What Is Q-Calculus?

Total Page:16

File Type:pdf, Size:1020Kb

What Is Q-Calculus? What is q-Calculus? Anthony Ciavarella July 1, 2016 Abstract In this talk, I will present a q-analog of the classical derivative from calculus. From there, I will prove q-analogs of the binomial theorem and Taylor's theorem. If time permits, I will show some applications of the q-calculus in number theory and physics. 1 q-Derivative In classical calculus we define the derivative of a function f to be df f(x + h) − f(x) = lim dx h!0 h Equivalently, we could define the derivative to be df f(qx) − f(x) = lim dx q!1 qx − x Now one might wonder, what happens when we don't take the limit, and just use the expression inside the limit as the definition of our derivative. This leads us into the exciting world of quantum calculus, also known as q-calculus. Definition 1.1. q −differential :A q −differential of a function f is defined to be dqf = f(qx) − f(x). From here, we can define our q − derivative to be d f f(qx) − f(x) q = dqx qx − x Now for an example, d qnxn − xn qn − 1 q (xn) = = xn−1 dqx qx − x q − 1 d n n−1 Comparing this to the classical result, dx (x ) = nx , we can define a q- qn−1 dn n dk n analog of a number to be [n] = q−1 . Comparing dxn (x ) = n! and dxk (x ) = n n−k k k!x to their q-analogs motivates the following two definitions. 1 Definition 1.2. q −factorial :A q −factorial of a natural number n is defined to be [n]! = [n] × [n − 1] × ::: × [1] if n > 0 and 1 if n = 0. Definition 1.3. q − factorial : For natural numbers n and k, the q-factorial is n [n]! defined to be k = [k]![n−k]! . 2 Taylor's Theorem Now that we have a q-derivative, it is reasonable to wonder if there are the- orems analogous to those from classical calculus. In fact, there is a q-analog of Taylor's theorem, but before proving it we are going to restate the classical Taylor theorem in a slightly weaker form. Theorem 2.1 (Taylor's theorem). Let P0;P1; :::; PN be polynomials and a be a number such that: (1) P0(a) = 1 and Pn(a) = 0 for n ≥ 1. (2) deg(Pn) = n. d (3) dx Pn(x) = Pn−1(x) for n ≥ 1 Then any polynomial f of degree n can be written in the form N X dnf f(x) = Pn(x) dxn x=a n=0 Proof. Let V be the vector space of polynomials of degree ≤ N. The polyno- mials P0; ::; PN are linearly independent by (2) since their degrees are strictly PN increasing. So they form a basis of V, and we have f = n=1 cnPn. Now to solve for ck, we will differentiate k times and evaluate at a. N N dkf X dk X = cn( Pn) = cnPn−k(a) = ck dxk x=a dxk x=a n=1 n=k Now that we have Taylor's theorem in a different form, we can state the q-analog of Taylor's theorem. Theorem 2.2 (q-Taylor's theorem). Let P0;P1; :::; PN be polynomials and a be a number such that: (1) P0(a) = 1 and Pn(a) = 0 for n ≥ 1. (2) deg(Pn) = n. dq (3) Pn(x) = Pn−1(x) for n ≥ 1 dq x Then any polynomial f of degree n can be written in the form N n X dq f f(x) = Pn(x) d xn x=a n=0 q 2 Proof. The proof is identical to the proof of Theorem 2.1. Although we now have the q-analog of Taylor's theorem, we still need to (x−a)n find the polynomials Pn. Naively one would expect Pn(x) = [n]! by analogy with the classical case, but these polynomials fail to satisfy condition (3). From conditions (1) and (2), we must have P0 = 1. In order to satisfy all of the 2 dq 2 x conditions we must then have P1 = x − a. Since x = [2]x, P2 = − ax − dq x [2] a2 2 (x−a)(x−qa) [2] + a = [2] satisfies the necessary conditions. Assuming this trend Qn−1 k k=0 (x−q a) continues, a reasonable guess would be Pn = [n]! . To simplify