Masteries · Jason GlowneyArithmoí Book 1

Masteries

1.6.4 Harmonic Logarithms and the Infinite Subtangent Space

We begin this sec­tion, by re­turn­ing to a de­riv­a­tive con­sid­ered ear­li­er in the chap­ter

dkd(θrm)k((θrm)00!)=0!θrm,\begin{array}{r} \frac{d^{k}}{d\left( \theta_{r}^{m} \right)^{k}}\left( \frac{\left( \theta_{r}^{m} \right)^{0}}{0!} \right) = \frac{0!}{\theta_{r}^{m}}, \end{array}
(1.6.77)

to cog­i­tate the in­def­i­nite in­te­gra­tion process for the sub­tan­gent space, start­ing at (0!θrm)\left( \frac{0!}{\theta_{r}^{m}} \right), find­ing the series

fℂ−k(0!θrm)=ln⁡(θrm)+θrm(ln⁡(θrm)−1)+(θrm)22!(ln⁡(θrm)−1−12)+(θrm)33!(ln⁡(θrm)−1−12−13)+…,\begin{array}{r} f_{\mathbb{C}}^{- k}\left( \frac{0!}{\theta_{r}^{m}} \right) = \ln\left( \theta_{r}^{m} \right) + \theta_{r}^{m}\left( \ln\left( \theta_{r}^{m} \right) - 1 \right) + \frac{\left( \theta_{r}^{m} \right)^{2}}{2!}\left( \ln\left( \theta_{r}^{m} \right) - 1 - \frac{1}{2} \right) \\ + \frac{\left( \theta_{r}^{m} \right)^{3}}{3!}\left( \ln\left( \theta_{r}^{m} \right) - 1 - \frac{1}{2} - \frac{1}{3} \right) + \ldots, \end{array}
(1.6.78)

for 0!θrm\frac{0!}{\theta_{r}^{m}}, having the matrix rep­re­sen­ta­tion (θrm)−1\left( \theta_{r}^{m} \right)^{- 1}. A closer look at the series above, shows each it­er­a­tive el­e­ment takes the form

(θrm)kk!(ln⁡(θrm)−(∑k=1n1k)),\begin{array}{r} \frac{\left( \theta_{r}^{m} \right)^{k}}{k!}\left( \ln\left( \theta_{r}^{m} \right) - \left( \sum_{k = 1}^{n}\frac{1}{k} \right) \right), \end{array}
(1.6.79)

in which, the har­mon­ic num­bers Hn=∑k=1n1kH_{n} = \sum_{k = 1}^{n}\frac{1}{k}, have ap­peared for each of the in­te­gra­tion re­sults, ev­i­dence of a deeper con­nec­tion the sub­tan­gent space has with analy­sis. An ex­am­ple of this con­nec­tion is seen by taking the limit as n→∞n \rightarrow \infty, for the dif­fer­ence be­tween the log­a­rithm func­tion and the har­mon­ic series, find­ing this limit con­verges to the neg­a­tive value of the Euler-Mascheroni con­stant γ\gamma

limn→∞⁡(ln⁡(n)−(∑k=1n 1k))=−γ≈−0.57721….\begin{array}{r} \lim_{n \rightarrow \infty}\left( \ln(n) - \left( \sum_{k = 1}^{n}{\ \frac{1}{k}} \right) \right) = - \gamma \approx - 0.57721\ldots. \end{array}
(1.6.80)

Know­ing this limit con­verges to −γ- \gamma, we can re­frame it in the con­text of the sub­tan­gent rep­re­sen­ta­tion

limk→∞⁡((θrm)kk!(ln⁡(θrm)−(∑j=1k1j))),\begin{array}{r} \lim_{k \rightarrow \infty}\left( \frac{\left( \theta_{r}^{m} \right)^{k}}{k!}\left( \ln\left( \theta_{r}^{m} \right) - \left( \sum_{j = 1}^{k}\frac{1}{j} \right) \right) \right), \end{array}
(1.16.81)

which will con­verge to zero given the pres­ence of the rec­i­p­ro­cal fac­to­r­i­al func­tion as k→∞k \rightarrow \infty. This leads to a way to convey the in­fi­nite series of in­te­grals that is worthy of fur­ther con­sid­er­a­tion

