EUROPEAN JOURNAL OF PURE AND APPLIED MATHEMATICS Vol. 13, No. 2, 2020, 351-368 ISSN 1307-5543 – www.ejpam.com Published by New York Business Global Approximation of Function in generalized Hölder Class H. K. Nigam1, Supriya Rani1,∗ 1Department of Mathematics, Central University of South Bihar, Gaya-824236 (Bihar), India Abstract. In the present work, we study error estimation of a function g ∈ H(η) r (r ≥ 1) class using Matrix-Hausdorff (T∆H) means of its Fourier series. Our Theorem 1 generalizes twelve previously known results. Thus, the results of [4, 5, 11–16, 18, 26, 29, 30] become the particular cases of our Theorem 1. Several useful results in the form of corollaries are also deduced from our Theorem 1. 2020 Mathematics Subject Classifications: 41A10, 41A25, 42B05, 42A10, 40G05, 40C05 Key Words and Phrases: Error estimation, Generalized Hölder class, Fourier series, Matrix (T ) means, Hausdorff (∆H) means, Matrix-Hausdorff (T∆H) product means 1. Introduction In the past few decades, the researchers have been greatly interested in studying the error estimation of functions in different function spaces using summability operators due to their variety of applications in science and engineering. In this direction, several researchers like [2, 3, 9, 10, 19–23, 25, 28] have obtained results on error estimation of functions in different Lipschitz classes and Hölder classes with different single summability operators. Taking a view point that a product summability is more effective than the individual single summability operator, researchers like [11, 13, 18, 27–29], have obtained error estimation of functions in various Lipschitz and Hölder classes using different product summability operators. After reviewing the above mentioned works, we observe that these works cannot provide the best error estimation of a function in the function spaces considered in their works. This fact strongly motivates us to consider a more advanced class of function, which provide the best approximation of a function using summability operator. Therefore, in the present work, we establish a theorem on the best error approximation of a function g in the generalized Hölder class H (η) r (r ≥ 1) using Matrix-Hausdorff (T∆H) ∗Corresponding author. DOI: https://doi.org/10.29020/nybg.ejpam.v13i2.3667 Email addresses: hknigam@cusb.ac.in (H. K. Nigam), supriya@cusb.ac.in (Supriya Rani) http://www.ejpam.com 351 c© 2020 EJPAM All rights reserved. S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 352 product operator of its Fourier series. Our main theorem generalizes tweleve previously known results. Thus, the results of [4, 5, 11–16, 18, 26, 29, 30] become the particular cases of our theorem. 2. Preliminaries Let ∑∞ l=0 cl be an infinite series having lth partial sum sl = ∑l ν=0 cν . Let T ≡ (bl,j) be an infinite triangular matrix satisfying the conditions of regularity [24] i.e.  ∑l j=0 bl,j = 1 as l→∞; ∀ j ≥ 0, bl,j = 0 as l→∞; ∃ M > 0 ∀ l ≥ 0, ∑∞ j=0 |bl,j | < M. (1) The sequence-to-sequence transformation tTl := l∑ j=0 bl,jsj = l∑ j=0 bl,l−jsl−j defines the sequence tTl of triangular matrix means of the sequence {sl} generated by the sequence of coefficients (bl,j). If tTl → s as l→∞, then the infinite series ∑∞ l=0 cl or the sequence {sl} is summable to s by triangular matrix (T ) [1]. A Hausdorff matrix H ≡ (hl,j) is an infinite lower triangular matrix [8] defined by hl,j ≡  ( l j ) ∆l−jµj , 0 ≤ j ≤ l; 0, j > l, where the operator ∆ is defined ∆µj ≡ µj − µj+1 and ∆l+1µj ≡ ∆l(∆µj). If t∆H l = ∑l m=0 hl,msm → s as l→∞ then the series or the sequence {sl} is summable to the sum s by the Hausdorff method (∆H method). A Hausdorff matrix H is regular, i.e., H preserves the limit of each convergent sequence iff ∫ 1 0 |dξ(z)| <∞, where the mass function ξ ∈ BV [0, 1], ξ(0+) = ξ(0) = 0, and ξ(1) = 1. In this case, µl has the representation µl = ∫ 1 0 zldξ(z) [17]. S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 353 Superimposing T - method on ∆H method, (T∆H) is obtained. T∆H mean of the sequence {sl} is given by tT∆H l := l∑ j=0 bl,jt ∆H j = l∑ j=0 bl,j j∑ v=0 hj,vsv. If tT∆H l → s as l→∞, then {sl} is summable by the T∆H means to the limit s. Since T and ∆H method are regular, then T∆H method is also regular. This can be shown as sl → s ⇒ t∆H l → s, as l→∞, since the ∆H method is regular, ⇒ T (t∆H l ) = tT∆H l → s, as l→∞, since the T method is regular, ⇒ T∆H method is regular. Remark 1. T∆H means reduces to (i) (C,α)∆H or Cα∆H means when bl,j = (l−j+α−1 α−1 ) (l+αα ) for all α ≥ −1. (ii) ( H, 1 l+1 ) ∆H or H1/l+1∆H means if bl,j = 1 (l−j+1) log(l+1) . (iii) (N, pl, ql)∆H or Np,q∆H means if bl,j = pl−jqj Rl , Rl = ∑l j=0 pjql−j . (iv) (N, pl)∆H or Np∆H means if bl,j = pl−j Pl where Pl = ∑l j=0 pj , ql = 1. (v) (Ñ , pl)∆H or Ñp∆H means if bl,j = pj Pl , ql = 1 ∀ l. (vi) (E, ql)∆H or Eq∆H means if bl,j = 1 (1+q)l ( l j ) ql−j . (vii) T (C,α) or TCα means if ξ(z) = ∏α j=1 z j , α ≥ 1. (viii) T (E, ql) or TEq means if hl,j = ( l j ) ql−j (1+q)l , 0 ≤ j ≤ l. In above Remark 1 (iii), (iv) and (v), {pl} and {ql} are two non-negative monotonic non-decreasing sequence of real constants. Remark 2. (i) (C,α)∆H or Cα∆H means further reduces to S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 354 (a) (C,α)(C,α) or CαCα means if ξ(z) = ∏α j=1 z j , α ≥ 1. (b) (C,α)(E, ql) or CαEq means if hl,j = ( l j ) ql−j (1+q)l , 0 ≤ j ≤ l. (c) (C, 1)∆H or C1∆H means if α = 1. (ii) ( H, 1 l+1 ) ∆H or H1/l+1∆H means further reduces to (a) ( H, 1 l+1 ) (C,α) or H1/l+1Cα means if ξ(z) = ∏α j=1 z j , α ≥ 1. (b) ( H, 1 l+1 ) (E, ql) or H1/l+1Eq if hl,j = ( l j ) ql−j (1+q)l , 0 ≤ j ≤ l. (iii) (N, pl, ql)∆H or Np,q∆H means further reduces to (a) (N, pl, ql)(C,α) or Np,qCα means if ξ(z) = ∏α j=1 z j , α ≥ 1. (b) (N, pl, ql)(E, ql) or Np,qEq means if hl,j = ( l j ) ql−j (1+q)l , 0 ≤ j ≤ l. (iv) (N, pl)∆H or Np∆H means further reduces to (a) (N, pl)(C,α) or NpCα means if ξ(z) = ∏α j=1 z j , α ≥ 1. (b) (N, pl)(E, ql) or NpEq means if hl,j = ( l j ) ql−j (1+q)l , 0 ≤ j ≤ l. (v) (Ñ , pl)∆H or Ñp∆H means further reduces to (a) (Ñ , pl)(C,α) or ÑpCα means if ξ(z) = ∏α j=1 z j , α ≥ 1. (b) (Ñ , pl)(E, ql) or ÑpEq means if hl,j = ( l j ) ql−j (1+q)l , 0 ≤ j ≤ l. (vi) (E, ql)∆H or Eq∆H means further reduces to (a) (E, ql)(C,α) or EqCα means if ξ(z) = ∏α j=1 z j , α ≥ 1. (b) (E, ql)(E, ql) or EqEq means if hl,j = ( l j ) ql−j (1+q)l , 0 ≤ j ≤ l. (vii) T (C,α) or TCα means further reduces to (a) T (C, 1) or TC1 means if α = 1. (viii) T (E, ql) or TEq means further reduces to (a) T (E, 1) or TE1 means if ql = 1 ∀ l. Remark 3. (i) Above particular case (i)(b) in Remark 2 is further reduced to C1Eq, CαE1 and C1E1 means for α = 1, ql = 1 ∀ l and α = 1, ql = 1 ∀ l respectively. (ii) Above particular cases (ii)(a) and (b) in Remark 2 are further reduced to H1/l+1C1 and H1/l+1E1 means for α = 1 and ql = 1 ∀ l respectively. S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 355 (iii) Above particular cases (iii)(a) and (b) in Remark 2 are further reduced to (N, pl, ql)(C, 1) and (N, pl, ql)(E, 1) means for α = 1 and ql = 1 ∀ l respectively. (iv) Above particular cases (iv)(a) and (b) in Remark 2 are further reduced to (N, pl)(C, 1) and (N, pl)(E, 1) means for α = 1 and ql = 1 ∀ l respectively. (v) Above particular cases (v)(a) and (b) in Remark 2 are further reduced to (Ñ , pl)(C, 1) and (Ñ , pl)(E, 1) means for α = 1 and ql = 1 ∀ l respectively. (vi) Above particular cases (vi)(a) in Remark 2 is further reduced to EqC1, E1Cα and E1C1 means for α = 1, ql = 1 ∀ l and ql = 1 ∀ l, α = 1 respectively. The space of the functions Lr is given by Lr[0, 2π] = { g : [0, 2π] 7→ R : ∫ 2π 0 |g(x)|rdx <∞, r ≥ 1 } . The norm ‖ · ‖(r) by { 1 2π ∫ 2π 0 |g(x)|rdx }1/r , r ≥ 1. As defined in [1], η : [0, 2π] 7→ R is an arbitrary function with η(s) > 0 for 0 < s ≤ 2π and lims→0+ η(s) = η(0) = 0. Now, we define H(η) r := { g ∈ Lr[0, 2π] : sup s 6=0 ‖g(·,+s)− g(·)‖r η(s) <∞, r ≥ 1 } and ‖ · ‖(η) r = ‖g‖(η) r = ‖g‖r + sup s 6=0 ‖g(·,+s)− g(·)‖r η(s) ; r ≥ 1. Clearly, ‖ · ‖(η) r is a norm on H (η) r . Note 1. η(s) and χ(s) denote moduli of continuity of order two such that η(s) χ(s) is positive, non-decreasing and ‖g‖(χ) r ≤ max ( 1, η(2π) χ(2π) ) ‖g‖(η) r <∞. Thus, H(η) r ⊂ H(χ) r ⊂ Lr; r ≥ 1 [1]. Remark 4. (i) If η(s) = sα in H(η), H(η) implies H(α) class. (ii) If η(s) = sα in H (η) r , H(η) implies Hα,r class. S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 356 (iii) If r →∞ in H (η) r , H (η) r implies H(η) class and Hα,r implies Hα class. We denote the lth partial sum of the Fourier series as sl(g;x)− g(x) = 1 2π ∫ π 0 φ(x, s) sin ( l + 1 2 ) s sin s 2 ds [1]. The l-order error estimation of function g is given by El(g) = min ‖g − tl‖r, where tl is a trigonometric polynomial of degree l [1]. If El(g)→ 0 as l→∞, then El(g) is said to be the best approximation of g [1]. We write φ(x, s) = g(x+ s) + g(x− s)− 2g(x); ∆bl,j = bl,j − bl,j+1; KT∆H l (s) = 1 2π l∑ j=0 bl,j j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) sin ( a+ 1 2 ) s sin s 2 . 