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Research article Topical Sections

Exploring quaternionic Bertrand curves: involutes and evolutes in E4

  • Received: 26 December 2024 Revised: 14 February 2025 Accepted: 26 February 2025 Published: 03 March 2025
  • MSC : 11R52, 53A04

  • This study investigated the concepts of (0, 2)-involute and (1, 3)-evolute curves associated with quaternionic Bertrand curves within the context of four-dimensional Euclidean space. Using a type-2 quaternionic frame, we derived mathematical expressions that define these interacting and evolute curves. The (0, 2)-involute curve is characterized by tangents orthogonal to points on the original quaternionic Bertrand curve, while the (1, 3)-evolute curve is constructed using specific normal vectors related to curvature properties. We presented a comprehensive framework that clarifies the interrelationships between the curvature functions of involute and evolute pairs and their connections to the Frenet frame. This framework provides a geometric basis for analyzing curves in higher-dimensional spaces. The findings enhance the understanding of quaternionic curves and their geometric properties, contributing to the broader field of differential geometry.

    Citation: Ayman Elsharkawy, Ahmer Ali, Muhammad Hanif, Fatimah Alghamdi. Exploring quaternionic Bertrand curves: involutes and evolutes in E4[J]. AIMS Mathematics, 2025, 10(3): 4598-4619. doi: 10.3934/math.2025213

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  • This study investigated the concepts of (0, 2)-involute and (1, 3)-evolute curves associated with quaternionic Bertrand curves within the context of four-dimensional Euclidean space. Using a type-2 quaternionic frame, we derived mathematical expressions that define these interacting and evolute curves. The (0, 2)-involute curve is characterized by tangents orthogonal to points on the original quaternionic Bertrand curve, while the (1, 3)-evolute curve is constructed using specific normal vectors related to curvature properties. We presented a comprehensive framework that clarifies the interrelationships between the curvature functions of involute and evolute pairs and their connections to the Frenet frame. This framework provides a geometric basis for analyzing curves in higher-dimensional spaces. The findings enhance the understanding of quaternionic curves and their geometric properties, contributing to the broader field of differential geometry.



    Let N be the set of natural numbers with N0=N{0}. For nN0, the following harmonic-like numbers are given by partial sums:

    ● The classical harmonic number and its quadratic counterpart

    Hn=n1k=01k+1andH2n=n1k=01(k+1)2.

    ● Skew harmonic number and its quadratic counterpart

    On=n1k=012k+1andO2n=n1k=01(2k+1)2.

    ● Alternating harmonic number and its quadratic counterpart

    ˉHn=n1k=0(1)kk+1andˉH2n=n1k=0(1)k(k+1)2.

    Among them, there are the following simple but useful relations:

    H2n=On+Hn2,H22n=O2n+H2n4;ˉH2n=OnHn2,ˉH22n=O2nH2n4.

    Harmonic numbers and their variants have been studied since the distant past and are involved in diverse fields (cf. [1,5,6,7,11,17,18]) such as analysis of algorithms in computer science, various topics of number theory, and combinatorial analysis. In this paper, we aim at presenting several algebraic identities about infinite series involving harmonic-like numbers, the binomial coefficient (3nn) in numerators, and a free variable "y".

    For nN0 and an indeterminate x, the shifted factorials (cf. [3, §1.1])) are usually defined by

    (x)0=1and(x)n=x(x+1)(x+n1)fornN.

    Denote by [xm]ϕ(x) the coefficient of xm in the formal power series ϕ(x). Then we can express harmonic-like numbers (see [11,18]) by extracting the initial coefficients of x from the quotients of shifted factorials as below:

    [x](1+x)nn!=Hn,[x2](1+x)nn!=H2nH2n2,[x]n!(1x)n=Hn,[x2]n!(1x)n=H2n+H2n2,[y](12+y)n(12)n=2On,[y2](12+y)n(12)n=2(O2nO2n),[y](12)n(12y)n=2On,[y2](12)n(12y)n=2(O2n+O2n).

    There exist many infinite series identities involving central binomial coefficients (see [12,14,19,25]). However, the closed form evaluations for the known series with (3nn) are rare. In a recent paper, Sun [23] reported several remarkable infinite series identities, detected by numerical experimentation. Among them, the following three (see [23, Eqs (2.12), (2.13), and (2.15)]) seem rather challenging:

    n=1(227)n(3nn)H2n=1+32{3ln23ln(33)}, (1.1)
    n=1(227)n(3nn)H3n=1+34ln(4(7+43)3)3ln2, (1.2)
    n=1(3+554)n(3nn){H3nH2n}=1+52ln(9352). (1.3)

    When making efforts to confirm these three formulae, two substantial novelties emerged. First, not only the harmonic numbers H3n and H2n are separable in the third series, but also independent series involving Hn and On can be evaluated explicitly in closed form (cf. Corollaries 6 and 10). Another surprising novelty (see Theorems 1 and 5) lies in the fact that these series are particular cases of more general algebraic identities containing a free variable "y", corresponding to the convergent rates of these numerical series. To our knowledge, most of the infinite series identities presented in this paper have not appeared previously in the literature.