∑k=0∞(θrm)kk!(ln⁡(θrm)−Hk),\begin{array}{r} \sum_{k = 0}^{\infty}{\frac{\left( \theta_{r}^{m} \right)^{k}}{k!}\left( \ln\left( \theta_{r}^{m} \right) - H_{k} \right)}, \end{array}
(1.6.82)

for HkH_{k}, defin­ing the kthk^{th} har­mon­ic number. The re­la­tion­ship be­tween the log­a­rithm func­tion and har­mon­ic num­bers brings us to math­e­mat­i­cal­ly relate the in­fi­nite sym­me­try group to what are de­fined as the har­mon­ic log­a­rithms. Steven Roman in 1992 de­fined the har­mon­ic log­a­rithms1, as

λnt(x)=⌊ n⌉!D−n(ln⁡(x)) t,\begin{array}{r} \lambda_{n}^{t}(x) = \left\lfloor \left. \ n \right\rceil!D^{- n}\left( \ln(x) \right) \right.\ ^{t}, \end{array}
(1.6.83)

where ⌊ n⌉!\left\lfloor \left. \ n \right\rceil! \right.is the Roman fac­to­r­i­al

⌊ n⌉! ={n! (n≥0)(−1)−n−1(−n−1)! (n<0)  , \begin{array}{r} \left\lfloor \left. \ n \right\rceil! \right.\ = \left\{ \begin{array}{r} n!\ (n \geq 0) \\ \frac{( - 1)^{- n - 1}}{( - n - 1)!}\ (n < 0) \end{array}\ \ ,\ \right. \end{array}
(1.6.84)

D−nD^{- n}, rep­re­sents the nthn^{th}in­te­gra­tion it­er­a­tion, tt is the order of the har­mon­ic log­a­rithm, and in­te­gra­tion is as­sumed to have no ar­bi­trary con­stants. For our case, the har­mon­ic log­a­rithms are first order in tt, where λ01(θrm)=ln⁡(θrm)\lambda_{0}^{1}\left( \theta_{r}^{m} \right) = \ln\left( \theta_{r}^{m} \right), which is the n=0n = 0 term in our in­fi­nite series, and can be re­stat­ed suc­cinct­ly, as

∑n=0∞λnt(θrm).\begin{array}{r} \sum_{n = 0}^{\infty}{\lambda_{n}^{t}\left( \theta_{r}^{m} \right)}. \end{array}
(1.6.85)

The value (0!θrm)\left( \frac{0!}{\theta_{r}^{m}} \right) in our in­fi­nite series rep­re­sen­ta­tion ap­pears to be a branch­ing point of the har­mon­ic log­a­rithm order, and at the same time, one for the ex­po­nen­tial map­ping, the tan­gent space, and the sub­tan­gent space. Roman de­fined the har­mon­ic log­a­rithm, as λ0t(θrm)=(ln⁡(θrm))t\lambda_{0}^{t}\left( \theta_{r}^{m} \right) = \left( \ln\left( \theta_{r}^{m} \right) \right)^{t}, and by this de­f­i­n­i­tion, it is also the in­te­gral of (0!θrm)\left( \frac{0!}{\theta_{r}^{m}} \right)

D−1λ−1t(θrm)=⌊ 0!⌉ λ0t(θrm)=(ln⁡(θrm))t.\begin{array}{r} D^{- 1}\lambda_{- 1}^{t}\left( \theta_{r}^{m} \right) = \left\lfloor \left. \ 0! \right\rceil \right.\ \lambda_{0}^{t}\left( \theta_{r}^{m} \right) = \left( \ln\left( \theta_{r}^{m} \right) \right)^{t}. \end{array}
(1.6.86)

Since θrm=reiθ\theta_{r}^{m} = re^{i\theta}, there are three dif­fer­ent ways to con­sid­er the in­te­gral:

