α, and αx in place of x, we also get −1 −1 kxkM = kα (αx)kM ≤ |α | · kαxkM, which yields
|α| · kxkM ≤ kαxkM, ∀ x ∈ X , α 6= 0, (3) and then (b) follows from (2) and (3). Finally, to prove (c) we use the fact that M is absorbing in Y. Start with x such that kxkM = 0. On the one hand, by the definition of k . kM, we know that x#(y) = 0, ∀ y ∈ M. (4) On the other hand, since M is absorbing, for every y ∈ Y there exists ρ > 0 such that ρy ∈ M, so by (4) we have x#(y) = ρ−1x#(ρy) = 0, thus proving that x# = 0. Finally, the injectivity of x 7−→ x# forces x = 0. Statements (i)-(ii) are now obvious from (a)-(c). Statement (iv) is obvious from the definition of k . kM. Clearly (iii) follows from (iv). Finally to prove (v), we start with some w# net (xλ)λ∈Λ in XM, which converges in norm to 0, and we show that xλ −−→ 0, which means that # xλ (y) → 0, ∀ y ∈ Y. (5) # First of all, since we have the inequality |xλ (y)| ≤ kxλkM, ∀ y ∈ M, the condition (5) is clearly satisfied if y ∈ M. By linearity we now have
# xλ (ρy) → 0, ∀ y ∈ M, ρ > 0, and then the desired conclusion (5) follows from the fact that M is absorbing in Y. Remarks 6-7. Suppose X and Y are in a dual pairing, and M ⊂ Y is non-empty and absorbing.
# 6. The set M is w -bounded, if and only if XM = X . In this case k . kM defines a norm on the whole space X , and the norm topology TM on X , defined by k . kM, is weaker than the strong topology (see DT II).
4 7. If M is w#-compact, convex, balanced (thus w#-bounded), then the norm topology TM is weaker than the Mackey topology (see DT II). In particular, the correspondence #: Y 3 y 7−→ y# ∈ X 0 establishes a topological linear isomorphism:
# ∼ ∗ ∗ (Y, w ) −→ ((X , TM) , w ).
Comment. As we shall see a little later, all normed spaces can be constructed according to the recipe indicated in Remark 7.
C. Examples: the `p-spaces
In this section we specialize the construction outlined in Proposition-Definition 2 to the following situation (all notations will be fixed throughout the entire sub-section): • S will denote a non-empty set (the interesting case will be when S is infinite); Q •X will denote the product space S K; L •Y will denote the direct sum S K. The spaces X and Y will be put in a dual pairing by
# # X x (y) = y (x) = xsys, ∀ x = (xs)s∈S ∈ X , y = (ys)s∈S ∈ Y. s∈S
(By construction, for every y = (ys)s∈S ∈ Y, the set supp y = {s ∈ S : ys 6= 0} is finite, so the above sum has only finitely many non-zero terms.)
Notations. For every “number” p ∈ [1, ∞], we define the set Mp ⊂ Y as follows: {y ∈ Y : maxs∈S |ys| ≤ 1}, if p = 1 p P p−1 Mp = {y ∈ Y : s∈S |ys| ≤ 1}, if 1 < p < ∞ P {y ∈ Y : s∈S |ys| ≤ 1}, if p = ∞ L (By the definition of Y as S K, the sums used in the definitions of Mp, p ∈ (1, ∞], involve only finitely many non-zero terms.) Using the notations from Proposition-Definition 2, we have, for each p ∈ [1, ∞] a vector space X , which from now on we denote by `p (S), equipped with a norm k . k , which Mp K Mp from now on we will simply denote by k . kp. When K = C, the field will be omitted from the notation. When S = N the set will also be omitted from the notation. The explicit presentation of the normed spaces (`p (S), k . k ), p ∈ [1, ∞] is as follows. K p Q Proposition 3. Use the notations as above, and fix some element x = (xs)s∈S ∈ S K. (i) The condition that x belongs to `∞(S) is equivalent to the condition: sup |x | < ∞. K s∈S s Moreover, in this case one has the equality
kxk∞ = sup |xs|. (6) s∈S
5 (ii) If 1 ≤ p < ∞, the condition that x belongs to `p (S) is equivalent to the condition: K P p s∈S |xs| < ∞. Moreover, in this case one has the equality
1/p X p kxkp = |xs| . (7) s∈S
Q Proof. (i). For every x ∈ S K, denote the quantity sups∈S |xs| ∈ [0, ∞] by Q∞(x). To prove the “only if” implication, assume first x ∈ `∞(S), so K # kxk∞ = sup |x (y)| < ∞. (8) y∈M∞ L In particular, if we consider, for every t ∈ S the element δt = (δts)s∈S ∈ S K (here δts denotes the Kronecker symbol, defined to be 1 if s = t, and 0, otherwise), then obviously # x (δt) = xt, and δt ∈ M∞, so by (8) we get |xt| ≤ kxk∞, ∀ t ∈ S, so
Q∞(x) ≤ kxk∞, (9) thus proving the desired implication. Conversely, assume Q (x) < ∞, and let us prove that x ∈ `∞(S). If we start with an ∞ K arbitrary y = (ys)s∈S ∈ M∞, then using the inequalities |xs| ≤ Q∞(x), we have # X X X |x (y)| = xsys ≤ |xs| · |ys| ≤ Q∞(x) · |ys| ≤ Q∞(x), s∈supp y s∈supp y s∈supp y so taking supremum (over all y ∈ M ) not only shows that x ∈ `∞(S), but also proves the ∞ K inequality kxk∞ ≤ Q∞(x), which combined with (9) yields the desired equality (6). P p (ii). Denote, for p ∈ [1, ∞), the quantity s∈S |xs| ∈ [0, ∞] by Qp(x). (By convention, P p p we define s∈S |xs| = ∞, if the S-tuple (|xs| )s∈S is not summable.) With this notation, the desired equality (7) reads
Q (x) = kxk p, ∀ x ∈ `p (S). (10) p p K We divide now the proof into two cases: (a) 1 < p < ∞; (b) p = 1. p 1 1 (a) Denote the number by q, so that + = 1, and the set M is defined as p − 1 p q p
M X q Mp = {y = (ys)s∈S ∈ K : |ys| ≤ 1}. (11) S s∈S
To prove the “only if” implication, fix some element x ∈ `p (S), so K # kxkp = sup |x (y)| < ∞, (12) y∈Mp
6 and let us show that Qp(x) < ∞. Let us define, for every finite set F ⊂ S, the quantity P p L Qp,F (x) = s∈F |xs| , and the element yF = (yF s)s∈S ∈ S K as follows: |x |p s , if s ∈ F and x 6= 0 F 1/q s xsQp (x) yF s = 0, if either s 6∈ F , or xs = 0. Remark that, by construction, using the identity qp − q = p, we have
p |xs| , if s ∈ F and xs 6= 0 q Qp,F (x) |yF s| = 0, if either s 6∈ F , or xs = 0.
P q so s∈S |yF s| is either equal to 0, if xs = 0, ∀ s ∈ F , or equal to 1 otherwise. In any case, it follows that yF belongs to Mp, and we have 0, if xs = 0, ∀ s ∈ F # X x (yF ) = xsyF s P p s∈F |xs| s∈F 1−1/q 1/p 1/q = Qp,F (x) = Qp,F (x) , otherwise Qp,F (x) By (12) the above estimate yields