    The rest of the paper is organized as follows. As preliminaries, we shall evaluate, in closed form, three series containing binomial coefficient (3nn), harmonic number Hn and a free variable "y" by integrating Lambert's series. Then in Sections 3–5, three classes of infinite series with harmonic-like numbers will be examined by applying the "coefficient extraction" method (see [8,13,24]) to cubic transformations for the 3F2-series, that result in several algebraic identities about these series and confirm or refine, as special numerical examples, three conjectured identities made recently by Sun [23]. Finally, the paper will end with Section 6, where concluding remarks and further problems are provided.

    In classical analysis and enumerative combinatorics, Lambert's binomial series are well-known (see Riordan [22, §4.5] and [9,10,16]), which can be reproduced as follows: Let T and τ be the two variables related by the equation τ=T/(1+T)β. Then

    (1+T)α=k=0αα+kβ(α+kβk)τkand(1+T)α+11+TTβ=k=0(α+kβk)τk. (2.1)

    As preliminaries, we are going to evaluate, in closed form, three series containing ternary coefficient (3nn) and a free variable "y" by integrating across the above two equations, that will be crucial for demonstrating infinite series identities involving harmonic numbers in the subsequent sections.

    For "α=0 and β=3", performing the replacement τxy/(1+y)3 in Lambert's second series, we can state the resulting equality as

    ϕ(T):=1+T12T=n=0(3nn)(xy)n(1+y)3n:x=T(1+y)3y(1+T)3. (2.2)

    Since the rightmost function is monotone around T=0, it determines an implicit inverse function T=T(x) in the neighborhood of x=0 with particular values "T(0)=0 and T(1)=y".

    By expressing the harmonic number Hn in terms of the integral

    Hn=101xn1xdx,

    we can insert Hn in the series (2.2) as follows:

    n=0(3nn)Hnyn(1+y)3n=10ϕ(T(1))ϕ(T(x))1xdx=(1+y)3yy012T(1+T)41+y12y1+T12T1T(1+y)3y(1+T)3dT=(1+y)3y01(12T)(1+y)(1+T)(12y)T(1+y)3y(1+T)3dT,

    where the change of variable x=T(1+y)3y(1+T)3 has been made so that the integral becomes explicit.

    For the sake of brevity, the notation "ρ" will be fixed, throughout the paper, for the algebraic number

    ρ:=32(2+1)1/332(21)1/310.105892543. (2.3)

    The convergence region of the preceding series is determined by

    1<27y4(1+y)3<1,ρ<y<12.

    This can be illustrated graphically as below:

    Figure 1.  Range of convergence.

    By decomposing the integrand into partial fractions

    1(12T)(1+y)(1+T)(12y)T(1+y)3y(1+T)3=3(1+T)(1+y)2(12y)32(1+y)2(12y)4+y×{4+y+yT+y(3+y)(1+y)4+y2y+4+yyT+y(3+y)+(1+y)4+y2y},

    we can explicitly compute the integral

    y01(12T)(1+y)(1+T)(12y)T(1+y)3y(1+T)3dT=3ln(1+y)(1+y)2(12y)+3(y4+y)2(1+y)2(12y)4+yln((1+y)(22yy2+yy2+4y)2)3(y+4+y)2(1+y)2(12y)4+yln((1+y)(22yy2yy2+4y)2).

    By cancelling the three terms containing ln(1+y) and then making substitution, we find the closed formula for the series as in the theorem below:

    Theorem 1 (ρ<y<1/2).

    n=1(3nn)Hnyn(1+y)3n=(1+y)3y01(12T)(1+y)(1+T)(12y)T(1+y)3y(1+T)3dT=3(1+y)ln(12y)2(2y1)+3(1+y)y2(12y)4+yln(2y(2+yy2+4y)2y(2+y+y2+4y)).

    For "α=1 and β=3", performing the replacement τxy/(1+y)3, we can rewrite Lambert's first series as

    ψ(T):=1+T=n=0(3nn)(xy)n(1+2n)(1+y)3n:x=T(1+y)3y(1+T)3. (2.4)

    Analogously, by putting the harmonic number Hn inside the series (2.4), we have

    n=0(3nn)Hnyn(1+2n)(1+y)3n=10ψ(T(1))ψ(T(x))1xdxx=T(1+y)3y(1+T)3=(1+y)3yy0(yT)(12T)dT(1+T)4{1T(1+y)3y(1+T)3}=y0(1+y)3(Ty)(12T)dT(1+T){T(1+y)3y(1+T)3}=y0(1+y)3(12T)dT(1+T)(1T2yTy23Ty).

    By decomposing the integrand into partial fractions

    (1+y)3(12T)dT(1+T)(1T2yTy23Ty)=31+y1+T(1+y)(3y+4+y)2y(T+(3+y)y+(1+y)4+y2y)(1+y)(3y4+y)2y(T+(3+y)y(1+y)4+y2y),

    we can explicitly compute the integral

    y0(1+y)3(12T)dT(1+T)(1T2yTy23Ty)=3(1+y)ln(1+y)(1+y)(3y+4+y)2yln((1+y)(3y+4+y)(3+y)y+(1+y)4+y)(1+y)(3y4+y)2yln((1+y)(3y4+y)(3+y)y(1+y)4+y),

    which is simplified into the closed formula as in the theorem below:

    Theorem 2 (ρ<y<1/2).

    n=1(3nn)Hnyn(1+2n)(1+y)3n=y0(1+y)3(12T)dT(1+T)(1T2yTy23Ty)=(1+y)4+y2yln(2y(2+y+y2+4y)2y(2+yy2+4y))32(1+y)ln(12y).