∫0!θrm dθrm=ln⁡(θrm),\begin{array}{r} \int_{}^{}\frac{0!}{\theta_{r}^{m}}\ d\theta_{r}^{m} = \ln{\left( \theta_{r}^{m} \right),} \end{array}
(1.6.87)
∫0!reiθ dr=ln⁡(r)eiθ,\begin{array}{r} \int_{}^{}\frac{0!}{re^{i\theta}}\ dr = \frac{\ln(r)}{e^{i\theta}}, \end{array}
(1.6.88)
∫0!reiθ dθ=ireiθ,\begin{array}{r} \int_{}^{}\frac{0!}{re^{i\theta}}\ d\theta = \frac{i}{{re}^{i\theta}}, \end{array}
(1.6.89)

where the result of the first in­te­gral is the sub­tan­gent space, the second an in­te­gral with re­spect to the radial com­po­nent, and the third is an in­te­gral with re­spect to the angle vari­able. We take con­tin­u­al in­te­grals of the sub­tan­gent space el­e­ments, find­ing the fol­low­ing in­fi­nite series emerges

fℂ−∞((0!θrm)dθrm)=ln⁡(θrm)+θrm(ln⁡(θrm)−1)+(θrm)22!(ln⁡(θrm)−1−12)+(θrm)33!(ln⁡(θrm)−1−12−13)+…,\begin{array}{r} f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)d\theta_{r}^{m} \right) = \ln\left( \theta_{r}^{m} \right) + \theta_{r}^{m}\left( \ln\left( \theta_{r}^{m} \right) - 1 \right) + \frac{\left( \theta_{r}^{m} \right)^{2}}{2!}\left( \ln\left( \theta_{r}^{m} \right) - 1 - \frac{1}{2} \right) \\ + \frac{\left( \theta_{r}^{m} \right)^{3}}{3!}\left( \ln\left( \theta_{r}^{m} \right) - 1 - \frac{1}{2} - \frac{1}{3} \right) + \ldots, \end{array}
(1.6.90)

and this is the same series that we found at the be­gin­ning of the sec­tion, for the in­fi­nite in­te­gral fℂ−∞(0!θrm)f_{\mathbb{C}}^{- \infty}\left( \frac{0!}{\theta_{r}^{m}} \right). Look­ing close­ly at this series, the vari­able θrm\theta_{r}^{m} rep­re­sents the tan­gent space, and by the de­f­i­n­i­tion of sub­tan­gent space, as the log­a­rithm of the tan­gent space, ln⁡(θrm)\ln\left( \theta_{r}^{m} \right) re­sults in

ln⁡(θrm)=ln⁡(reiθ)=ln⁡(r)+iθ.\begin{array}{r} \ln\left( \theta_{r}^{m} \right) = \ln\left( re^{i\theta} \right) = \ln{(r) + i\theta.} \end{array}
(1.6.91)

What stands out about the in­fi­nite sub­tan­gent space in­te­gral, is that we are also able to pro­ceed in the de­riv­a­tive di­rec­tion in­fi­nite­ly, mean­ing that there is not a hard stop in the process. This in­fi­nite de­riv­a­tive takes on the fol­low­ing al­ter­nat­ing series

fℂ∞((ln⁡(θrm))dθrm)=0!θrm−1!(θrm)2+2!(θrm)3−3!(θrm)4+4!(θrm)5−5!(θrm)6+…,\begin{array}{r} f_{\mathbb{C}}^{\infty}\left( \left( \ln\left( \theta_{r}^{m} \right) \right)d\theta_{r}^{m} \right) = \frac{0!}{\theta_{r}^{m}} - \frac{1!}{\left( \theta_{r}^{m} \right)^{2}} + \frac{2!}{\left( \theta_{r}^{m} \right)^{3}} - \frac{3!}{\left( \theta_{r}^{m} \right)^{4}} + \frac{4!}{\left( \theta_{r}^{m} \right)^{5}} - \frac{5!}{\left( \theta_{r}^{m} \right)^{6}} + \ldots, \end{array}
(1.6.92)

where we have passed through the "zero-point" in the process, mean­ing that the sub­tan­gent space ln⁡(θrm)\ln\left( \theta_{r}^{m} \right) is a con­tin­u­ous func­tion. The other two in­te­gral ex­am­ples are also con­tin­u­ous in the in­te­gra­tion di­rec­tion, where we find the fol­low­ing in­te­gral series

