<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">AM</journal-id><journal-title-group><journal-title>Applied Mathematics</journal-title></journal-title-group><issn pub-type="epub">2152-7385</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/am.2014.510151</article-id><article-id pub-id-type="publisher-id">AM-46594</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>COMPUTER SCIENCE &amp; COMMUNICATIONS</subject><subject>ENGINEERING</subject><subject>PHYSICS &amp; MATHEMATICS</subject></subj-group></article-categories><title-group><article-title>On q-Deformed Calculus in Quantum Geometry</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Olaniyi</surname><given-names>S. Maliki</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Emmanuel</surname><given-names>I. Ugwu</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Industrial Mathematics and Applied Statistics, Ebonyi State University, Abakaliki, Nigeria</addr-line></aff><aff id="aff2"><addr-line>Department of Industrial Physics, Ebonyi State University, Abakaliki, Nigeria</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>somaliki@yahoo.com(OSM)</email>;<email>ugwuei@yahoo.com(EIU)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>22</day><month>05</month><year>2014</year></pub-date><volume>05</volume><issue>10</issue><fpage>1586</fpage><lpage>1593</lpage><history><date date-type="received"><day>21</day>	<month>March</month>	<year>2014</year></date><date date-type="rev-recd"><day>21</day>	<month>April</month>	<year>2014</year>	</date><date date-type="accepted"><day>28</day>	<month>April</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
	The
relation between noncommutative (or quantum) geometry and themathematics of spacesis in many ways
similar to the relation between quantum physicsand classical physics. One moves from the commutative algebra of
functions on a space (or a commutative algebra of classical observable in
classical physics) to a noncommutative algebra representing a noncommutative
space (or a noncommutative algebra of
quantum observables in quantum physics). The object of this paper is to study
the basic rules governing <em>q</em>-calculus
as compared with the classical Newton-Leibnitz calculus.

</p></abstract><kwd-group><kwd>Quantum Geometry</kwd><kwd> &lt;i&gt;q&lt;/i&gt;-Numbers</kwd><kwd> &lt;i&gt;q&lt;/i&gt;-Factorials</kwd><kwd> &lt;i&gt;q&lt;/i&gt;-Calculus</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>There exists an intimate relationship between classical geometry and physics, and to appreciate this we will consider the Einstein field equations (EFE) of special relativity written as:</p><disp-formula id="scirp.46594-formula906"><label>(EFE)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\f7f3f18e-527f-4fdf-bb96-cde1a7d9aac0.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\c0877e13-c884-41b1-9d98-57d66f2e6288.png" xlink:type="simple"/></inline-formula> is the Einstein tensor, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\8c842146-cf2e-48cb-81b3-0f25945ac0af.png" xlink:type="simple"/></inline-formula>is the Ricci tensor. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e49b215f-1461-44fc-923c-151cbc4dd4f7.png" xlink:type="simple"/></inline-formula>is the energy-momen-</p><p>tum tensor.</p><p>For the moment we are only interested in three basic properties of the above equation.</p><p>1) The equation (EFE) is a tensor equation. This is necessarily so, since the principle of invariance under coordinate transformations must hold, in other words the equations of physics must look the same in any frame of reference.</p><p>2) We can interpret equation (EFE) more simply as</p><disp-formula id="scirp.46594-formula907"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b4b94e5e-fa1e-4f56-9117-c86492517fef.png"/></disp-formula><p>i.e. it is the presence of matter in space that distorts the neighbouring geometry. Most equations of mathematical physics can be interpreted similarly.</p><p>3) The solution to equation (EFE) is a geometrical object, namely a line element given by</p><disp-formula id="scirp.46594-formula908"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\360163d2-34d1-4b22-a2d8-a491db4566e9.