    Alternatively, rewriting Lambert's first series

    (1+T)α1α=n=11α+nβ(α+nβn)τn:τ=T/(1+T)β

    and letting "α0 and β=3", we deduce the identity

    σ(T):=3ln(1+T)=n=1(3nn)(xy)nn(1+y)3n:x=T(1+y)3y(1+T)3. (2.5)

    By inserting Hn in the above series, we obtain an integral expression

    n=1(3nn)Hn(xy)nn(1+y)3n=10σ(T(1))σ(T(x))1xdxxT(1+y)3y(1+T)3=3y0ln(1+T1+y)(12T)(1+y)3(1+T)(Ty)(1T2yTy23Ty)dT=3y0ln(1+T1+y){1Ty31+T+y2+3y+2TyT2y+Ty2+3Ty1}dT.

    In view of the partial fraction decomposition

    y2+3y+2TyT2y+Ty2+3Ty1=1T+y(3+y)+(1+y)4+y2y)+1T+y(3+y)(1+y)4+y2y),

    it suffices to evaluate, for a parameter λ subject to T+λ0 for T(0,y), the parametric integral

    J(λ,y)=y0ln(1+T1+y)dTT+λ=Li2(1+y1λ)Li2(11λ)+ln(λλ1)ln(1+y),

    with particular cases

    J(1,y)=12ln2(1+y)andJ(y,y)=π26+ln(1+y)ln(y1+y)Li2(11+y).

    Hereafter, the dilogarithm function (see Lewin [20, §1.1]) is defined for all complex values of z by

    Li2(z)=z0ln(1τ)τandLi2(z)=n=1znn2for|z|1.

    By making substitution and then simplifying the terms concerning logarithms and dilogarithms in the resulting expression, we find the explicit formula as in the following theorem:

    Theorem 3 (ρ<y<1/2).

    n=1(3nn)Hnynn(1+y)3n=y03dT1+Tln(1T(1+y)3y(1+T)3)=π22+3Θ(y)+3ln(1+y)ln(y(1+y)3),

    where, for simplicity, Θ(y) denotes the sum of five dilogarithmic values

    Θ(y)=Li2(yy2+4y2)+Li2(y+y2+4y2)Li2(yy2+4y2+2y)Li2(y+y2+4y2+2y)Li2(11+y).

    According to Bailey [3], the classical hypergeometric series reads as

    1+pFp[a0,a1,a2,,apb1,b2,,bp|z]=k=0zkk!(a0)k(a1)k(a2)k(ap)k(b1)k(b2)k(bp)k.

    We shall confine ourselves only to examining the series with |z|<1 and none of the parameters in the numerator and denominator being a non-positive integer, which imply that the corresponding series is well-defined and convergent.

    There are many transformation and summation formulae for hypergeometric series (see Bailey [3] and Brychkov [4, Chapter 8]) in the literature. In 1928, Bailey [2] discovered an important cubic transformation (see the next section). Half a century later, Gessel and Stanton [15, Eq (5.4)] found the following counterpart

    3F2[1+a3,2+a3,3+a31+a+c2,2+ac2|27y4(1+y)3]=(1+y)1+a12y×4F3[1+a3,a,c,1ca3,1+a+c2,2+ac2|y4]. (3.1)

    Under the parameter replacements "a6ax,c2cx", this transformation can be reformulated as

    n=0(y4(1+y)3)n(1+6ax)3nn!(1+3axcx)n(12+3ax+cx)n=(1+y)1+6ax12y{1+6cxk=1(y4)k(k+2ax)(1+6ax)k1(1+2cx)k1(12cx)kk!(1+3axcx)k(12+3ax+cx)k}, (3.2)

    where "y(ρ,12)", or equivalently, 27y4(1+y)3(1,1) so that the series are convergent.

    The above transformation is an analytic equality with respect to x in the neighborhood of x=0. Equating the constant terms on both sides yields the algebraic identity below:

    n=0(3nn)yn(1+y)3n=1+y12y.

    As illustrated in the introduction, harmonic-like numbers can be expressed in terms of x-coefficients from quotients of shifted factorials. By examining the coefficients of x across the above equation, we find that the corresponding equation involving harmonic numbers can be written as

    n=1yn(1+y)3n(3nn){6aH3n(3ac)Hn2(3a+c)On}=6a1+y12yln(1+y)+6c1+y12yk=1(k1)!(12)k(y4)k.

    The rightmost series admits the closed form expression, as in the lemma below:

    Lemma 4 (4<y<4).

    W(y)=k=1(k1)!(12)k(y4)k=4y4+yArcTanhy4+y=4y4+yln4+yy2.

    Proof. Recall the beta function (see [21, §16])

    B(a,b)=10xa1(1x)b1dx=Γ(a)Γ(b)Γ(a+b),where(a)>0and(b)>0.

    We can express W(y) as a definite integral

    W(y)=k=1(k1)!(12)k(y4)k=k=1B(k,12)(y4)k=k=1(y4)k10xk1dx1x=10dxx1xk=1(xy4)k=10ydx1x(4+xy)=102y4+yT2ydT,

    where the last line is justified by the change of variable 1xT. Then the formula in the lemma follows by evaluating the last integral explicitly.

    Therefore, we find the general formula below:

    n=1yn(1+y)3n(3nn){6aH3n(3ac)Hn2(3a+c)On}=6a1+y12yln(1+y)+6c1+y12yW(y).