fℂ−∞((0!θrm)dr)=e−iθln⁡(r)+re−iθ(ln⁡(r)−1) +r22!e−iθ(ln⁡(r)−1−12)+r33!e−iθ(ln⁡(r)−1−12−13)+…,\begin{array}{r} f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)dr \right) = {e^{- i\theta}\ln}(r) + {re}^{- i\theta}\left( \ln(r) - 1 \right) \\ \ + \frac{r^{2}}{2!}e^{- i\theta}\left( \ln(r) - 1 - \frac{1}{2} \right) + \frac{r^{3}}{3!}e^{- i\theta}\left( \ln(r) - 1 - \frac{1}{2} - \frac{1}{3} \right) + \ldots, \end{array}
(1.6.93)
fℂ−∞((0!θrm)dθ)=ie−iθr−e−iθr−ie−iθr+e−iθr+…,\begin{array}{r} f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)d\theta \right) = \frac{{ie}^{- i\theta}}{r} - \frac{e^{- i\theta}}{r} - \frac{{ie}^{- i\theta}}{r} + \frac{e^{- i\theta}}{r} + \ldots, \end{array}
(1.6.94)

and de­riv­a­tive series, as

fℂ∞((e−iθln⁡(r))dr)=0!reiθ−1!r2eiθ+2!r3eiθ−3!r4eiθ+4!r5eiθ−5!r6eiθ+…,\begin{array}{r} f_{\mathbb{C}}^{\infty}\left( \left( {e^{- i\theta}\ln}(r) \right)dr \right) = \frac{0!}{re^{i\theta}} - \frac{1!}{r^{2}e^{i\theta}} + \frac{2!}{r^{3}e^{i\theta}} - \frac{3!}{r^{4}e^{i\theta}} + \frac{4!}{r^{5}e^{i\theta}} - \frac{5!}{r^{6}e^{i\theta}} + \ldots, \end{array}
(1.6.95)
fℂ∞((ie−iθr)dθ)=1reiθ−ireiθ−1reiθ+ireiθ+1reiθ−ireiθ−….\begin{array}{r} f_{\mathbb{C}}^{\infty}\left( \left( \frac{{ie}^{- i\theta}}{r} \right)d\theta \right) = \frac{1}{re^{i\theta}} - \frac{i}{re^{i\theta}} - \frac{1}{re^{i\theta}} + \frac{i}{re^{i\theta}} + \frac{1}{re^{i\theta}} - \frac{i}{re^{i\theta}} - \ldots. \end{array}
(1.6.96)

The first two in­fi­nite in­te­gral series fℂ−∞((0!θrm)dθrm)f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)d\theta_{r}^{m} \right), fℂ−∞((0!θrm)dr)f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)dr \right) are con­ver­gent, ev­i­denced by the pres­ence of the rec­i­p­ro­cal fac­to­r­i­al func­tions

fℂ−∞((0!θrm)dθrm)=∑k=0∞(θrm)kk!(ln⁡(θrm)−Hk)=−eθrm(Γ(0,θrm)+γ),\begin{array}{r} f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)d\theta_{r}^{m} \right) = \sum_{k = 0}^{\infty}{\frac{\left( \theta_{r}^{m} \right)^{k}}{k!}\left( \ln\left( \theta_{r}^{m} \right) - H_{k} \right) =} - e^{\theta_{r}^{m}}\left( \Gamma\left( 0,\theta_{r}^{m} \right) + \gamma \right), \end{array}
(1.6.97)
fℂ−∞((0!θrm)dr)=∑k=0∞(r)kk!e−iθ(ln⁡(r)−Hk)=−e−iθer(Γ(0,r)+γ),\begin{array}{r} f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)dr \right) = \sum_{k = 0}^{\infty}{\frac{(r)^{k}}{k!}e^{- i\theta}\left( \ln(r) - H_{k} \right) =} - e^{- i\theta}e^{r}\left( \Gamma(0,r) + \gamma \right), \end{array}
(1.6.98)

find­ing the in­fi­nite sub­tan­gent space con­verges to two very beau­ti­ful forms, each com­prised of the ex­po­nen­tial func­tion, the in­com­plete gamma func­tion, and the Euler-Mascheroni con­stant γ\gamma, clear­ing a path to analy­sis and number theory.