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\9383052a-0893-43b8-b382-cf56c65725cb.png" xlink:type="simple"/></inline-formula> is the metric tensor to be solved for in (EFE).</p><sec id="s1_1"><title>1.1. Quantum Geometry</title><p>Every geometry is associated with some kind of space. Quantum (or noncommutative) geometry [<xref ref-type="bibr" rid="scirp.46594-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.46594-ref2">2</xref>] deals with quantum spaces, including the classical concept of space as a very special case. In classical geometry spaces are always regarded as collections of points equipped with the appropriate additional structure (as for example a topological structure given by the collection of open sets, or a smooth structure given by the atlas). In contrast to classical geometry, quantum spaces are not interpretable in this way. In general, quantum spaces have no points at all! They exhibit non-trivial quantum fluctuations’ of geometry at all scales.</p><p>In generalizing classical geometry to the non-commutative level, there are two important conceptual steps:</p><p>1) Translation of geometry into a commutative algebra format;</p><p>2) Non-commutative generalizations.</p></sec><sec id="s1_2"><title>1.2. Reformulating Basic Geometrical Concepts</title><p>It turns out that the geometrical structure on any given topological space X is always completely expressible in the language of some associated *-algebra [<xref ref-type="bibr" rid="scirp.46594-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.46594-ref4">4</xref>] .</p><p>Points</p><p> Let X be a compact topological space, and let </p><p> be the </p><p>-algebra of continuous complex-valued functions on X. Every element </p><p> naturally gives rise to a linear functional </p><p> defined by </p><disp-formula id="scirp.46594-formula909"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b79beef1-a774-4286-a241-8ae83ad1365e.png"/></disp-formula><p>This map is multiplicative in the sense that</p><disp-formula id="scirp.46594-formula910"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\01705ead-3bcf-428c-8969-228db3c1fbf2.png"/></disp-formula><p>Furthermore, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\d8762855-89a6-427e-b4da-a506e972222c.png" xlink:type="simple"/></inline-formula>is Hermitian in the sense that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1d9a17f3-5813-48b3-b75d-021f14a36aa3.png" xlink:type="simple"/></inline-formula> it is also non-zero, i.e. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1a489a7a-e968-42d1-b572-841329092a1c.png" xlink:type="simple"/></inline-formula>is a character</p><p>on A. Conversely, consider an arbitrary character<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\6d846494-fa84-4b74-89fe-156fd744cf64.png" xlink:type="simple"/></inline-formula>, then it can be shown that there exists a unique point <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\311c9202-6100-4466-b69e-f2d3fc6e2655.png" xlink:type="simple"/></inline-formula> such that<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\07fed966-11cf-40bc-a62f-54847cce7aec.png" xlink:type="simple"/></inline-formula>. In other words, we have a natural bijection between points of X and characters of A. It is important to note that this characterization of points also remains valid at the smooth level, in which X could be a compact smooth manifold and the associated *-algebra consists of smooth functions on X.</p></sec><sec id="s1_3"><title>1.3. The Gelfand-Naimark Theorem</title><p>The algebra <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e1ee97bc-ab7a-4034-bd65-7d770087adb5.png" xlink:type="simple"/></inline-formula> of complex-valued functions on a compact topological space X, equipped with the maximum norm</p><disp-formula id="scirp.46594-formula911"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\56681944-c5fd-43f4-b787-a1da8a799a81.png"/></disp-formula><p>is a commutative C<sup>*</sup>-algebra [<xref ref-type="bibr" rid="scirp.46594-ref2">2</xref>] . The classical theorem of Gelfand and Naimark characterizes the algebras of the form<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\bf56401a-fc0e-478a-887b-bbf68383b6c0.png" xlink:type="simple"/></inline-formula>, as commutative unital C<sup>*</sup>-algebras. This means that for every commutative unital C<sup>*</sup>-algebra</p><p>A there exists (up to homeomerphisms) a unique compact topological space X such that<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\7abb813f-8670-4a56-987f-8fd9af1f452d.png" xlink:type="simple"/></inline-formula>.