notation, we will introduce the q-analog of (x − a)n Definition 2.1. q-analog of (x − a)n: The q-analog of (x − a)n is defined to be n Qn−1 k (x − a)q = k=0 (x − q a). Before proving that these Pn satisfies the conditions in the q-Taylor's theo- rem, we will need the following lemma. Lemma 2.3 (q-Product Rule). d d g d f q (f(x)g(x)) = f(qx) q + g(x) q dqx dqx dqx Proof. dq(f(x)g(x)) = f(qx)g(qx) − f(x)g(x) = f(qx)g(qx) − f(qx)g(x) + f(qx)g(x) − f(x)g(x) = f(qx)dqg(x) + g(x)dqf(x) (1) d (f(x)g(x)) d g d f q = f(qx) q + g(x) q dqx dqx dqx I would like to point out that this expression is symmetric in f and g, however the symmetry is hidden in the definition of the q-derivative. Theorem 2.4. dq (x − a)n = [n](x − a)n−1 dq x q q Proof. For n = 1 this is clearly true. Suppose this theorem holds for n − 1, then we have n n−1 n−1 (x − a)q = (x − a)q (x − q a) Using the product rule, dq n n−1 n−1 dq n−1 (x − a)q = (x − a)q + (qx − q a) (x − a)q dqx dqx dq n n−1 n−2 n−2 (x − a)q = (x − a)q + q(x − q a)[n − 1](x − a)q dqx 3 dq n n−1 n−1 (x − a)q = (1 + q[n − 1])(x − a)q = [n](x − a)q dqx So the theorem, holds 8n 2 N S 0 by induction. n At this point, I would like to note that the definition of (x + a)q can be ex- −n 1 tended to negative integers with the following definition, (x−a)q = −n n . (x−q a)q 3 Binomial Theorem and Euler's Identities Now that we have the q-Taylor's theorem, we can use it to prove two q-analogs of the binomial theorem. Theorem 3.1 (Gauss' Binomial Theorem). n n X k(k−1) n k n−k (x + a) = q 2 a x q k k=0 Note: This expression is not symmetric in x and a, because the second value will be multiplied by some powers of q. Proof. k dq n n−k k (1 + x)q = [n][n − 1]:::[n − k + 1](1 + x)q dqx (n−k)(n−k−1) n−k n−k−1 2 n−k−1 n−k 2 n−k (0+a)q = (a+0)(qa+0):::(q a) = 1×q×q ×:::×q ×a = q a Using the q-Taylor's theorem we have n n X (n−k)(n−k−1) n n−k k (x + a) = q 2 a x q n − k k=0 When we replace k with n − k as the variable of summation,, this simplifies to n n X k(k−1) n k n−k (x + a) = q 2 a x q k k=0 n n Since n−k = k . Theorem 3.2 (Heine's Binomial Theorem). 1 1 X [n][n − 1]:::[n − k + 1] = xk (1 − x)n [k]! q k=0 Note: this equality holds as an equivalence of formal power series so issues of convergence are ignored. 4 Proof. The proof of this theorem is completely analogous to the proof of Gauss's binomial theorem and can be found in full in Kac's textbook Quantum Calculus. Now that we have these two formulas, one might wonder what happens in the limit where n goes to infinity. In the classical case, both sides go to infinity and we extract no new information, however this is not so in the quantum case. Theorem 3.3 (Euler's Identities). 1 1 k Y k 1 X k(k−1) x (1 + q x) = (1 + x) = q 2 q (1 − q)(1 − q2):::(1 − qk) k=0 k=0 1 1 Y 1 1 X xk = = (1 − qkx) (1 − x)1 (1 − q)(1 − q2):::(1 − qk) k=0 q k=0 for jqj < 1. Proof. We have qn − 1 1 lim [n] = lim ( ) = n!1 n!1 q − 1 1 − q when jqj < 1. And n (qn − 1)(qn−1 − 1):::(qn−k+1 − 1) 1 lim = lim = n!1 k n!1 (q − 1)(q2 − 1):::(qk − 1) (1 − q)(1 − q2):::(1 − qk) Plugging these two results into Gauss' and Heine's binomial theorems gives us the desired identities. 4 Applications The two Euler identites derived using the q-calculus have many applications in number theory. A few of them will be listed here and the proofs can be found in Victor Kac's textbook Quantum Calculus. Definition 4.1. The classical partition function p(n) is defined to be the num- ber of ways that a positive integer n can be written as a sum of positive integers, 1 if n = 0 and 0 if n < 0.