The pres­ence of the har­mon­ic log­a­rithms in these in­fi­nite in­te­gral series leads us to con­sid­er them in terms of Roman's work. Roman de­fines the Log­a­rith­mic Bi­no­mi­al For­mu­la, for a pos­i­tive real number aa, as the Taylor series ex­pan­sion

λnt(r+a)=∑k=0∞[Dkλnt(r)]r=ak!rk,\begin{array}{r} \lambda_{n}^{t}(r + a) = \sum_{k = 0}^{\infty}\frac{\left\lbrack D^{k}\lambda_{n}^{t}(r) \right\rbrack_{r = a}}{k!}r^{k}, \end{array}
(1.6.99)

which is valid for |r|<a|r| < a. Taking the ex­am­ple, λnt(r+a)=λnt(r+1)\lambda_{n}^{t}(r + a) = \lambda_{n}^{t}(r + 1), we find the series con­verges for |r+1|<1|r + 1| < 1, to

λnt(r+1)=∑n=0∞(r+1)n(ln⁡(r+1)−Hn)=−ln⁡(r+1)+ln⁡(−r)r.\begin{array}{r} \lambda_{n}^{t}(r + 1) = \sum_{n = 0}^{\infty}{(r + 1)^{n}\left( \ln{(r + 1) - H_{n}} \right)} = - \frac{\ln{(r + 1) +}\ln( - r)}{r}. \end{array}
(1.6.100)

A for­mu­la for the har­mon­ic log­a­rithms can be stated ex­plic­it­ly, as fol­lows:

De­f­i­n­i­tion (1.6.101) – The Har­mon­ic Log­a­rithm For­mu­la is de­fined, as

λnt(r)=rn∑j=0t(−1)j(t)jcn(j)ln⁡(r)t−j,\lambda_{n}^{t}(r) = r^{n}\sum_{j = 0}^{t}{( - 1)^{j}(t)_{j}c_{n}^{(j)}\ln(r)^{t - j}},

for (t)j=t(t−1)…(t−j+1),(t)0=1(t)_{j} = t(t - 1)\ldots(t - j + 1),(t)_{0} = 1, where the con­stants cn(j)c_{n}^{(j)} are unique­ly de­ter­mined by the ini­tial con­di­tions

cn(0){1 for n≥00 for n<0  and c0(j){1 for j=00 for j≠0 ,c_{n}^{(0)}\left\{ \begin{array}{r} 1\ for\ n \geq 0 \\ 0\ for\ n < 0 \end{array} \right.\ \ and\ c_{0}^{(j)}\left\{ \begin{array}{r} 1\ for\ j = 0 \\ 0\ for\ j \neq 0 \end{array} \right.\ ,

and the re­cur­rence re­la­tion for j>0\ j > 0, is

ncn(j)=cn(j−1)+[n]cn−1(j).nc_{n}^{(j)} = c_{n}^{(j - 1)} + \lbrack n\rbrack c_{n - 1}^{(j)}.

The num­bers cn(j)c_{n}^{(j)}, are known as the har­mon­ic num­bers per Roman, and by their de­f­i­n­i­tion, they are char­ac­ter­ized by in­ter­est­ing nest­ing be­hav­iors. Start­ing, for cn(1)=Hnc_{n}^{(1)} = H_{n}, we ex­press the next two Roman har­mon­ic number series

