Statistical convergence in a paranormed space
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* Corresponding author: Abdullah Alotaibi aalotaibi@kau.edu.sa
Department of Mathematics, King Abdulaziz University, P.O. Box 80203, Jeddah 21589, Saudi Arabia
Journal of Inequalities and Applications 2012, 2012:39 doi:10.1186/1029-242X-2012-39
The electronic version of this article is the complete one and can be found online at: http://www.journalofinequalitiesandapplications.com/content/2012/1/39
| Received: | 14 August 2011 |
| Accepted: | 21 February 2012 |
| Published: | 21 February 2012 |
© 2012 Alotaibi and Altheabi et al; licensee Springer.
This is an open access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Abstract
In this article, we define the notion of statistical convergence, statistical Cauchy and strongly p-Cesàro summability in a paranormed space. We establish some relations between them.
AMS subject classification (2000): 41A10; 41A25; 41A36; 40A05; 40A30.
Keywords:
density; statistical convergence; statistical Cauchy; para-normed space; strongly p-Cesàro summability.1 Introduction and preliminaries
The concept of statistical convergence for sequences of real numbers was introduced by Fast [1] and Steinhaus [2] independently in the same year 1951 and since then several generalizations and applications of this notion have been investigated by various authors, namely [3-11]. This notion was defined in normed spaces by Kolk [12] and in locally convex Hausdorff topological spaces by Maddox [13]. Çakalli [14] extended this notation to topological Hausdorff groups. Recently, in [15,16], the concept of statistical convergence is studied in probabilistic normed space and in intuitionistic fuzzy normed spaces, respectively. In this article, we shall study the concept of statistical convergence, statistical Cauchy, and strongly p-Cesàro summability in a paranormed space.
Let K be a subset of the set of natural numbers ℕ. Then the asymptotic density of K denoted by δ(K), is defined as
, where the vertical bars denote the cardinality of the enclosed set.
A number sequence x = (xk) is said to be statistically convergent to the number L if for each ϵ > 0, the set K(ϵ) = {k ≤ n: |xk - L| > ϵ} has asymptotic density zero, i.e.,
In this case we write st-lim x = L.
A number sequence x = (xk) is said to be statistically Cauchy sequence if for every ϵ > 0, there exists a number N = N(ϵ) such that
The concept of paranorm is a generalization of absolute value (see [17]).
A paranorm is a function g: X → ℝ defined on a linear space X such that for all x, y, z ∈ X
(P1) g(x) = 0 if x = θ
(P2) g(-x) = g(x)
(P3) g(x + y) ≤ g(x) + g(y)
(P4) If (αn) is a sequence of scalars with αn → α0 (n → ∞) and xn, a ∈ X with xn → a (n → ∞) in the sense that g(xn - a) → 0 (n → ∞), then αnxn → α0a (n → ∞), in the sense that g(αnxn - α0a) → 0 (n → ∞).
A paranorm g for which g(x) = 0 implies x = θ is called a total paranorm on X, and the pair (X, g) is called a total paranormed space.
Note that each seminorm (norm) p on X is a paranorm (total) but converse need not be true.
In this article, we define and study the notion of convergence, statistical convergence, statistical Cauchy, and strong summability by a modulus function in a paranormed space.
Let (X, g) be a paranormed space.
Definition 1.1. A sequence x = (xk) is said to be convergent (or g-convergent) to the number ξ in (X, g) if for every ε > 0, there exists a positive integer k0 such that g(xk - ξ) < ε whenever k ≥ k0. In this we write g-lim x = ξ, and ξ is called the g-limit of x.
Definition 1.2. A sequence x = (xk) is said to be statistically convergent to the number ξ in (X, g) (or g(st)-convergent) if for each ϵ > 0,
In this case, we write g(st)-lim x = ξ. We denote the set of all g(st)-convergent sequences by Sg.
Definition 1.3. A number sequence x = (xk) is said to be statistically Cauchy sequence in (X, g) (or g(st)-Cauchy) if for every ϵ > 0 there exists a number N = N(ϵ) such that
2 Main results
Theorem 2.1. If a sequence x = (xk) is statistically convergent in (X, g) then g(st)-limit is unique.
Proof. Suppose that g(st)-lim x = ξ1 and g(st)-lim x = ξ2. Given ε > 0, define the following sets as:
Since g(st)-lim x = ξ1, we have δ(K1(ε)) = 0. Similarly, g(st)-lim x = ξ2 implies that δ(K2(ε)) = 0. Now, let K(ε) = K1(ε)∪K2(ε). Then δ(K(ε)) = 0 and hence the compliment KC(ε) is a nonempty set and δ(KC(ε)) = 1. Now if k ∈ ℕ\K(ε), then we have g(ξ1-ξ2) ≤ g(xn-ξ1)+g(xn-ξ2) < ε/2+ε/2 = ε.
Since ε > 0 was arbitrary, we get g(ξ1 - ξ2) = 0 and hence ξ1 = ξ2.
Theorem 2.2. If g-lim x = ξ then g(st)-lim x = ξ but converse need not be true in general.
Proof. Let g-lim x = ξ. Then for every ε > 0, there is a positive integer N such that
for all n ≥ N. Since the set A(ϵ):= {k ∈ ℕ: g(xk - ξ) ≥ ε} ⊂ {1, 2, 3, ...}, δ(A(ϵ)) = 0. Hence g(st)-lim x = ξ.
The following examle shows that the converse need not be true.
Example 3.1. Let X = ℓ(1/k): = {x = (xk): ∑k |xk|1/k < ∞} with the paranorm g(x) = (∑k |xk|1/k). Define a sequence x = (xk) by
and write
We see that
and hence
Therefore g-lim x does not exist. On the other hand δ(K(ε)) = 0, that is, g(st)-lim x = 0.