Recommended publications
  • Edward Close Response IQNJ Nccuse V5.2 ED 181201
    One Response to “An Evaluation of TDVP” With Explanations of Fundamental Concepts Edward R. Close, PhD, PE, DF (ECA), DSPE) and With Vernon M Neppe, MD, PhD, Fellow Royal Society (SA), DPCP (ECA), DSPE a b ABSTRACT Dr. Vernon M. Neppe and I first published an innovative, consciousness-based paradigm in a volume entitled Reality Begins with Consciousness in 2012.1 It was the combination of many years of independent research by us, carried out before we met, and then initially about 3 years of direct collaboration, that has now stretched beyond a decade. Hailed by some peer reviewers as the next major paradigm shift, the Triadic Dimensional Vortical Paradigm (TDVP) has been further developed and expanded over the past seven years in a number of papers and articles published outside of mainstream scientific journals because of the unspoken taboo against including consciousness in mathematical physics. This article is a response to criticisms leveled in the article, “An Evaluation of TDVP,” published in Telicom XXX, no. 5 (Oct-Dec 2018), by physicists J. E. F. Kaan and Simon Olling Rebsdorf.2 This article, along with Dr. Neppe’s rejoinder (which immediately follows this article), underlines the difficulty that mainstream scientists have had in understanding the basics and implications of TDVP. In addition to replying to the criticisms in Kaan and Rebsdorf’s article, this article contains explanations of some of the basic ideas that make TDVP a controversial shift from materialistic physicalism to a comprehensive consciousness-based scientific paradigm. 1.0 INTRODUCTION a Dr. Close PhD, DPCP (ECAO), DSPE is a Physicist, Mathematician, Cosmologist, Environmental Engineer and Dimensional Biopsychophysicist.
    [Show full text]
  • Notes on Euler's Work on Divergent Factorial Series and Their Associated
    Indian J. Pure Appl. Math., 41(1): 39-66, February 2010 °c Indian National Science Academy NOTES ON EULER’S WORK ON DIVERGENT FACTORIAL SERIES AND THEIR ASSOCIATED CONTINUED FRACTIONS Trond Digernes¤ and V. S. Varadarajan¤¤ ¤University of Trondheim, Trondheim, Norway e-mail: [email protected] ¤¤University of California, Los Angeles, CA, USA e-mail: [email protected] Abstract Factorial series which diverge everywhere were first considered by Euler from the point of view of summing divergent series. He discovered a way to sum such series and was led to certain integrals and continued fractions. His method of summation was essentialy what we call Borel summation now. In this paper, we discuss these aspects of Euler’s work from the modern perspective. Key words Divergent series, factorial series, continued fractions, hypergeometric continued fractions, Sturmian sequences. 1. Introductory Remarks Euler was the first mathematician to develop a systematic theory of divergent se- ries. In his great 1760 paper De seriebus divergentibus [1, 2] and in his letters to Bernoulli he championed the view, which was truly revolutionary for his epoch, that one should be able to assign a numerical value to any divergent series, thus allowing the possibility of working systematically with them (see [3]). He antic- ipated by over a century the methods of summation of divergent series which are known today as the summation methods of Cesaro, Holder,¨ Abel, Euler, Borel, and so on. Eventually his views would find their proper place in the modern theory of divergent series [4]. But from the beginning Euler realized that almost none of his methods could be applied to the series X1 1 ¡ 1!x + 2!x2 ¡ 3!x3 + ::: = (¡1)nn!xn (1) n=0 40 TROND DIGERNES AND V.