</p><p>As we have earlier observed, the points of the space X are recovered as characters of the associated algebra A. In terms of this identification, the topology on X coincides with the weak<sup>*</sup>-topology, induced from the dual space<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\8c0f7e24-e8b6-4b55-aa93-f2b1b42e232c.png" xlink:type="simple"/></inline-formula>, consisting of continuous linear functionals on A. It turns out that homomorphisms between C<sup>*</sup>-algebras are automatically continuous, in particular characters are continuous linear functionals.</p></sec></sec><sec id="s2"><title>2. The Quantum Plane</title><p>A simple example of quantum geometry is the quantum plane (<xref ref-type="fig" rid="fig1">Figure 1</xref>). Usually, a plane is described by two coordinate functions x, y. Naturally, the functions xy and yx are the same since it does not matter whether you measure x first and then y or y first and then x. This is precisely what is lost in the quantum world.</p><p>In the quantum plane we replace the property <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\14c9f721-fe47-491c-b4d2-d354218fec5a.png" xlink:type="simple"/></inline-formula> by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\080d5f2e-b400-490c-aead-63ebc5a08ff1.png" xlink:type="simple"/></inline-formula> where q is some parameter. We no longer have points, however we can continue to work algebraically with x and y.</p><p>Define<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\a1b6ceec-3d30-43c1-a6b6-47a5a12eee21.png" xlink:type="simple"/></inline-formula>, the commutator bracket. Hence <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\6d7ea71b-2bf7-4acd-a0be-da8c9e1a2f96.png" xlink:type="simple"/></inline-formula> can be rewritten as</p><disp-formula id="scirp.46594-formula912"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\c6908e61-e601-41e6-bbf1-d1bd10e76434.png"/></disp-formula><p>The commutative case is obtained when<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5258f9e4-f281-4c1b-bea1-29be932c3cf6.png" xlink:type="simple"/></inline-formula>.</p><sec id="s2_1"><title>2.1. q-Deformed Calculus</title><p>It is interesting to know that one can really do geometry in this setting, where coordinates do not commute. This is the remarkable discovery in recent times. For example, we can follow the approach of Newton-Leibnitz defining differentiation by</p><disp-formula id="scirp.46594-formula913"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\0d10de8b-8f05-4382-8b74-1c99a7db3b44.png"/></disp-formula><p>But when <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\a7dedf3b-25b5-4134-80bd-548eaabd90ae.png" xlink:type="simple"/></inline-formula> and in particular <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b9e9e318-6c90-420d-b1a8-92b795cb6a0f.png" xlink:type="simple"/></inline-formula> we get instead</p><disp-formula id="scirp.46594-formula914"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5c1fe930-c79a-4ed5-8cdd-14ebb7124c38.png"/></disp-formula><p>Thus for example the derivative of the function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\d91b8409-dda1-4955-aef2-b515c4f2ce6a.png" xlink:type="simple"/></inline-formula> in this non-commutative setting would be</p><disp-formula id="scirp.46594-formula915"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5b9879ac-784c-40ef-bb67-543d46a412b5.png"/></disp-formula><p>We observe here that when <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\f255f5c2-e829-4169-9999-de949566c827.png" xlink:type="simple"/></inline-formula> the derivative of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\2b8d30ce-04ef-4197-b4bc-6eda934cbcb1.png" xlink:type="simple"/></inline-formula> for the commutative case is obtained, i.e.<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\bf214a6a-8394-4f31-8665-a794c1b808b1.