cn(1)=1+12+13+…+1n,\begin{array}{r} c_{n}^{(1)} = 1 + \frac{1}{2} + \frac{1}{3} + \ldots + \frac{1}{n}, \end{array}
(1.6.102)
cn(2)=1+12(1+12)+13(1+12+13)+…+1n(1+12+…1n),\begin{array}{r} c_{n}^{(2)} = 1 + \frac{1}{2}\left( 1 + \frac{1}{2} \right) + \frac{1}{3}\left( 1 + \frac{1}{2} + \frac{1}{3} \right) + \ldots + \frac{1}{n}\left( 1 + \frac{1}{2} + \ldots\frac{1}{n} \right), \end{array}
(1.6.103)
cn(3)=1+12(1+12(1+12))+13(1+12(1+12)+13(1+12+13))c_{n}^{(3)} = 1 + \frac{1}{2}\left( 1 + \frac{1}{2}\left( 1 + \frac{1}{2} \right) \right) + \frac{1}{3}\left( 1 + \frac{1}{2}\left( 1 + \frac{1}{2} \right) + \frac{1}{3}\left( 1 + \frac{1}{2} + \frac{1}{3} \right) \right)
+…1n(1+12(1+12)+13(1+12+13)+…+1n(1+12+…1n)),\begin{array}{r} + \ldots\frac{1}{n}\left( 1 + \frac{1}{2}\left( 1 + \frac{1}{2} \right) + \frac{1}{3}\left( 1 + \frac{1}{2} + \frac{1}{3} \right) + \ldots + \frac{1}{n}\left( 1 + \frac{1}{2} + \ldots\frac{1}{n} \right) \right), \end{array}
(1.6.104)

for which, re­peat­ing pat­terns of the se­quences can be ap­pre­ci­at­ed. Con­cern­ing the Roman har­mon­ic num­bers for n>0,j>0n > 0,j > 0, the fol­low­ing holds for cn(j)c_{n}^{(j)}

cn(j)=∑k=1n1kck(j−1),\begin{array}{r} c_{n}^{(j)} = \sum_{k = 1}^{n}\frac{1}{k}c_{k}^{(j - 1)}, \end{array}
(1.6.105)

and these har­mon­ic number se­quences demon­strate as­ymp­tot­ic be­hav­ior for cn(j)c_{n}^{(j)}, when n≥0n \geq 0, for the limit of cn(j)c_{n}^{(j)}, as jj ap­proach­es in­fin­i­ty,

limj→∞⁡cn(j)=n.\begin{array}{r} \lim_{j \rightarrow \infty}c_{n}^{(j)} = n. \end{array}
(1.6.106)

Fur­ther in­ter­est sur­round­ing the har­mon­ic num­bers is found in the an­a­lyt­ic re­la­tion­ship they have with the digam­ma func­tion ψ(0)(x)\psi^{(0)}(x), and the Euler-Mascheroni con­stant γ\gamma

Hk=γ+ψ(0)(k+1),\begin{array}{r} H_{k} = \gamma + \psi^{(0)}(k + 1), \end{array}
(1.6.107)

The digam­ma func­tion ψ(0)(x)\psi^{(0)}(x), is de­fined as the log­a­rith­mic de­riv­a­tive of the gamma func­tion

ψ(0)(x)=ddxln⁡(Γ(x)),\begin{array}{r} \psi^{(0)}(x) = \frac{d}{dx}\ln{\left( \Gamma(x) \right),} \end{array}
(1.6.108)

and for ψ(0)(k+1)\psi^{(0)}(k + 1), it be­comes the fol­low­ing as­ymp­tot­ic series

ψ(0)(k+1)=−γ+∑j=1∞kj(j+k).\begin{array}{r} \psi^{(0)}(k + 1) = - \gamma + \sum_{j = 1}^{\infty}\frac{k}{j(j + k)}. \end{array}
(1.6.109)

The pro­found link that the ex­po­nen­tial map­ping has with in­te­gra­tion is just as deep the one the log­a­rithm func­tion has with dif­fer­en­ti­a­tion. We end this sec­tion with a result that re­veals a beau­ti­ful con­nec­tion be­tween the har­mon­ic log­a­rithms and the ex­po­nen­tial map­ping. As we are aware, ln⁡(x)\ln(x) has the in­def­i­nite in­te­gral rep­re­sen­ta­tion

∫1x dx=ln⁡(x).\begin{array}{r} \int_{}^{}\frac{1}{x}\ dx = \ln(x). \end{array}
(1.6.110)