    [Show full text]
  • Calculus Terminology
    AP Calculus BC Calculus Terminology Absolute Convergence Asymptote Continued Sum Absolute Maximum Average Rate of Change Continuous Function Absolute Minimum Average Value of a Function Continuously Differentiable Function Absolutely Convergent Axis of Rotation Converge Acceleration Boundary Value Problem Converge Absolutely Alternating Series Bounded Function Converge Conditionally Alternating Series Remainder Bounded Sequence Convergence Tests Alternating Series Test Bounds of Integration Convergent Sequence Analytic Methods Calculus Convergent Series Annulus Cartesian Form Critical Number Antiderivative of a Function Cavalieri’s Principle Critical Point Approximation by Differentials Center of Mass Formula Critical Value Arc Length of a Curve Centroid Curly d Area below a Curve Chain Rule Curve Area between Curves Comparison Test Curve Sketching Area of an Ellipse Concave Cusp Area of a Parabolic Segment Concave Down Cylindrical Shell Method Area under a Curve Concave Up Decreasing Function Area Using Parametric Equations Conditional Convergence Definite Integral Area Using Polar Coordinates Constant Term Definite Integral Rules Degenerate Divergent Series Function Operations Del Operator e Fundamental Theorem of Calculus Deleted Neighborhood Ellipsoid GLB Derivative End Behavior Global Maximum Derivative of a Power Series Essential Discontinuity Global Minimum Derivative Rules Explicit Differentiation Golden Spiral Difference Quotient Explicit Function Graphic Methods Differentiable Exponential Decay Greatest Lower Bound Differential
    [Show full text]
  • Euler and His Work on Infinite Series
    BULLETIN (New Series) OF THE AMERICAN MATHEMATICAL SOCIETY Volume 44, Number 4, October 2007, Pages 515–539 S 0273-0979(07)01175-5 Article electronically published on June 26, 2007 EULER AND HIS WORK ON INFINITE SERIES V. S. VARADARAJAN For the 300th anniversary of Leonhard Euler’s birth Table of contents 1. Introduction 2. Zeta values 3. Divergent series 4. Summation formula 5. Concluding remarks 1. Introduction Leonhard Euler is one of the greatest and most astounding icons in the history of science. His work, dating back to the early eighteenth century, is still with us, very much alive and generating intense interest. Like Shakespeare and Mozart, he has remained fresh and captivating because of his personality as well as his ideas and achievements in mathematics. The reasons for this phenomenon lie in his universality, his uniqueness, and the immense output he left behind in papers, correspondence, diaries, and other memorabilia. Opera Omnia [E], his collected works and correspondence, is still in the process of completion, close to eighty volumes and 31,000+ pages and counting. A volume of brief summaries of his letters runs to several hundred pages. It is hard to comprehend the prodigious energy and creativity of this man who fueled such a monumental output. Even more remarkable, and in stark contrast to men like Newton and Gauss, is the sunny and equable temperament that informed all of his work, his correspondence, and his interactions with other people, both common and scientific. It was often said of him that he did mathematics as other people breathed, effortlessly and continuously.
    [Show full text]
  • On the Euler Integral for the Positive and Negative Factorial
    On the Euler Integral for the positive and negative Factorial Tai-Choon Yoon ∗ and Yina Yoon (Dated: Dec. 13th., 2020) Abstract We reviewed the Euler integral for the factorial, Gauss’ Pi function, Legendre’s gamma function and beta function, and found that gamma function is defective in Γ(0) and Γ( x) − because they are undefined or indefinable. And we came to a conclusion that the definition of a negative factorial, that covers the domain of the negative space, is needed to the Euler integral for the factorial, as well as the Euler Y function and the Euler Z function, that supersede Legendre’s gamma function and beta function. (Subject Class: 05A10, 11S80) A. The positive factorial and the Euler Y function Leonhard Euler (1707–1783) developed a transcendental progression in 1730[1] 1, which is read xedx (1 x)n. (1) Z − f From this, Euler transformed the above by changing e to g for generalization into f x g dx (1 x)n. (2) Z − Whence, Euler set f = 1 and g = 0, and got an integral for the factorial (!) 2, dx ( lx )n, (3) Z − where l represents logarithm . This is called the Euler integral of the second kind 3, and the equation (1) is called the Euler integral of the first kind. 4, 5 Rewriting the formula (3) as follows with limitation of domain for a positive half space, 1 1 n ln dx, n 0. (4) Z0 x ≥ ∗ Electronic address: [email protected] 1 “On Transcendental progressions that is, those whose general terms cannot be given algebraically” by Leonhard Euler p.3 2 ibid.