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_2"><title>2.2. Basic Notions of q-Calculus</title><p>The mathematical study of noncommutative geometry is intimately related to the so-called q-calculus (q- numbers, q-factorials, q-differentials and integrals, basic q-hypergeometric functions, and q-orthogonal polynomials). Here we give a brief introduction to q-numbers and q-factorials which will be required in the subsequent sections.</p><sec id="s2_2_1"><title>2.2.1. q-Numbers and q-Factorials</title><p>For any nonzero complex number q, the q-number<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\d0adf99b-651c-474a-8773-58dddd1afde3.png" xlink:type="simple"/></inline-formula>, is defined by</p><disp-formula id="scirp.46594-formula916"><label>(2.1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b2cfc1ed-f6b5-49d2-a669-b1adc6a1a678.png"/></disp-formula><fig id="fig1"><label>Figure 1</label><caption><p> The quantum plane (xy ≠ yx)</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\af561034-c273-45ad-8e91-0d2b37410feb.png"/></fig><p>We observe that,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5bc3af97-2153-46f5-9838-9f85ee38329a.png" xlink:type="simple"/></inline-formula>. The following expression which is easily proved will prove useful.</p><disp-formula id="scirp.46594-formula917"><label>(2.2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\36c1c169-a184-42fa-a9f4-92f18394efa6.png"/></disp-formula><p>Thus given<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\98a8140f-49e6-431a-a7f1-083c2ef19b9f.png" xlink:type="simple"/></inline-formula>, as shown previously<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\f6305674-69e6-4829-b9b1-f6efe544e6a7.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_2_2"><title>2.2.2. Proposition</title><p>The q-numbers satisfy the following relations derived from the property of the exponential function</p><p>1) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\cb0c3166-0b72-4497-bd02-66db14a4ec7f.png" xlink:type="simple"/></inline-formula></p><p>2) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1f2e9c36-1ad2-4d39-a623-883fe1b93ff4.png" xlink:type="simple"/></inline-formula></p><p>3) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\0f4b5f0c-e361-4863-bcc3-8fdfb4027bd7.png" xlink:type="simple"/></inline-formula></p><p>4) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1f7310a7-a035-4de4-97ae-35d6e0016a7b.png" xlink:type="simple"/></inline-formula></p><p>5) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b75c84d4-70cf-4f5b-808d-ba065f1eebb3.png" xlink:type="simple"/></inline-formula></p><p>The proof of 1) is easy to see from the fact that;</p><disp-formula id="scirp.46594-formula918"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\4a1e6a1b-4df0-4f76-a89e-ec7ab53e5663.png"/></disp-formula><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5acf4346-c02f-444c-93a2-ff499e2f29ed.png" xlink:type="simple"/></inline-formula></p><p>Hence;</p><disp-formula id="scirp.46594-formula919"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\fe410751-4f34-44e3-969e-4452d557e05c.png"/></disp-formula><p>The rest of the identities can be proved similarly. It is important to note that the relations 1)-5) remain valid</p><p>when q is considered an indeterminate. Consequently any q-number<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\d768db35-5d47-413b-8468-a3c571019281.png" xlink:type="simple"/></inline-formula>, belongs to the space</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\f8b09305-8326-49a9-976c-88354208da30.png" xlink:type="simple"/></inline-formula>of Laurent polynomials [<xref ref-type="bibr" rid="scirp.46594-ref2">2</xref>] in q with integral coefficients.</p><p>Suppose<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\aeb0513f-e11c-43c8-bf35-17793eb45bfe.png" xlink:type="simple"/></inline-formula>, then we define the q-factorial <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e54426c8-cdbd-4f6f-b115-a41357a12afe.png" xlink:type="simple"/></inline-formula> by setting;</p><disp-formula id="scirp.46594-formula920"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\19591a03-80b6-42a3-aa20-e26768f2d93a.png"/></disp-formula><p>The following expression is quite useful in the theory of hypergeometric functions as well as in combinatorics.