Theorem 2.3. Let g(st)-lim x = ξ1 and g(st) - lim y = ξ2. Then
(i) g(st)-lim(x ± y) = ξ1 ± ξ2,
(ii) g(st)-lim αx = αξ1, α ∈ ℝ.
Proof. It is easy to prove.
Theorem 2.4. A sequence x = (xk) in (X, g) is statistically convergent to ξ if and only if there exists a set K = {k1 < k2 < ⋯ < kn < ⋯ } ⊆ ℕ with δ(K) = 1 such that
.
Proof. Suppose that g(st)-lim x = ξ. Now, write for r = 1, 2, ....
and
Then δ(Kr) = 0,
and
Now we have to show that for n ∈ Mr,
is g-convergent to ξ. On contrary suppose that
is not g-convergent to ξ. Therefore there is ε > 0 such that
for infinitely many terms. Let
and
. Then
and by (2.4.1), Mr ⊂ Mε. Hence δ(Mr) = 0, which contradicts (2.4.2) and we get that
is g-convergent to ξ.
Conversely, suppose that there exists a set K = {k1 < k2 < k3 < ⋯ < kn < ⋯} with δ(K) = 1 such that
. Then there is a positive integer N such that g(xn - ξ) < ε for n > N. Put Kε(t): = {n ∈ ℕ: g(xn-ξ) ≥ ε} and K': = {kN+1, kN+2, ...}. Then δ(K') = 1 and Kε ⊆ ℕ-K' which implies that δ(Kε) = 0. Hence g(st)-lim x = ξ.
Theorem 2.5. Let (X, g) be a complete paranormed space. Then a sequence x = (xk) of points in (X, g) is statistically convergent if and only if it is statistically Cauchy.
Proof. Suppose that g(st)-lim x = ξ. Then, we get
where A(ε): = {n ∈ ℕ: g(xn - ξ) ≥ ε/2}. This implies that
Let m ∈ AC(ε). Then g(xm - ξ) < ε/2. Now, let B(ε): = {n ∈ ℕ: g(xm - xn) ≥ ε}. We need to show that B(ε) ⊂ A(ε). Let n ∈ B(ε). Then g(xn - xm) ≥ ε and hence g(xn - ξ) ≥ ε/2, i.e. n ∈ A(ε). Otherwise, if g(xn - ξ) < ε then
which is not possible. Hence B(ε) ⊂ A(ε), which implies that x = (xk) is g(st)-convergent.
Conversely, suppose that x = (xk) is g(st)-Cauchy but not g(st)-convergent. Then there exists M ∈ ℕ such that δ(G(ε) = 0,
where G(ε): = {n ∈ ℕ: g(xn - xM) ≥ ε}, and δ(D(ε)) = 0, where D(ε): ={n ∈ ℕ: g(xn - ξ) < ε/2}, i.e., δ(DC(ε)) = 1. Since g(xn - xm) ≤ 2g(xn - ξ) < ε,
if g(xn - ξ) < ε/2. Therefore δ(GC(ε)) = 0, i.e., δ(G(ε) = 1, which leads to a contradiction, since x = (xk) was g(st)-Cauchy. Hence x = (xk) must be g(st)-convergent.
3 Strong summability
In this section, we define the notion of strong summability by a modulus function and establish its relation with statistical convergence in a paranormed space.
Definition 3.1. A sequence x = (xk) is said to be strongly p-Cesàro summable (0 < p < ∞) to the limit ξ in (X, g) if
and we write it as xk → ξ[C1, g]p. In this case ξ is called the [C1, g]p-limit of x.
Theorem 3.1. (a) If 0 < p < ∞ and xk → ξ[C1, g]p, then x = (xk) is statistically convergent to ξ in (X, g).
(b) If x = (xk) is bounded and statistically convergent to ξ in (X, g) then xk → ξ[C1, g]p.
Proof. (a) Let xk → ξ[C1, g]p, then
as n → ∞. That is,
and so δ(Kε) = 0, where Kε: = {k ≤ n: (g(xk - ξ))p ≥ ε} . Hence x = (xk) is statistically convergent to ξ in (X, g).
(b) Suppose that x = (xk) is bounded and statistically convergent to ξ in (X, g). Then for ε > 0, we have δ(Kε) = 0. Since x ∈ l∞, there exists M > 0 such that g(xk - ξ) ≤ M (k = 1, 2, ...). We have
where
Now if k ∉ Kε then S1(n) < εq. For k ∈ Kε, we have
as n → ∞, since δ(Kε) = 0. Hence xk → ξ[C1, g]p.
This completes the proof of the theorem.
Recall that a modulus f is a function from [0, ∞) to [0, ∞) such that (i) f(x) = 0 if and only if x = 0, (ii) f(x + y) ≤ f(x) + f(y) for all x, y ≥ 0, (iii) f is increasing, and (iv) f is continuous from the right at 0.
Now we define the following:
Definition 3.2. Let f be a modulus. we say that a sequence x = (xk) is strongly p-Cesàro summable with respect to f to the limit ξ in (X, g) if
(0 < p < ∞). In this case we write xk → ξ(w(f, g, p)).
As in [13], it is easy to prove the following:
Theorem 3.2. (a) Let f be any modulus and xk → ξ(w(f, g, p)). Then x = (xk) is statistically convergent to ξ in (X, g).
(b) Sg = w(f, g, p) If and only if f is bounded.
Competing interests
The authors declare that they have no competing interests.
Authors' contributions
The authors have equitably contributed in obtaining the new results presented in this article. All authors read and approved the final manuscript.
Acknowledgements
The authors would like to thank the Deanship of Scientific Research at King Abdulaziz University for its financial support under a grant with number 156/130/1431.
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