    [Show full text]
  • Quantum Riemannian Geometry of Phase Space and Nonassociativity
    Demonstr. Math. 2017; 50: 83–93 Demonstratio Mathematica Open Access Research Article Edwin J. Beggs and Shahn Majid* Quantum Riemannian geometry of phase space and nonassociativity DOI 10.1515/dema-2017-0009 Received August 3, 2016; accepted September 5, 2016. Abstract: Noncommutative or ‘quantum’ differential geometry has emerged in recent years as a process for quantizing not only a classical space into a noncommutative algebra (as familiar in quantum mechanics) but also differential forms, bundles and Riemannian structures at this level. The data for the algebra quantisation is a classical Poisson bracket while the data for quantum differential forms is a Poisson-compatible connection. We give an introduction to our recent result whereby further classical data such as classical bundles, metrics etc. all become quantised in a canonical ‘functorial’ way at least to 1st order in deformation theory. The theory imposes compatibility conditions between the classical Riemannian and Poisson structures as well as new physics such as n typical nonassociativity of the differential structure at 2nd order. We develop in detail the case of CP where the i j commutation relations have the canonical form [w , w¯ ] = iλδij similar to the proposal of Penrose for quantum twistor space. Our work provides a canonical but ultimately nonassociative differential calculus on this algebra and quantises the metric and Levi-Civita connection at lowest order in λ. Keywords: Noncommutative geometry, Quantum gravity, Poisson geometry, Riemannian geometry, Quantum mechanics MSC: 81R50, 58B32, 83C57 In honour of Michał Heller on his 80th birthday. 1 Introduction There are today lots of reasons to think that spacetime itself is better modelled as ‘quantum’ due to Planck-scale corrections.
    [Show full text]
  • List of Mathematical Symbols by Subject from Wikipedia, the Free Encyclopedia
    List of mathematical symbols by subject From Wikipedia, the free encyclopedia This list of mathematical symbols by subject shows a selection of the most common symbols that are used in modern mathematical notation within formulas, grouped by mathematical topic. As it is virtually impossible to list all the symbols ever used in mathematics, only those symbols which occur often in mathematics or mathematics education are included. Many of the characters are standardized, for example in DIN 1302 General mathematical symbols or DIN EN ISO 80000-2 Quantities and units – Part 2: Mathematical signs for science and technology. The following list is largely limited to non-alphanumeric characters. It is divided by areas of mathematics and grouped within sub-regions. Some symbols have a different meaning depending on the context and appear accordingly several times in the list. Further information on the symbols and their meaning can be found in the respective linked articles. Contents 1 Guide 2 Set theory 2.1 Definition symbols 2.2 Set construction 2.3 Set operations 2.4 Set relations 2.5 Number sets 2.6 Cardinality 3 Arithmetic 3.1 Arithmetic operators 3.2 Equality signs 3.3 Comparison 3.4 Divisibility 3.5 Intervals 3.6 Elementary functions 3.7 Complex numbers 3.8 Mathematical constants 4 Calculus 4.1 Sequences and series 4.2 Functions 4.3 Limits 4.4 Asymptotic behaviour 4.5 Differential calculus 4.6 Integral calculus 4.7 Vector calculus 4.8 Topology 4.9 Functional analysis 5 Linear algebra and geometry 5.1 Elementary geometry 5.2 Vectors and matrices 5.3 Vector calculus 5.4 Matrix calculus 5.5 Vector spaces 6 Algebra 6.1 Relations 6.2 Group theory 6.3 Field theory 6.4 Ring theory 7 Combinatorics 8 Stochastics 8.1 Probability theory 8.2 Statistics 9 Logic 9.1 Operators 9.2 Quantifiers 9.3 Deduction symbols 10 See also 11 References 12 External links Guide The following information is provided for each mathematical symbol: Symbol: The symbol as it is represented by LaTeX.