    By specifying two parameters, a and c, we deduce four independent series

    a=0:n=1yn(1+y)3n(3nn)ˉH2n=31+y12yW(y),c=0:n=1yn(1+y)3n(3nn){H3nH2n}=1+y12yln(1+y),c=3a:n=1yn(1+y)3n(3nn){H3n2On}=1+y12yln(1+y)31+y12yW(y),c=3a:n=1yn(1+y)3n(3nn){H3nHn}=1+y12yln(1+y)+31+y12yW(y).

    Combining the above formulae with Theorem 1 and then keeping in mind the equalities

    H2n=ˉH2n+Hn,On=ˉH2n+Hn2,H3n=(H3nHn)+Hn,

    we establish further closed formulae for four series with a free variable "y".

    Theorem 5 (ρ<y<1/2).

    (a)n=1(3nn)ˉH2nyn(1+y)3n=3+3y12y4y4+yln4+y+y2,(b)n=1(3nn)H2nyn(1+y)3n=3+3y24yy4+yln(2(1+y+y2+4y)2y(2+y+y2+4y))(3+3y)ln(12y)2(12y),(c)n=1(3nn)Onyn(1+y)3n=3+3y24yy4+yln(1+y+y2+4y12y)(3+3y)ln(12y)4(12y),(d)n=1(3nn)H3nyn(1+y)3n=1+y24yln((1+y)2(12y)3)+3+3y24yy4+yln(2(1+y+y2+4y)2y(2+y+y2+4y)).

    Numerous infinite series identities with different convergence rates can be derived by assigning particular values for y in Theorems 1 and 5. Five groups of representative examples are recorded as corollaries. In particular, the second formula (b) and the last formula (e) displayed in Corollary 6 confirm (1.1) and (1.2) conjectured by Sun [23, Eqs (2.12) and (2.13)].

    Corollary 6 (y3352 in Theorems 1 and 5).

    (a)n=1(227)n(3nn)ˉH2n=332ln(31),(b)n=1(227)n(3nn)H2n=1+32{3ln23ln(33)},(c)n=1(227)n(3nn)Hn=334ln(43)+3ln(2+33),(d)n=1(227)n(3nn)On=3+32{ln(1+32)34ln3},(e)n=1(227)n(3nn)H3n=1+34ln(4(7+43)3)3ln2.

    Corollary 7 (y52 in Theorems 1 and 5).

    (a)n=1(18)n(3nn)ˉH2n=3(15)5ln(512),(b)n=1(18)n(3nn)H2n=3(2+5)5ln(3+52)3ln55,(c)n=1(18)n(3nn)Hn=32ln(3+52)+35ln(11+5510),(d)n=1(18)n(3nn)On=3(1+5)25ln(2+5)3ln525,(e)n=1(18)n(3nn)H3n=ln(11+55)+35ln(4+255).

    Corollary 8 (y525 in Theorems 1 and 5).

    (a)n=1(564)n(3nn)ˉH2n=6(51)11ln(552),(b)n=1(564)n(3nn)H2n=6511ln(25+9522)311ln(233510),(c)n=1(564)n(3nn)Hn=3511ln(26711952)611ln(7+510),(d)n=1(564)n(3nn)On=3(1+5)11ln(4+511)+3511ln5,(e)n=1(564)n(3nn)H3n=6511ln(4(4+5)11)+111ln(200(2667735)116).

    Corollary 9 (y110 in Theorems 1 and 5).

    (a)n=1(100729)n(3nn)ˉH2n=38313ArcCos(161200),(b)n=1(100729)n(3nn)H2n=98ln(65)38313ArcCos(6780),(c)n=1(100729)n(3nn)Hn=98ln(65)+38313ArcCos(79878000),(d)n=1(100729)n(3nn)On=916ln(65)316313ArcCos(720),(e)n=1(100729)n(3nn)H3n=38ln(3215)38313ArcCos(6780).

    Corollary 10 (y7352 in Theorems 1 and 5).

    (a)n=1(3+554)n(3nn)ˉH2n=6565ln(1+15+653+5),(b)n=1(3+554)n(3nn)H2n=3(1+5)4ln(2+53)+3/25+5ln(351+30654),(c)n=1(3+554)n(3nn)Hn=3(1+5)4ln(2+53)+3/25+5ln(113+185825113185825),(d)n=1(3+554)n(3nn)On=3(1+5)8ln(2+53)+3/85+5ln(354+21565),(e)n=1(3+554)n(3nn)H3n=1+54ln(11+556)+3/25+5ln(351+30654).

    We remark that the second formula (b) and the last series (e) in this corollary refine identity (1.3) conjectured by Sun [23, Eq (2.15)]:

    n=1(3+554)n(3nn){H3nH2n}=1+52ln(9352).

    Now, we turn to examine Bailey's cubic transformation (Bailey [2, Eq (4.05)])

    3F2[a3,1+a3,2+a31+a+c2,2+ac2|27y4(1+y)3]=(1+y)a×3F2[a,c,1c1+a+c2,2+ac2|y4]. (4.1)

    Under the parameter replacements "a1+6ax,c2cx", it can be reformulated as

    n=0(y4(1+y)3)n(1+6ax)3nn!(1+3ax+cx)n(32+3axcx)n=(1+y)1+6ax×{1+2cxk=1(y4)k(1+6ax)k(1+2cx)k1(12cx)kk!(1+3ax+cx)k(32+3axcx)k}, (4.2)

    where, as before, both series converge for "y(ρ,12)", or equivalently, 27y4(1+y)3(1,1).