3. Main Theorem Theorem 1. If g ∈ H(η) r class, r ≥ 1, then the error estimation of g using T∆H product means of its Fourier series is given by ‖tT∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) , where T ≡ (bl,j) is an infinite triangular matrix satisfying (1) and η, χ are as defined in Note 1, provided l−1∑ j=0 |∆bl,j | = O ( 1 l + 1 ) (2) and (l + 1)bl,l = O(1). (3) 4. Lemmas Lemma 1. Under the conditions of regularity of matrix T ≡ (bl,j), KT∆H l (s) = O(l + 1) for 0 < s < 1 l + 1 . S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 357 Proof. For 0 ≤ s ≤ 1 l+1 , sin s 2 ≥ s π , sin ls ≤ ls, we have KT∆H l (s) = 1 2π l∑ j=0 bl,j j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) sin ( a+ 1 2 ) s 2 sin s 2 = 1 2π l∑ j=0 bl,j j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) (2a+ 1) s2 s π = 1 4 l∑ j=0 bl,j { j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z)(2a+ 1) } = 1 4 l∑ j=0 bl,j [ 2 j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a a dξ(z) ] + 1 4 l∑ j=0 bl,j [ j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) ] . (4) First, we solve 2 j∑ a=0 ( j a ) za(1− z)j−aa = 2(1− z)j j∑ a=0 ( j a )( z 1− z )a a = 2(1− z)j j∑ a=0 ( j a ) daa, (5) where z 1− z = d. Now, j∑ a=0 ( j a ) daa = ( j 0 ) d00 + ( j 1 ) d11 + ( j 2 ) d22 + · · ·+ ( j j ) djj = ( j 1 ) d+ 2 ( j 2 ) d2 + 3 ( j 3 ) d3 · · ·+ j ( j j ) dj . (6) We observe that (1 + d)j = ( j 0 ) 1j−0 · d0 + ( j 1 ) 1j−1 · d1 + ( j 2 ) 1j−2 · d2 + · · ·+ ( j j ) 1j−j · dj (1 + d)j = ( j 0 ) + ( j 1 ) d+ ( j 2 ) d2 + · · ·+ ( j j ) dj j(1 + d)j−1 = 0 + ( j 1 ) + 2 ( j 2 ) d+ 3 ( j 3 ) d2 + · · ·+ j ( j j ) dj−1 (by differentiating w.r.t d) S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 358 jd(1 + d)j−1 = ( j 1 ) d+ 2 ( j 2 ) d2 + 3 ( j 3 ) d3 + · · ·+ j ( j j ) dj (7) (multiplying both side by d). Now, from (6) and (7), we get j∑ a=0 ( j a ) daa = jd(1 + d)j−1 = j ( z 1− z )( 1 (1− z)j−1 ) = jz (1− z)j . (8) Thus, from (5) and (8), we get 2 j∑ a=0 ( j a ) za(1− z)j−aa = 2(1− z)j j∑ a=0 ( j a ) daa = 2(1− z)j jz (1− z)j = 2jz. (9) Now, j∑ a=0 ( j a ) za(1− z)j−a = ( j 0 ) z0(1− z)j + ( j 1 ) z1(1− z)j−1 + · · ·+ ( j j ) zj(1− z)j−j = (1− z + z)j = 1. (10) Thus, from (4), (9) and (10), we get KT∆H l (s) = 1 4 l∑ j=0 bl,j [ j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a(2a+ 1) dξ(z) ] = 1 4 l∑ j=0 bl,j ∫ 1 0 (2jz + 1) dz = 1 4 l∑ j=0 bl,j(j + 1). = O(l + 1) l∑ j=0 bl,j = O(l + 1). S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 359 Lemma 2. Under the conditions of regularity of matrix T ≡ (bl,j), KT∆H l (s) = O ( 1 s2(l + 1) ) for 1 l + 1 ≤ s ≤ π. Proof. For 1 l+1 ≤ s ≤ π, sin s 2 ≥ s π , sin2 ls ≤ 1 and sup0≤z≤1 |ξ′(z)| = N , we have KT∆H l (s) = 1 π l∑ j=0 bl,j j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) sin ( a+ 1 2 ) s 2 sin s 2 = 1 2π l∑ j=0 bl,j j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) sin ( a+ 1 2 ) s s π = 1 2s n∑ j=0 bl,j j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) sin ( a+ 1 2 ) s ≤ N 2s ∣∣∣∣ l∑ j=0 bl,jIm j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−aei(a+ 1 2)s dξ(z) ∣∣∣∣. (11) Now, first we solve j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a sin ( a+ 1 2 ) s dξ(z) = (1− z)j j∑ a=0 ∫ 1 0 ( j a )( z 1− z )a Im { ei(a+ 1 2)s } dξ(z) = (1− z)j j∑ a=0 ∫ 1 0 ( j a )( z 1− z )a Im { eias · e is 2 } dξ(z) = (1− z)jIm [ e is 2 j∑ a=0 ∫ 1 0 ( j a )( zeis 1− z )a dξ(z) ] = Im [ e is 2 ∫ 1 0 (1− z + zeis)jdz ] = Im [ e is 2 ∫ 1 0 { 1 + z(eis − 1) }j dz ] = Im [ ei(j+1)s − 