    [Show full text]
  • Leonhard Euler English Version
    LEONHARD EULER (April 15, 1707 – September 18, 1783) by HEINZ KLAUS STRICK , Germany Without a doubt, LEONHARD EULER was the most productive mathematician of all time. He wrote numerous books and countless articles covering a vast range of topics in pure and applied mathematics, physics, astronomy, geodesy, cartography, music, and shipbuilding – in Latin, French, Russian, and German. It is not only that he produced an enormous body of work; with unbelievable creativity, he brought innovative ideas to every topic on which he wrote and indeed opened up several new areas of mathematics. Pictured on the Swiss postage stamp of 2007 next to the polyhedron from DÜRER ’s Melencolia and EULER ’s polyhedral formula is a portrait of EULER from the year 1753, in which one can see that he was already suffering from eye problems at a relatively young age. EULER was born in Basel, the son of a pastor in the Reformed Church. His mother also came from a family of pastors. Since the local school was unable to provide an education commensurate with his son’s abilities, EULER ’s father took over the boy’s education. At the age of 14, EULER entered the University of Basel, where he studied philosophy. He completed his studies with a thesis comparing the philosophies of DESCARTES and NEWTON . At 16, at his father’s wish, he took up theological studies, but he switched to mathematics after JOHANN BERNOULLI , a friend of his father’s, convinced the latter that LEONHARD possessed an extraordinary mathematical talent. At 19, EULER won second prize in a competition sponsored by the French Academy of Sciences with a contribution on the question of the optimal placement of a ship’s masts (first prize was awarded to PIERRE BOUGUER , participant in an expedition of LA CONDAMINE to South America).
    [Show full text]
  • Math 63: Winter 2021 Lecture 17
    Math 63: Winter 2021 Lecture 17 Dana P. Williams Dartmouth College Monday, February 15, 2021 Dana P. Williams Math 63: Winter 2021 Lecture 17 Getting Started 1 We should be recording. 2 Remember it is better for me if you have your video on so that I don't feel I'm just talking to myself. 3 Our midterm will be available Friday after class and due Sunday by 10pm. It will cover through Today's lecture. More details soon. 4 Time for some questions! Dana P. Williams Math 63: Winter 2021 Lecture 17 Rules To Differentiate With The following are routine consequences of the definition. Lemma If f (x) = c for all x 2 R, then f 0(x) = 0 for all x 2 R. If f (x) = x for all x 2 R, then f 0(x) = 1 for all x 2 R. Theorem Suppose that f and g are differentiable at x0. Then so are f ± g, f fg, and if g(x0) 6= 0, g . Futhermore, 0 0 0 1 (f ± g) (x0) = f (x0) ± g (x0), 0 0 0 2 (fg) (x0) = f (x0)g(x0) + f (x0)g (x0), and 0 f 0(x )g(x )−f (x )g 0(x ) 3 f 0 0 0 0 (x0) = 2 . g g(x0) Dana P. Williams Math 63: Winter 2021 Lecture 17 More Formulas Corollary Suppose that f is differentiable at x0 and c 2 R. Then cf is 0 0 differentiable at x0 and (cf ) (x0) = cf (x0). Corollary Suppose that n 2 Z and f (x) = xn.
    [Show full text]
  • Classical/Quantum Dynamics in a Uniform Gravitational Field: A
    Classical/Quantum Dynamics in a Uniform Gravitational Field: A. Unobstructed Free Fall Nicholas Wheeler, Reed College Physics Department August 2002 Introduction. Every student of mechanics encounters discussion of the idealized one-dimensional dynamical systems 0:free particle F (x)=mx¨ with F (x)= −mg : particle in free fall −kx : harmonic oscillator at a very early point in his/her education, and with the first & last of those systems we are never done: they are—for reasons having little to do with their physical importance—workhorses of theoretical mechanics, traditionally employed to illustrated formal developments as they emerge, one after another. But—unaccountably—the motion of particles in uniform gravitational fields1 is seldom treated by methods more advanced than those accessible to beginning students. It is true that terrestrial gravitational forces are so relatively weak that they can—or could until recently—usually be dismissed as irrelevant to the phenomenology studied by physicists in their laboratories.2 But the free fall 1 It is to avoid that cumbersome phrase that I adopt the “free fall” locution, though technically free fall presumes neither uniformity nor constancy of the ambient gravitational field. If understood in the latter sense, “free fall” lies near the motivating heart of general relativity, which is certainly not a neglected subject. 2 There are exceptions: I am thinking of experiments done several decades ago where neutron diffraction in crystals was found to be sensitive to the value of g. And of experiments designed to determine whether antiparticles “fall up” (they don’t). 2 Classical/quantum motion in a uniform gravitational field: free fall problem—especially if construed quantum mechanically, with an eye to the relation between the quantum physics and classical physics—is itself a kind of laboratory, one in which striking clarity can be brought to a remarkable variety of formal issues.