    When x=0, the above series becomes the following simpler one:

    n=0(3nn)yn(1+2n)(1+y)3n=1+y.

    Instead, the coefficients of x across (4.2) result in the general formula as below:

    n=1yn(1+y)3n(3nn){6aH3n(3a+c)Hn2(3ac)On1+2n+4(3ac)n(1+2n)2}=6a(1+y)ln(1+y)+2c(1+y)k=1(k1)!(32)k(y4)k.

    For brevity, we introduce the notations U(y) and V(y) for the two series:

    U(y)=k=1(k1)!(32)k(y4)kandV(y)=n=0yn(1+y)3n(3nn)n(1+2n)2.

    They are evaluated in closed form by the following lemma:

    Lemma 11.

    (a)U(y)=2+24+yyln4+yy2,4<y<4;(b)V(y)=(1+y)3yln(y+1+y)(1+y),ρ<y<1/2.

    Proof. The first series can be evaluated by computing the integral as follows:

    U(y)=k=1(k1)!(32)k(y4)k=k=1B(k,32)(y4)k=k=1(y4)k10xk11xdx=101xdxxk=1(xy4)k=10y1xdx4+xy=102yT24+yT2ydT1xT=2+24+yyln4+yy2.

    For the second series V(y), by shifting forward the summation index nn+1, we can rewrite it as

    V(y)=n=0yn(1+y)3n(3nn)n(1+2n)2=y(1+y)3n=0yn(1+y)3n(3n+3n)13+2n.

    Then, for "α=β=3", perform the replacement τxy/(1+y)3 in Lambert's second series

    n=0xnyn(1+y)3n(3n+3n)=(1+T)412T.

    Now multiplying this equation by x12 and then integrating across over x[0,1], we can proceed with

    n=0yn(1+y)3n(3n+3n)23+2n=10x12(1+T)412Tdxx=T(1+y)3y(1+T)3=(1+y)9yyy0T(1+T)3dT.

    By means of integration by parts, we can further compute

    y0T(1+T)3dT=2y1+y+y01T(1+T)dT=2ln(y+1+y)2y1+y.

    After substitution, the second formula in Lemma 11 follows accordingly.

    Therefore, we obtain the following reduced transformation:

    n=0yn(1+y)3n(3nn){6aH3n(3a+c)Hn2(3ac)On1+2n}=6a(1+y)ln(1+y)+2c(1+y)U(y)4(3ac)V(y). (4.3)

    By specifying two parameters, a and c in the above equality, we deduce four independent series:

    a=0:n=1yn(1+y)3n(3nn){ˉH2n1+2n}=(1+y)U(y)+2V(y),c=0:n=1yn(1+y)3n(3nn){H3nH2n1+2n}=(1+y)ln(1+y)2V(y),c=3a:n=1yn(1+y)3n(3nn){H3nHn1+2n}=(1+y)ln(1+y)+(1+y)U(y),c=3a:n=1yn(1+y)3n(3nn){H3n2On1+2n}=(1+y)ln(1+y)(1+y)U(y)4V(y).

    For the above four equations, first replacing U(y) and V(y) by their algebraic values in Lemma 11, and then putting the resulting equations in conjunction with that in Theorem 2, we establish, after some routine simplifications, four closed formulae as in the following theorem:

    Theorem 12 (ρ<y<1/2).

    (a)n=1yn(1+y)3n(3nn)ˉH2n1+2n=2(1+y)3yln(y+1+y)+2(1+y)4+yyln(4+yy2),(b)n=1yn(1+y)3n(3nn)H2n1+2n=2(1+y)3yln(y+1+y)3+3y2ln(12y)+(1+y)4+y2yln(2+2y2y2+4y2y(2+yy2+4y)),(c)n=1yn(1+y)3n(3nn)On1+2n=2(1+y)3yln(y+1+y)3+3y4ln(12y)+(1+y)4+y2yln(1+yy2+4y12y),(d)n=1yn(1+y)3n(3nn)H3n1+2n=2(1+y)+1+y2ln((1+y)2(12y)3)+(1+y)4+y2yln(2+2y2y2+4y2y(2+yy2+4y)).

    By assigning particular values for y in Theorems 2 and 12, we can deduce numerous infinite series identities with different convergence rates. In order to show the variety of implications, we record five representative classes of infinite series values.

    Corollary 13 (y52 in Theorems 2 and 12).

    (a)n=1(18)n(3nn)ˉH2n1+2n=22ln(3+101+2)(3+5)ln(1+52),(b)n=1(18)n(3nn)H2n1+2n=22ln(3+101+2)(645)ln(1+52)5ln5,(c)n=1(18)n(3nn)Hn1+2n=(553)ln(1+52)5ln5,(d)n=1(18)n(3nn)On1+2n=22ln(3+101+2)(92352)ln(1+52)52ln5,(e)n=1(18)n(3nn)H3n1+2n=(51)(2+ln2)(535)ln(1+52)5ln5.

    Corollary 14 (y3352 in Theorems 2 and 12).