</p><disp-formula id="scirp.46594-formula921"><label>(2.3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\a92006b0-9849-4ccc-bc4b-1e2388fd2cce.png"/></disp-formula><p>It is now possible for us to relate the above with the q-factorials. We observe that;</p><disp-formula id="scirp.46594-formula922"><label>(2.4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\361129ee-fd8e-48d6-89b7-c3a7a6bc6971.png"/></disp-formula><p>From equation (2.3) we note that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\6a5a0cb5-5542-41d4-ac4f-827837889e28.png" xlink:type="simple"/></inline-formula> For<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\cc38e145-1ba2-47f0-877c-b1402d590c93.png" xlink:type="simple"/></inline-formula>, define</p><disp-formula id="scirp.46594-formula923"><label>(2.5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b1e31f77-3973-4453-927a-5e95c12dda63.png"/></disp-formula><p>which converges<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\22b9237e-6681-4e09-8cc5-c97a988238a7.png" xlink:type="simple"/></inline-formula>, and defines an analytic function on<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5202b4ab-ac64-4dbb-88a2-9404d7978fa9.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_2_3"><title>2.2.3. Proposition</title><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\f9a8d47e-084b-4d95-bc2c-3605f8d76ca9.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5687e779-7a6a-4bbf-b53d-877055f04720.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b6dbb08a-8439-4f17-8cf3-37efbb1108b7.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_2_4"><title>Proof</title><disp-formula id="scirp.46594-formula924"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\0e837d58-a3de-49a1-ab2b-c99501682cf0.png"/></disp-formula><p>Remark: We can also define and show that;</p><disp-formula id="scirp.46594-formula925"><label>(2.6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\9ab8b111-81a7-4242-8155-d8686eeac971.png"/></disp-formula></sec><sec id="s2_2_5"><title>2.2.4. q-Binomial Coefficients</title><p>The q-binomial coefficients are defined by the formula;</p><disp-formula id="scirp.46594-formula926"><label>(2.7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\318de98d-341d-4597-9a7c-bc23c4d7b594.png"/></disp-formula><p>Remark: There exist a close analogy between the classical binomial coefficients <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\ac5ecdd9-1ee8-482a-bc8f-1c3ba967f8c2.png" xlink:type="simple"/></inline-formula> and</p><p>their q-analogues. Many of the identities satisfied by the former have their counterparts for the q-binomial coefficients. For example the classical identity;</p><disp-formula id="scirp.46594-formula927"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\16f15d3b-a874-43f5-a91d-a0f5b08eb3ec.png"/></disp-formula><p>simply translates to;</p><disp-formula id="scirp.46594-formula928"><label>2.8</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\179461a7-b42c-43d5-bbb5-ca6e8536123f.png"/></disp-formula></sec><sec id="s2_2_6"><title>2.2.5. Proposition</title><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\0b02e5c2-29cc-4d3f-9f6c-03b2aeea9b50.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\7d225e11-839d-4005-a201-e7719e29f119.png" xlink:type="simple"/></inline-formula> be noncommuting variables satisfying the relation<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\cb9d79a1-3738-4ccc-bc77-cad0102dd51b.png" xlink:type="simple"/></inline-formula>, then we have</p><disp-formula id="scirp.46594-formula929"><label>(2.9)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1a69218b-3999-4376-8d41-2e9163cde476.png"/></disp-formula><p>In case q is a primitive p<sup>th</sup> root of unity, and p is odd, then</p><disp-formula id="scirp.46594-formula930"><label>(2.10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e8a0c19f-a460-49f6-a7e5-032f93f3f863.png"/></disp-formula></sec><sec id="s2_2_7"><title>Proof</title><p>Equation (2.9) can be established by induction on n, and employing the first identity in (2.8). The second assertion follows directly from (2.9). Observe that:</p><disp-formula id="scirp.46594-formula931"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\33534198-39a7-4aa6-9985-2fd1d16c66f7.png"/></disp-formula><p>From (2.7)</p><disp-formula id="scirp.46594-formula932"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\c51a5523-79d7-4b5b-bfa6-5bf8c108cc7a.png"/></disp-formula><p>and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\4978b23b-c812-4510-9616-5886cfa01073.png" xlink:type="simple"/></inline-formula>.