1 (1 + j)(e is 2 − e −is 2 ) ] = Im [ ei(j+1)s − 1 (j + 1)2i sin s 2 ] = Im [ cos(j + 1)s+ i sin(j + 1)s− 1 2i(j + 1) sin s 2 ] = sin2(j + 1) s2 (j + 1) sin s 2 . (12) S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 360 Now, from (11) and (12), we get KT∆H l (s) ≤ N 2s ∣∣∣∣ l∑ j=0 bl,j sin2(j + 1) s2 (j + 1) sin s 2 ∣∣∣∣ ≤ N 2s ∣∣∣∣ l∑ j=0 bl,j 1 (j + 1) sπ ∣∣∣∣ = Nπ 2s2 ∣∣∣∣ l∑ j=0 bl,j 1 j + 1 ∣∣∣∣ Using Abel’s Lemma, we have KT∆H l (s) = Nπ 2s2 ∣∣∣∣ l−1∑ j=0 (bl,j − bl,j+1) j∑ k=0 1 k + 1 + bl,l l∑ j=0 1 j + 1 ∣∣∣∣ ≤ Nπ 2s2 ∣∣∣∣ l−1∑ j=0 ∆bl,j j∑ k=0 1 k + 1 ∣∣∣∣+ bl,l ∣∣∣∣ l∑ j=0 1 j + 1 ∣∣∣∣ ≤ Nπ 2s2  l−1∑ j=0 |∆bl,j |+ bl,l  max 0≤j≤p ∣∣∣∣ p∑ j=0 1 j + 1 ∣∣∣∣ = Nπ 2s2 [ O ( 1 l + 1 ) + O ( 1 l + 1 )] = O ( 1 s2(l + 1) ) . Lemma 3. [28] Let g ∈ H(η) r , then for 0 < s ≤ π : (i) ‖φ(·, s)‖r = O(η(s)); (ii) ‖φ(·+ z, s)− φ(·, s)‖r = { O(η(s)) O(η(z)). (iii) If η(s) and χ(s) are as defined in Note 1, then ‖φ(·+z, s)−φ(·, s)‖r = O ( χ(|z|) ( η(s) χ(s) )) . 5. Proof of the main theorem 5.1. Proof of Theorem 1 Proof. Following [7], sl(g;x) of Fourier series sl(g;x)− g(x) = 1 2π ∫ π 0 φ(x, s) sin ( l + 1 2 ) s sin s 2 ds. S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 361 The Hausdorff matrix mean of sl(x), denoted by t∆H l (x), we get t∆H l (x)− g(x) = l∑ j=0 hl,j(sj(x)− g(x)) = l∑ j=0 ( l j ) ∆l−jµj { 1 2π ∫ π 0 φ(x, s) sin ( j + 1 2 ) s sin s 2 ds } = 1 2π ∫ π 0 φ(x, s) l∑ j=0 ( l j ) ∆l−j (∫ 1 0 zj dξ(z) ) sin ( j + 1 2 ) s sin s 2 ds = 1 2π ∫ π 0 φ(x, s) l∑ j=0 ∫ 1 0 ( l j ) zj(1− z)l−j dξ(z) sin ( j + 1 2 ) s sin s 2 ds. The T transform of t∆H l (x) denoted by tT∆H l (x), is given by tT∆H l (x)− g(x) = l∑ j=0 bl,j ( 1 2π ∫ π 0 φ(x, s) j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) sin ( a+ 1 2 ) s sin s 2 ds ) = 1 2π ∫ π 0 φ(x, s) l∑ j=0 bl,j j∑ a=0 ∫ 1 0 ( j a ) za(1− z)j−a dξ(z) sin ( a+ 1 2 ) s sin s 2 ds = ∫ π 0 φ(x, s)KT∆H l (s) ds. Let Tl(x) = tT∆H l (x)− g(x) = ∫ π 0 φ(x, s)KT∆H l (s) ds. Then Tl(x+ z)− Tl(x) = ∫ π 0 (φ(x+ z, s)− φ(x, s))KT∆H l (s) ds. Using generalized Minkowski’s inequality [6], we obtain ‖Tl(·,+z)− Tl(·)‖r ≤ ∫ π 0 ‖φ(·+ z, s)− φ(·, s)‖rKT∆H l (s) ds = ∫ 1 l+1 0 ‖φ(·+ z, s)− φ(·, s)‖rKT∆H l (s) ds + ∫ π 1 l+1 ‖φ(·+ z, s)− φ(·, s)‖rKT∆H l (s) ds = I1 + I2. (13) Using Lemmas 1 and 3 (iii), we get I1 = ∫ 1 l+1 0 ‖φ(·+ z, s)− φ(·, s)‖rKT∆H l (s) ds S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 362 = O(l + 1) ( χ(|z|) ∫ 1 l+1 0 η(s) χ(s) ds ) = ( χ(|z|) η( 1 l+1) χ( 1 l+1) ) . (14) Also, using Lemmas 2 and 3 (iii), we get I2 = ∫ π 1 l+1 ‖φ(·+ z, s)− φ(·, s)‖rKT∆H l (s) ds = O ( 1 l + 1 ∫ π 1 l+1 χ(|z|) η(s) s2χ(s) ds ) . (15) From (13), (14) and (15), we have sup z 6=0 ‖Tl(·,+z)− Tl(·)‖r χ(|z|) = O  η ( 1 l+1 ) χ ( 1 l+1 ) + O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . (16) Again applying Minkowski’s inequality and using Lemmas 1, 2 and 3 (i), we obtain ‖Tl(·)‖r = ‖tT∆H l − g‖r ≤ (∫ 1 l+1 0 + ∫ π 1 l+1 ) ‖φ(·, s)‖rKT∆H l (s) ds = O ( (l + 1) ∫ 1 l+1 0 η(s) ds ) + O ( 1 l + 1 ∫ π 1 l+1 η(s) s2 ds ) = O ( η ( 1 l + 1 )) + O ( 1 l + 1 ∫ π 1 l+1 η(s) s2 ds ) . (17) We know that ‖Tl(·)‖(χ) r = ‖Tl(·)‖r + sup z 6=0 ‖Tl(·,+z)− Tl(·)‖r χ(|z|) . (18) Now, using (16), (17) and (18), we get ‖Tl(·)‖(χ) r = O ( η ( 1 l + 1 )) + O ( 1 l + 1 ∫ π 1 l+1 η(s) s2 ds ) + O  η ( 1 l+1 ) χ ( 1 l+1 ) + O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . (19) S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 363 By the monotonicity of χ(s), η(s) = η(s) χ(s)χ(s) ≤ χ(π) η(s) χ(s) for 0 < s ≤ π, we get ‖Tl(·)‖(χ) r = O  η ( 1 l+1 ) χ ( 1 l+1 ) + O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . (20) Since η and χ are as defined in Note 1, therefore 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ≥ η ( 1 l+1 ) χ ( 1 l+1 ) ( 1 l + 1 )∫ π 1 l+1 1 s2 ds ≥ η ( 1 l+1 ) 2χ ( 1 l+1 ) . Then, η ( 1 l+1 ) χ ( 1 l+1 ) = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . (21) From (20) and (21), we get ‖Tl(·)‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) , ‖tT∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . (22) 6. Corollaries Corollary 1. Let g ∈ H(α),r; r ≥ 1 and 0 ≤ β < α ≤ 1, then ‖tT∆H l − g‖(β),r = { O((l + 1)β−α) if 0 ≤ β < α < 1 O ( log π(l+1) l+1 ) if β = 0, α = 1. Proof. The proof is obtained by putting η(s) = sα, χ(s) = sβ, 0 ≤ β < α ≤ 1 in Theorem 1. Corollary 2. Following the Remark 1(i), we obtain ‖tCα∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . Corollary 3. Following the Remark 1(ii), we obtain ‖tH1/l+1∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 364 Corollary 4. Following the Remark 1(iii), we obtain ‖tNp,q∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . Corollary 5. Following the Remark 1(iv), we obtain ‖tNp∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . Corollary 6. Following the Remark 1(v), we obtain ‖tÑp∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . Corollary 7. Following the Remark 1(vi), we obtain ‖tEq∆H l − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . Corollary 8. Following the Remark 1(vii), we obtain ‖tTCαl − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . Corollary 9. Following the Remark 1(viii), we obtain ‖tTEql − g‖(χ) r = O ( 1 l + 1 ∫ π 1 l+1 η(s) s2χ(s) ds ) . Remark 5. (i) Corollary 2 can be further reduced for CαEq and C1∆H means in view of Remark 2 (i)(b) and (c) respectively. (ii) Corollary 3 can be further reduced for H1/l+1Cα and H1/l+1Eq means in view of Remark 2 (ii)(a) and (b) respectively. (iii) Corollary 4 can be further reduced for Np,qCα and Np,qEq in view of Remark 2 (iii)(a) and (b) respectively. (iv) Corollary 5 can be further reduced for NpCα and NpEq means in view of Remark 2 (iv)(a) and (b) respectively. (v) Corollary 6 can be further reduced for ÑpCα and ÑpEq means in view of Remark 2 (v)(a) and (b) respectively. S. Rani, H. K. Nigam / Eur. J. Pure Appl. Math, 13 (2) (2020), 351-368 365 (vi) Corollary 7 can be further reduced for EqCα means in view of Remark 2 (vi)(a). (vii) Corollaries 8 can be further reduced for TC1 means in view of Remark 2 (vii)(a). (viii) Corollaries 9 can be further reduced for TE1 means in view of Remark 2 (viii)(a). Remark 6. (i) In our Theorem 1, if r →∞ in H (η) r class, then this turns down to H(η) class. Also putting η(s) = sα and χ(s) = sβ in our