    [Show full text]
  • Quantum Trajectories, State Diffusion and Time Asymmetric Eventum Mechanics
    QUANTUM TRAJECTORIES, STATE DIFFUSION AND TIME ASYMMETRIC EVENTUM MECHANICS V P BELAVKIN Abstract. We show that the quantum stochastic Langevin model for contin- uous in time measurements provides an exact formulation of the Heisenberg uncertainty error-disturbance principle. Moreover, as it was shown in the 80’s, this Markov model induces all stochastic linear and non-linear equations of the phenomenological "quantum trajectories" such as quantum state di¤usion and spontaneous localization by a simple quantum …ltering method. Here we prove that the quantum Langevin equation is equivalent to a Dirac type boundary- value problem for the second-quantized input ”o¤er waves from future”in one extra dimension, and to a reduction of the algebra of the consistent histories of past events to an Abelian subalgebra for the “trajectories of the output particles”. This result supports the wave-particle duality in the form of the thesis of Eventum Mechanics that everything in the future is constituted by quantized waves, everything in the past by trajectories of the recorded parti- cles. We demonstrate how this time arrow can be derived from the principle of quantum causality for nondemolition continuous in time measurements. 1. Introduction Quantum mechanics itself, whatever its interpretation, does not ac- count for the transition from ‘possible to the actual’ - Heisenberg. Schrödinger believed that all problems of interpretation of quantum mechanics including the above problem for time arrow should be formulated in continuous time in the form of di¤erential equations. He thought that the quantum jump problem would have been resolved if quantum mechanics had been made consistent with relativity theory of events and the time had been treated appropriately as a future – past boundary value problem of a microscopic information dynamics.
    [Show full text]
  • Summation of Divergent Power Series by Means of Factorial Series
    Summation of divergent power series by means of factorial series Ernst Joachim Weniger Institut f¨ur Physikalische und Theoretische Chemie, Universit¨at Regensburg, D-93040 Regensburg, Germany Abstract Factorial series played a major role in Stirling’s classic book Methodus Differentialis (1730), but now only a few specialists still use them. This article wants to show that this neglect is unjustified, and that factorial series are useful numerical tools for the summation of divergent (inverse) power series. This is documented by summing the divergent asymptotic expansion for the exponential integral E1(z) and the factorially divergent Rayleigh-Schr¨odinger perturba- tion expansion for the quartic anharmonic oscillator. Stirling numbers play a key role since they occur as coefficients in expansions of an inverse power in terms of inverse Pochhammer symbols and vice versa. It is shown that the relationships involving Stirling numbers are special cases of more general orthogonal and triangular transformations. Keywords: Factorial series; Divergent asymptotic (inverse) power series; Stieltjes series; Quartic anharmonic oscillator; Stirling numbers; General orthogonal and triangular transformations; 2010 MSC: 11B73; 40A05; 40G99; 81Q15; 1. Introduction Power series are extremely important analytical tools not only in mathematics, but also in the mathematical treat- ment of scientific and engineering problems. Unfortunately, a power series representation for a given function is from a numerical point of view a mixed blessing. A power series converges within its circle of convergence and diverges outside. Circles of convergence normally have finite radii, but there are many series expansions of consider- able practical relevance, for example asymptotic expansions for special functions or quantum mechanical perturbation expansions, whose circles of convergence shrink to a single point.
    [Show full text]