    (a)n=1(227)n(3nn)ˉH2n1+2n=9+332ln(31)+96ln(3+223+2),(b)n=1(227)n(3nn)H2n1+2n=92ln(332)+332ln((3+1)3123)+96ln(3+223+2),(c)n=1(227)n(3nn)Hn1+2n=94ln(34)+332ln((3+1)4243),(d)n=1(227)n(3nn)On1+2n=34(33)ln(233)9ln343+96ln(3+223+2),(e)n=1(227)n(3nn)H3n1+2n=333+32ln(2332)+332ln(2+323).

    Corollary 15 (y324 in Theorems 2 and 12).

    (a)n=1(2+227)n(3nn)ˉH2n1+2n=33ln(6231)+9226ln(627+6(22)3),(b)n=1(2+227)n(3nn)H2n1+2n=33ln(312)(992)ln(1+23)+9226ln(627+6(22)3),(c)n=1(2+227)n(3nn)Hn1+2n=33ln(2+32+3)(992)ln(1+23),(d)n=1(2+227)n(3nn)On1+2n=(9292)ln(63)332ln(2+3)+9226ln(627+6(22)3),(e)n=1(2+227)n(3nn)H3n1+2n=626+33ln(312)(332)ln(3+223).

    Corollary 16 (y15 in Theorems 2 and 12).

    (a)n=1(25216)n(3nn)ˉH2n1+2n=1265ln(1+65)12215ln(1+2125),(b)n=1(25216)n(3nn)H2n1+2n=95ln(53)+1265ln(1+65)+6215ln(921215),(c)n=1(25216)n(3nn)Hn1+2n=95ln(53)+3215ln(2571321250),(d)n=1(25216)n(3nn)On1+2n=910ln(53)+1265ln(1+65)+3215ln(62115),(e)n=1(25216)n(3nn)H3n1+2n=125+35ln(203)+6215ln(921215).

    Corollary 17 (y110 in Theorems 2 and 12).

    (a)n=1(100729)n(3nn)ˉH2n1+2n=275arccot39395arccot39,(b)n=1(100729)n(3nn)H2n1+2n=275arccot393920arccos(6780)2720ln(65),(c)n=1(100729)n(3nn)Hn1+2n=93920arccos(79878000)2720ln(65),(d)n=1(100729)n(3nn)On1+2n=275arccot393920arccos(2740)2740ln(65),(e)n=1(100729)n(3nn)H3n1+2n=9593920arccos(6780)920ln(3215).

    Under the parameter replacements "a6ax,c2cx", Bailey's cubic transformation (4.1) can be reformulated alternatively as

    n=0(y4(1+y)3)n(6ax)3nn!(1+3axcx)n(12+3ax+cx)n=(1+y)6ax×{1+12acx2k=1(y4)k(1+6ax)k1(1+2cx)k1(12cx)kk!(1+3axcx)k(12+3ax+cx)k}.

    Both series in the above equation converge subject to the same condition "y(ρ,12)", or equivalently, 27y4(1+y)3(1,1) (as before).

    Equating the constant terms from both sides yields the algebraic identity below

    n=1(3nn)ynn(1+y)3n=3ln(1+y).

    Instead, the coefficients of x result in the following infinite series identity involving a free variable "y" and two linear parameters a and c:

    n=1yn(1+y)3n(3nn){6aH3n(3ac)Hn2(3a+c)Onn2an2}=9aln2(1+y)+6ck=1(k1)!k(12)k(y4)k.

    Let U(y) and V(y) stand for the two series

    U(y)=k=1(k1)!k(12)k(y4)kandV(y)=n=1ynn2(1+y)3n(3nn).

    They admit closed formulae as in the lemma below:

    Lemma 18.

    (a)U(y)=2ln2(2y+4+y),4<y<4;(b)V(y)=3{π26+lnyln(1+y)2ln2(1+y)Li2(11+y)},ρ<y<1/2.

    Proof. The first series U(y) can be reformulated as

    U(y)=k=1(k1)!k(12)k(y4)k=k=1B(k,12)(y4)k=k=1(y/4)kk10xk1dx1x=10dxx1xk=1(xy/4)kk=10ln(1+xy4)dxx1x=10dTTln(1+(2+y)T+T2(1+T)2)x4T(1+T)2=10dTT{2ln(1+T)ln(1+4T(y+4+y)2)ln(1+4T(y4+y)2)}=π26+Li2(4(y+4+y)2)+Li2(4(y4+y)2).

    Then the closed formula for U(y) in the lemma follows by applying the dilogarithmic equation

    Li2(x)+Li2(x1)=π26ln2x2,wherex>0.

    For the second series, we can rewrite it by reindexing nn+1 as

    V(y)=n=1ynn2(1+y)3n(3nn)=3y(1+y)3n=0yn(1+y)3n(3n+2n)1(1+n)2.

    Now specializing Lambert's second series by "α=2 and β=3" and τxy/(1+y)3

    n=0xnyn(1+y)3n(3n+2n)=(1+T)312T,wherex=T(1+y)3y(1+T)3,

    then integrating twice across this equation, we can proceed with

    n=0yn(1+y)3n(3n+2n)1(1+n)2=10dttt0(1+T)312Tdx=10(1+T)3lnx12Tdx=(1+y)3yy0dT1+Tln(T(1+y)3y(1+T)3)x=T(1+y)3y(1+T)3=(1+y)3y{y0dT1+Tln(T(1+y)3y)3y0ln(1+T)1+TdT}=(1+y)3y{π26+lnyln(1+y)2ln2(1+y)Li2(11+y)}.