Theorem 1, H(η) class then this turns down to Hα class. Then for β = 0 in Hα class, this turns down to Lipα class. (ii) In our Theorem 1, by putting η(s) = sα, χ(s) = sβ in H (η) r class, H (η) r class then this turns down to Hα,r class. Then for β = 0 in Hα,r class, this turns down to Lip(α, r) class. Remark 7. (i) If ζ(s) = sα and r →∞ then Lip(ζ(s), r) class turns down to Lipα class. Thus, the results of [12], [15], [16] and [30] reduces to Lipα class. (ii) If β = 0, ζ(s) = sα and r → ∞ then W (Lr, ζ(s)) class turns down to Lipα class. Thus, the results of [11], [13] and [14] reduces to Lipα class. 7. Particular cases (i) Using Remark 6(i) and putting hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, the result of Dhakal [4] follows. (ii) Using Remark 6(i) , putting bl,j = pl−jqj Rl , Rl = ∑l j=0 pjql−j and hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, the result of Dhakal [5] follows. (iii) Using Remark 6(i), putting bl,j = 1 2l ( l j ) and hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, then in view of Remark 7(ii), the result of Nigam [11] follows. (iv) Using Remark 6(i), putting ξ(z) = ∏α j=1 z j , α ≥ 1 and hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, then in view of Remark 7(i), the result of Nigam [12] follows. (v) Using Remark 6(i), putting bl,j = 1 l+1 and hl,j = 1 (1+q)l ( l j ) ql−j in our Theorem 1, in view of Remark 7(ii), the result of Nigam [13] follows. (vi) Using Remark 6(i) and 6(ii), putting bl,j = pl−j Pj , ∑l j=0 pj 6= 0, ql = 1 ∀ l and hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1 then in view of Remark 7(ii), the result of Nigam and Sharma [14] follows. REFERENCES 366 (vii) Using Remark 6(i), putting bl,j = 1 l+1 and hl,j = 1 (1+q)l ( l j ) ql−j in our Theorem 1, then in view of Remark 7(i), the result of Nigam and Sharma [15] follows. (viii) Using Remark 6(i), putting bl,j = 1 2l ( l j ) and hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, then in view of Remark 7(i), the result of Nigam and Sharma [16] follows. (ix) Using Remark 6(ii), putting bl,j = pl−jqj Rl , Rl = ∑l j=0 pjql−j and hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, the result of Kushwaha and Dhakal [18] follows. (x) Using Remark 6(i), putting ξ(z) = ∏α j=1 z j , α ≥ 1 and hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, the result of Tiwari and Bariwal [26] follows. (xi) Using Remark 6(i), putting bl,j = 1 l+1 and hl,j = 1 (1+q)l ( l j ) ql−j in our Theorem 1, the result of Lal [29] follows. (xii) Using Remark 6(i), putting hl,j = 1 l+1 , 0 ≤ j ≤ l in our Theorem 1, then in view of Remark 7(i), the result of Shrivastava, Rathore and Shukla [30] follows. 8. Conclusion In this paper, we obtain the error estimation of the function g in the Hölder space H (η) r (r ≥ 1) by Matrix-Hausdorff (T∆H) product means of its Fourier series. Since, in view of Remark 1, the product summability means Cα∆H , H1/l+1∆H , Np,q∆H , Np∆H , Ñp∆H , Eq∆H , TCα and TEq are the particular cases of T∆H product means. Some useful results are also deduced in the form of corollaries from our theorem. 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