Taking suc­ces­sive in­te­grals of ln⁡(x)\ln(x), the fol­low­ing series emerges

ln⁡(x)+x(ln⁡(x)−1)+x22!(ln⁡(x)−1−12)+x33!(ln⁡(x)−1−12−13)+…,\begin{array}{r} \ln(x) + x\left( \ln(x) - 1 \right) + \frac{x^{2}}{2!}\left( \ln(x) - 1 - \frac{1}{2} \right) + \frac{x^{3}}{3!}\left( \ln(x) - 1 - \frac{1}{2} - \frac{1}{3} \right) + \ldots, \end{array}
(1.6.111)

which can be rep­re­sent­ed in the sum­ma­tion form

∑k=0∞xkk!(ln⁡(x)−Hk),\begin{array}{r} \sum_{k = 0}^{\infty}{\frac{x^{k}}{k!}\left( \ln(x) - H_{k} \right)}, \end{array}
(1.6.112)

for HkH_{k}, the kthk^{th} har­mon­ic number. The ex­po­nen­tial series ∑k=0∞xkk!\sum_{k = 0}^{\infty}\frac{x^{k}}{k!} con­verges, while the series ∑k=0∞(ln⁡(x)−Hk)\sum_{k = 0}^{\infty}\left( \ln(x) - H_{k} \right) does not con­verge. Since the rec­i­p­ro­cal fac­to­r­i­al func­tion ap­proach­es zero at a much faster rate than −Hk- H_{k} ap­proach­es −∞- \infty, the el­e­ment-by-el­e­ment prod­uct of the two series does con­verge

∑k=0∞xkn!(ln⁡(x)−Hk)=−ex(Γ(0,x)+γ).\begin{array}{r} \sum_{k = 0}^{\infty}{\frac{x^{k}}{n!}\left( \ln(x) - H_{k} \right)} = {- e}^{x}\left( \Gamma(0,x) + \gamma \right). \end{array}
(1.6.113)

This result is anal­o­gous to that found for the series fℂ−∞((0!θrm)dθrm)f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)d\theta_{r}^{m} \right), fℂ−∞((0!θrm)dr)f_{\mathbb{C}}^{- \infty}\left( \left( \frac{0!}{\theta_{r}^{m}} \right)dr \right) (1.6.89,90), where the in­com­plete gamma func­tion Γ(s,x)\Gamma(s,x) has the fol­low­ing in­te­gral rep­re­sen­ta­tion

Γ(s,x)=∫x∞ts−1e−tdt.\begin{array}{r} \Gamma(s,x) = \int_{x}^{\infty}{t^{s - 1}e^{- t}}dt. \end{array}
(1.6.114)

We plot below the func­tion −ex(Γ(0,x)+γ),{- e}^{x}\left( \Gamma(0,x) + \gamma \right),to see that the func­tion takes on com­plex values for x<0x < 0, where a phase tran­si­tion occurs at the "zero-point", where values of the func­tion go from real num­bers to com­plex num­bers. Like the log­a­rithm func­tion, a sin­gu­lar­i­ty exists at x=0x = 0, at which, the func­tion −ex(Γ(0,x)+γ)=−∞{- e}^{x}\left( \Gamma(0,x) + \gamma \right) = - \infty.

Figure
Figure 1.6.6 – The func­tion −ex(Γ(0,x)+γ){- e}^{x}\left( \Gamma(0,x) + \gamma \right).

For the equa­tion −ex(Γ(0,x)+γ){- e}^{x}\left( \Gamma(0,x) + \gamma \right), let x=ibx = ib, which, in terms of an imag­i­nary vari­able, gives us an in­fi­nite sum­ma­tion of in­te­grals, equal to