</p></sec></sec></sec><sec id="s3"><title>3. q-Differential and q-Integral Operators</title><p>The following are important basic notions derived from their analogue in classical calculus, and will be employed subsequently.</p><sec id="s3_1"><title>3.1. The q-Differential Operator</title><p>For<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\a6b5e866-7178-4b84-b2ea-5ddda7af1fda.png" xlink:type="simple"/></inline-formula>, we define the q-differential operator <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\a5e6b377-f1bf-40b2-99c4-853d8c2a2956.png" xlink:type="simple"/></inline-formula> by:</p><disp-formula id="scirp.46594-formula933"><label>(3.1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\bb313bf1-493e-46c6-bf85-705654db75b3.png"/></disp-formula><p>Note that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\31a29d47-8987-45ce-af97-cbd15a5cd4da.png" xlink:type="simple"/></inline-formula> as<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\87dddc3a-412a-4c39-8c55-3047a0549eab.png" xlink:type="simple"/></inline-formula>.</p><sec id="s3_1_1"><title>Proposition:</title><disp-formula id="scirp.46594-formula934"><label>. (3.2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\57549a51-67a2-416e-b41d-0bb037e84454.png"/></disp-formula><p>Provided the expression on the right hand side exists.</p></sec><sec id="s3_1_2"><title>Proof</title><p>Let<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1618affd-67b5-474e-8c9d-50d3088d9024.png" xlink:type="simple"/></inline-formula>, then by Taylor’s series, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\7eec954f-4654-410b-b9ed-e8ec0a0cc666.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.46594-formula935"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\148ca994-6765-4a75-b5f7-9e9411a43638.png"/></disp-formula><p>Setting<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\89d05b7a-e939-47cf-b696-dbf0b12a5a46.png" xlink:type="simple"/></inline-formula>, we have:</p><disp-formula id="scirp.46594-formula936"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b7601716-c032-4de8-ac1a-269b7b8c0888.png"/></disp-formula><p>The formula for the product of two functions is given by</p><disp-formula id="scirp.46594-formula937"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\eea037fa-1d40-424e-ae0f-8906a69fd39d.png"/></disp-formula><p>We can now define the q-analogue of the Newton-Leibnitz rule:</p><disp-formula id="scirp.46594-formula938"><label>(3.3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\0add7ec8-8fac-45b5-a1ac-7aa21cd62897.png"/></disp-formula><p>Thus,</p><disp-formula id="scirp.46594-formula939"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e6b5e8c2-d5b9-437d-9261-11f96529a7fa.png"/></disp-formula><p>By induction on n, it follows from (3.3) that:</p><disp-formula id="scirp.46594-formula940"><label>(3.4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e0cd6822-28ac-40ec-892f-8a7bc892a2c2.png"/></disp-formula><p>As a special case when<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e373023d-f424-4c38-96af-b72036d96c2c.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\c86f6c4c-f4e4-4639-87f3-97d150b32818.png" xlink:type="simple"/></inline-formula>is evaluated to give:</p><disp-formula id="scirp.46594-formula941"><label>(3.5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\8cb74c81-5232-456c-aeda-12e66d857a85.png"/></disp-formula></sec></sec><sec id="s3_2"><title>3.2. The q-Integral Operator</title><p>The q-integral operator will be defined as the inverse of the q-differential operator.</p><p>Given<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\578ddafc-7364-4829-8599-ace1ed2f6203.png" xlink:type="simple"/></inline-formula>, we have:</p><disp-formula id="scirp.46594-formula942"><label>(3.6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\3c470045-b647-4285-9865-1c311cdd906a.png"/></disp-formula><p>It then follows that;<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\2622ce99-d6e0-4d3b-81af-36049f709c8b.png" xlink:type="simple"/></inline-formula>.