    By substitution, the closed formula for V(y) in the lemma follows consequently.

    Thus, we have the following reduced transformation:

    n=1yn(1+y)3n(3nn){6aH3n(3ac)Hn2(3a+c)Onn}=9aln2(1+y)+6cU(y)+2aV(y). (5.1)

    By specifying two parameters, a and c, we deduce four independent series

    a=0:n=1yn(1+y)3n(3nn)ˉH2nn=3U(y),c=0:n=1yn(1+y)3n(3nn){H3nH2nn}=32ln2(1+y)+V(y)3,c=3a:n=1yn(1+y)3n(3nn){H3n2Onn}=32ln2(1+y)+3U(y)+V(y)3,c=3a:n=1yn(1+y)3n(3nn){H3nHnn}=32ln2(1+y)3U(y)+V(y)3.

    For these four equations, replacing U(y) and V(y) first by their algebraic expressions and then relating the resulting equations to that in Theorem 3, we find, after some simplifications, four infinite series identities as below:

    Theorem 19 (ρ<y<1/2). Letting Θ(y) be defined as in Theorem 3, the following algebraic identities hold:

    (a)n=1yn(1+y)3n(3nn)ˉH2nn=6ln2(2y+4+y),(b)n=1yn(1+y)3n(3nn)H2nn=π22+3Θ(y)+3lnyln(1+y)92ln2(1+y)+6ln2(2y+4+y),(c)n=1yn(1+y)3n(3nn)Onn=π24+32Θ(y)+32lnyln(1+y)94ln2(1+y)+6ln2(2y+4+y),(d)n=1yn(1+y)3n(3nn)H3nn=2π23+3Θ(y)+4lnyln(1+y)5ln2(1+y)+6ln2(2y+4+y)Li2(11+y).

    By assigning five particular values for y in Theorems 3 and 19, five classes of infinite series identities are displayed in the following corollaries:

    Corollary 20 (y52 in Theorems 3 and 19).

    (a) n=1(18)n(3nn)ˉH2nn=32ln2(1+52),(b) n=1(18)n(3nn)H2nn=π22+32ln22+3Θ(52)+6ln(1+5)ln(1+54),(c) n=1(18)n(3nn)Hnn=π22+3Θ(52)+92ln(1+5)ln(1+54),(d) n=1(18)n(3nn)Onn=π24+32ln22+32Θ(52)+154ln(1+5)ln(1+54),(e)n=1(18)n(3nn)H3nn=2π23+112ln22+3Θ(52)+ln(1+5)2ln((1+5)17238)Li2(1+54).

    Corollary 21 (y525 in Theorems 3 and 19).

    (a) n=1(564)n(3nn)ˉH2nn=32ln2(5+510),(b) n=1(564)n(3nn)H2nn=π22+3Θ(525)+32ln(5+58)ln(64+1285)+32ln2(5+510),(c) n=1(564)n(3nn)Hnn=π22+3Θ(525)+32ln(5+58)ln(64+1285),(d) n=1(564)n(3nn)Onn=π24+32Θ(525)+34ln(5+58)ln(64+1285)+32ln2(5+510),(e) n=1(564)n(3nn)H3nn=2π23+3Θ(525)Li2(5+58)+32ln2(5+510)+ln(5+58)ln(8(5+5)754).

    Corollary 22 (y13 in Theorems 3 and 19).

    (a)n=1(964)n(3nn)ˉH2nn=32ln2(7+136),(b) n=1(964)n(3nn)H2nn=π2232ln(43)ln(643)+3Θ(13)+32ln2(7+136),(c) n=1(964)n(3nn)Hnn=π2232ln(43)ln(643)+3Θ(13),(d) n=1(964)n(3nn)Onn=π2434ln(43)ln(643)+32Θ(13)+32ln2(7+136),(e) n=1(964)n(3nn)H3nn=2π23ln(43)ln(10243)+3Θ(13)Li2(34)+32ln2(7+136).

    Corollary 23 (y3352 in Theorems 3 and 19).

    (a) n=1(227)n(3nn)ˉH2nn=32ln2(31),(b) n=1(227)n(3nn)H2nn=π22+32ln(54)ln(23)+6ln(1+3)ln(1+32)+3Θ(3353),(c) n=1(227)n(3nn)Hnn=π22+32ln(1+33)ln(27(1+3)34)+3Θ(3353),(d) n=1(227)n(3nn)Onn=π24+34ln(1+32)ln((1+3)52)+34ln(54)ln(23)+32Θ(3353),(e) n=1(227)n(3nn)H3nn=2π23+32ln2(1+32)Li2(1+33)+3Θ(3353)+ln(1+33)ln(35(1+3)724).

    Corollary 24 (y324 in Theorems 3 and 19).

    (a) n=1(2+227)n(3nn)ˉH2nn=32ln2(1+32+6),(b) n=1(2+227)n(3nn)H2nn=π22+3Θ(324)+32ln2(1+32+6)+32ln(1+23)ln(27(1+2)2),(c) n=1(2+227)n(3nn)Hnn=π22+3Θ(324)+32ln(1+23)ln(27(1+2)2),(d) n=1(2+227)n(3nn)Onn=π24+32Θ(324)+32ln2(1+32+6)+34ln(1+23)ln(27(1+2)2),(e) n=1(2+227)n(3nn)H3nn=2π23+3Θ(324)+32ln2(1+32+6)Li2(1+23)+ln(1+23)ln(35(1+2)34).