∑k=0∞(ib)kk!(ln⁡(ib)−Hk)=eib(Ci(b)−iSi(b)+ln⁡(ib)−ln⁡(b)−γ),\begin{array}{r} \sum_{k = 0}^{\infty}{\frac{(ib)^{k}}{k!}\left( \ln(ib) - H_{k} \right)} = e^{ib}\left( Ci(b) - iSi(b) + \ln(ib) - \ln(b) - \gamma \right), \end{array}
(1.6.115)

where Ci(b), Si(b)Ci(b),\ Si(b) are the cosine and sine in­te­grals,

Ci(b)=−∫b∞cos⁡(t)t dt,  Si(b)=−∫b∞sin⁡(t)t dt,\begin{array}{r} Ci(b) = - \int_{b}^{\infty}{\frac{\cos(t)}{t}\ dt},\ \ Si(b) = - \int_{b}^{\infty}{\frac{\sin(t)}{t}\ dt,} \end{array}
(1.6.116)

and the sum­ma­tion can also take more fa­mil­iar form

∑k=0∞(ib)kk!(ln⁡(ib)−Hk)=−eib(Γ(0,ib)+γ).\begin{array}{r} \sum_{k = 0}^{\infty}{\frac{(ib)^{k}}{k!}\left( \ln(ib) - H_{k} \right)} = - e^{ib}\left( \Gamma(0,ib) + \gamma \right). \end{array}
(1.6.117)

Plot­ting the func­tion −eib(Γ(0,ib)+γ)- e^{ib}\left( \Gamma(0,ib) + \gamma \right) (Figure 1.6.6), we can see real and imag­i­nary wave­forms em­a­nat­ing from the "zero-point" in both di­rec­tions, which is due to the in­flu­ence of the trigono­met­ric func­tions in the equa­tion.

Figure
Figure 1.6.7 – The func­tion −eib(Γ(0,ib)+γ)- e^{ib}\left( \Gamma(0,ib) + \gamma \right).

Next, we can set our vari­able to be com­plex, as z=(a+ib)z = (a + ib), which rep­re­sents the non-polar form of tan­gent space θr1,\theta_{r}^{1},whose in­te­gral sum­ma­tion equals

∑n=0∞(a+ib)nn!(ln⁡(a+ib)−Hn)=−ea+ib(Γ(0,a+ib)+γ).\begin{array}{r} \sum_{n = 0}^{\infty}{\frac{(a + ib)^{n}}{n!}\left( \ln(a + ib) - H_{n} \right)} = {- e}^{a + ib}\left( \Gamma(0,a + ib) + \gamma \right). \end{array}
(1.6.118)

We plot the com­plex-valued vari­able in­com­plete gamma func­tion por­tion from above, Γ(0,(a+ib))\Gamma\left( 0,(a + ib) \right), in Figure 1.6.7, find­ing a promi­nent sin­gu­lar­i­ty forms for the reals at a,b=0a,b = 0, due to the gamma func­tion's pole at zero, and in this case equals com­plex in­fin­i­ty ∞~\widetilde{\infty},

Γ(0,0)=Γ(0)=∞~.\begin{array}{r} \Gamma(0,0) = \Gamma(0) = \widetilde{\infty}. \end{array}
(1.6.119)
Figure 1.6.8 – Γ(0,(a+ib))\Gamma\left( 0,(a + ib) \right) real-valued (left), and imag­i­nary-valued (right).

Our con­sid­er­a­tions of the in­fi­nite sym­me­try group's tan­gent space, brings us to con­tem­plate the deeper con­structs of the har­mon­ic series, and the log­a­rithm, gamma, and digam­ma func­tions; all of which play promi­nent roles in number theory and the study of primes. In Part II, of Arith­moí-Math­e­mat­i­cal Foun­da­tions, we expand the study of har­mon­ic log­a­rithms into their higher and lower-order forms, to prove in detail that these in­fi­nite in­te­grals con­verge to the stated func­tions in this sec­tion. The har­mon­ic log­a­rithms are ex­tend­ed to the hyper-har­mon­ic log­a­rithm space, defin­ing the ex­ten­sive field of func­tions dis­tinct from the tan­gent spaces and their ex­po­nen­tial­ly ex­tend­ed forms. This func­tion­al space in­ter­re­lates with the Lie al­ge­bras and groups we have learned about, by their in­ter­twined dy­nam­ics, and opens the po­ten­tial for pro­found phys­i­cal and meta­phys­i­cal im­pli­ca­tions.

  1. Roman, Steven, "The Log­a­rith­mic Bi­no­mi­al For­mu­la", The Amer­i­can Math­e­mat­i­cal Month­ly, Vol. 99, No. 7 (Aug. - Sep. 1992)