</p><p>Hence, summing these relations over <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\479a1462-a50b-40ee-b624-0c48ba271606.png" xlink:type="simple"/></inline-formula> gives:</p><disp-formula id="scirp.46594-formula943"><label>(3.7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\06d1f29b-12e1-4218-8b1c-0f7553f098e0.png"/></disp-formula><p>Assuming <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\f24ca972-020d-4237-8734-2a74b548d4f1.png" xlink:type="simple"/></inline-formula> so that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\75121add-ba42-484e-ae52-3568d33ffcfd.png" xlink:type="simple"/></inline-formula> as<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\bd7259db-3c2b-4dde-b916-8e91a071a1c1.png" xlink:type="simple"/></inline-formula>, it follows that</p><disp-formula id="scirp.46594-formula944"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1f91544f-381e-4ba8-9ceb-043e114d494b.png"/></disp-formula><p>We can now formally define the q-integral of a function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\c6e1f508-41fc-41d2-adea-2340f37ef872.png" xlink:type="simple"/></inline-formula> on a given interval <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\afd00167-c5f4-41d6-931a-f844af1569cf.png" xlink:type="simple"/></inline-formula> as</p><disp-formula id="scirp.46594-formula945"><label>(3.8)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\e1bf7249-ce0a-4fc2-983b-9f6fc579e4bb.png"/></disp-formula><p>On the semi-infinite interval<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b0ba780f-8ec2-4555-bcd1-66256ba29680.png" xlink:type="simple"/></inline-formula>, the q-integral of a function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\0f9492f6-8ca2-4153-b93d-0563eafa6a43.png" xlink:type="simple"/></inline-formula> is defined as:</p><disp-formula id="scirp.46594-formula946"><label>(3.9)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\6c29af4b-1ba4-4614-a265-44cb7207cfc0.png"/></disp-formula><p>Over any closed interval<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\593fdabe-e213-4802-8b64-e41d1e6e00e7.png" xlink:type="simple"/></inline-formula>, the q-integral of a function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\1d214bc6-1b6a-44c7-8226-d8dde9265539.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.46594-formula947"><label>(3.10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\b390b2bd-f369-4c6d-8b09-e5608d85475c.png"/></disp-formula><p>We now define the integral over the interval<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\210da45e-3acb-4044-ac1b-306a4beba269.png" xlink:type="simple"/></inline-formula>. This is achieved by setting <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\5a79bdc2-79ae-4666-8c96-dd8f6982c27c.png" xlink:type="simple"/></inline-formula> in equations (3.8) and (3.9) and summing to get:</p><disp-formula id="scirp.46594-formula948"><label>(3.11)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\909dab97-1d4b-43de-8f69-650d95d0c988.png"/></disp-formula><p>The integration by parts formula of Newton-Leibnitz calculus is interpreted in the present noncommutative context as:</p><disp-formula id="scirp.46594-formula949"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\21-7401928x\0dc572f6-6d4f-4afa-aeeb-070a1a55152f.png"/></disp-formula></sec></sec><sec id="s4"><title>4. Application</title><p>There are a number of applications of the foregoing, we mention here just two, namely:</p><p>1) q-binomial formulae in two variables satisfying a quadratic relation, this has recently been published in [<xref ref-type="bibr" rid="scirp.46594-ref5">5</xref>] and [<xref ref-type="bibr" rid="scirp.46594-ref6">6</xref>] . These relations have applications in quantum group theory and non-commutative geometry.</p><p>2) A recent trend in modern physics is the study of the quantum anti-de Sitter space [<xref ref-type="bibr" rid="scirp.46594-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.46594-ref8">8</xref>] possibly in connection with q = root of unity [<xref ref-type="bibr" rid="scirp.46594-ref9">9</xref>] .</p></sec><sec id="s5"><title>Acknowledgements</title><p>This work began at the African Institute for mathematical sciences (AIMS) in Muizenberg South Africa, when the first author visited in 2010. 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