    By integrating Lambert's series and manipulating the cubic transformations for 3F2-series through the "coefficient extraction method", we have shown several algebraic formulae for infinite series containing binomial coefficient (3nn), harmonic-like numbers, and in particular, a free variable "y". As showcases, three classes of infinite series were examined in detail from Sections 3–5. More variants of these series exist and can be treated analogously. For instance, the transformation formula (3.1) under the replacements "a1+6ax,c2cx" becomes

    3F2[1+2ax,23+2ax,43+2ax1+3ax+cx,32+3axcx|27y4(1+y)3]=(1+y)2+6ax12y×4F3[43+2ax,1+6ax,2cx,12cx13+2ax,1+3ax+cx,32+3axcx|y4].

    Then by carrying out the same procedure as in the preceding sections, we can establish the algebraic identities for five infinite series, as in the theorem below:

    Theorem 25 (ρ<y<1/2). Letting Λ(y) be the function defined by

    Λ(y)=3ln(12y)+2yy2+4yln(2y(2+y+y2+4y)2y(2+yy2+4y)),

    we have the closed algebraic formulae for five infinite series:

    (a) n=1yn(1+y)3n(3n+1n)ˉH2n+1=2(y2)(1+y)2(12y)y2+4yln4+yy2,(b) n=1yn(1+y)3n(3n+1n)H2n+1=(1+y)212y{2y4y2+4yln4+yy2Λ(y)2},(c) n=1yn(1+y)3n(3n+1n)Hn=(1+y)24y2Λ(y),(d) n=1yn(1+y)3n(3n+1n)On+1=(1+y)212y{2y4y2+4yln4+yy2Λ(y)4},(e) n=1yn(1+y)3n(3n+1n)H3n+1=(1+y)212y{2y4y2+4yln4+yy2Λ(y)2+ln(1+y)}.

    From the algebraic identities exhibited for the series with harmonic-like numbers of the first order, it is natural to ask: what would happen for the corresponding series involving harmonic-like numbers of the second order? Our computations manifested that the resulting expressions are very complex and convoluted, which can be exemplified by the following attempt made by the authors. Extracting the coefficient of x2 across (3.2), we can derive, after a number of reductions and simplifications, the following formulae:

    (a)n=1yn(1+y)3n(3nn){ˉH22n+H22n}=6y+62y1{U(y)+W(y)},(b)n=1yn(1+y)3n(3nn){(H3nH2n)2+H22nH23n}=1+y12yln2(1+y),(c)n=1yn(1+y)3n(3nn){(2OnH3n)2+4O2nH23n}=1+y12y{ln2(1+y)+6ln(1+y)W(y)10U(y)12W(y)},(d)n=1yn(1+y)3n(3nn){(HnH3n)2+H2nH23n}=1+y12y{ln2(1+y)6ln(1+y)W(y)2U(y)};

    where W(y)andU(y) are as in Lemmas 4 and 18, respectively, and W(y) is given by

    W(y)=k=1(k1)!(12)k(y4)k¯H2k=(1y4+y)ln2(4+y+y2)y4+yLi2(2yy+4+y).

    There are altogether nine harmonic-like numbers appearing in the above four series

    {H2n,O2n,H23n;H2n,O2n,H23n;HnOn,HnH3n,H3nOn}.

    To evaluate the nine corresponding independent "nuclear series", it is necessary to find five similar independent equations. It seems quite a tough problem that the authors failed to arrive at solutions, even though we did succeed in determining the following long and ugly expression involving six terms in dilogarithms (that prevents us from making further simplifications). Perhaps the only value of this formula lies in its existence.

    n=1(3nn)H2nyn(1+y)3n=y03(1+y)3ln(T(1+y)3y(1+T)3)dT(12y)(1+T)(T2y+Ty2+3Ty1)=π2(1+y)2(12y)+3(1+y)ln2(1+y)12y+3(1+y)lnyln(1+y)12y3(1+y)12yLi2(11+y)+9(1+y)12yy4+yln(1+y)ln(2+y+4y+y22)+3(1+y)2(12y)(1+y4+y){3Li2(2y(1+y)(y4+y))3Li2(2yy4+y)+Li2(2y3/2y(3+y)(1+y)4+y)}+3(1+y)2(12y)(1y4+y){3Li2(2y(1+y)(y+4+y))3Li2(2yy+4+y)+Li2(2y3/2y(3+y)+(1+y)4+y)}.

    Therefore, to evaluate the series containing binomial coefficient (3nn) and harmonic-like numbers of the second and/or higher orders, one needs to find out different approaches. The interested readers are enthusiastically encouraged to make further explorations.

    C. Li: Writing, computation and review; W. Chu: Methodology and supervision. Both of authors have read and approved the final version of the manuscript for publication.

    The authors declare they have not used Artificial Intelligence tools in the creation of this article.

    The authors express their gratitude to anonymous referees for their careful reading, critical comments and valuable suggestions that make the manuscript improved substantially during the revision.

    Prof. Wenchang Chu is the Guest Editor of special issue "Combinatorial Analysis and Mathematical Constants" for AIMS Mathematics. Prof. Wenchang Chu was not involved in the editorial review and the decision to publish this article. The authors declare that there are no conflicts of interest regarding the publication of this paper.



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