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An Amazing Prime Heuristic.Pdf
This document has been moved to https://arxiv.org/abs/2103.04483 Please use that version instead. AN AMAZING PRIME HEURISTIC CHRIS K. CALDWELL 1. Introduction The record for the largest known twin prime is constantly changing. For example, in October of 2000, David Underbakke found the record primes: 83475759 264955 1: · The very next day Giovanni La Barbera found the new record primes: 1693965 266443 1: · The fact that the size of these records are close is no coincidence! Before we seek a record like this, we usually try to estimate how long the search might take, and use this information to determine our search parameters. To do this we need to know how common twin primes are. It has been conjectured that the number of twin primes less than or equal to N is asymptotic to N dx 2C2N 2C2 2 2 Z2 (log x) ∼ (log N) where C2, called the twin prime constant, is approximately 0:6601618. Using this we can estimate how many numbers we will need to try before we find a prime. In the case of Underbakke and La Barbera, they were both using the same sieving software (NewPGen1 by Paul Jobling) and the same primality proving software (Proth.exe2 by Yves Gallot) on similar hardware{so of course they choose similar ranges to search. But where does this conjecture come from? In this chapter we will discuss a general method to form conjectures similar to the twin prime conjecture above. We will then apply it to a number of different forms of primes such as Sophie Germain primes, primes in arithmetic progressions, primorial primes and even the Goldbach conjecture. -
For Digital Simulation and Advanced Computation 2002 Annual Research Report
for Digital Simulation and Advanced Computation 2002 Annual Research Report 2002 Annual Research Report of the Supercomputing Institute for Digital Simulation and Advanced Computation Visit us on the Internet: www.msi.umn.edu Supercomputing Institute for Digital Simulation and Advanced Computation University of Minnesota 599 Walter 117 Pleasant Street SE Minneapolis, Minnesota 55455 ©2002 by the Regents of the University of Minnesota. All rights reserved. This report was prepared by Supercomputing Institute researchers and staff. Editor: Tracey Bartlett This information is available in alternative formats upon request by individuals with disabilities. Please send email to [email protected] or call (612) 625-1818. The University of Minnesota is committed to the policy that all persons shall have equal access to its programs, facilities, and employment without regard to race, color, creed, religion, national origin, sex, age, marital status, disability, public assistance status, veteran status, or sex- ual orientation. contains a minimum of 10% postconsumer waste Table of Contents Introduction Supercomputing Resources Overview....................................................................................................................................2 Supercomputers ........................................................................................................................3 Research Laboratories and Programs ......................................................................................5 Supercomputing Institute -
A Short and Simple Proof of the Riemann's Hypothesis
A Short and Simple Proof of the Riemann’s Hypothesis Charaf Ech-Chatbi To cite this version: Charaf Ech-Chatbi. A Short and Simple Proof of the Riemann’s Hypothesis. 2021. hal-03091429v10 HAL Id: hal-03091429 https://hal.archives-ouvertes.fr/hal-03091429v10 Preprint submitted on 5 Mar 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A Short and Simple Proof of the Riemann’s Hypothesis Charaf ECH-CHATBI ∗ Sunday 21 February 2021 Abstract We present a short and simple proof of the Riemann’s Hypothesis (RH) where only undergraduate mathematics is needed. Keywords: Riemann Hypothesis; Zeta function; Prime Numbers; Millennium Problems. MSC2020 Classification: 11Mxx, 11-XX, 26-XX, 30-xx. 1 The Riemann Hypothesis 1.1 The importance of the Riemann Hypothesis The prime number theorem gives us the average distribution of the primes. The Riemann hypothesis tells us about the deviation from the average. Formulated in Riemann’s 1859 paper[1], it asserts that all the ’non-trivial’ zeros of the zeta function are complex numbers with real part 1/2. 1.2 Riemann Zeta Function For a complex number s where ℜ(s) > 1, the Zeta function is defined as the sum of the following series: +∞ 1 ζ(s)= (1) ns n=1 X In his 1859 paper[1], Riemann went further and extended the zeta function ζ(s), by analytical continuation, to an absolutely convergent function in the half plane ℜ(s) > 0, minus a simple pole at s = 1: s +∞ {x} ζ(s)= − s dx (2) s − 1 xs+1 Z1 ∗One Raffles Quay, North Tower Level 35. -
Bayesian Perspectives on Mathematical Practice
Bayesian perspectives on mathematical practice James Franklin University of New South Wales, Sydney, Australia In: B. Sriraman, ed, Handbook of the History and Philosophy of Mathematical Practice, Springer, 2020. Contents 1. Introduction 2. The relation of conjectures to proof 3. Applied mathematics and statistics: understanding the behavior of complex models 4. The objective Bayesian perspective on evidence 5. Evidence for and against the Riemann Hypothesis 6. Probabilistic relations between necessary truths? 7. The problem of induction in mathematics 8. Conclusion References Abstract Mathematicians often speak of conjectures as being confirmed by evi- dence that falls short of proof. For their own conjectures, evidence justifies further work in looking for a proof. Those conjectures of mathematics that have long re- sisted proof, such as the Riemann Hypothesis, have had to be considered in terms of the evidence for and against them. In recent decades, massive increases in com- puter power have permitted the gathering of huge amounts of numerical evidence, both for conjectures in pure mathematics and for the behavior of complex applied mathematical models and statistical algorithms. Mathematics has therefore be- come (among other things) an experimental science (though that has not dimin- ished the importance of proof in the traditional style). We examine how the evalu- ation of evidence for conjectures works in mathematical practice. We explain the (objective) Bayesian view of probability, which gives a theoretical framework for unifying evidence evaluation in science and law as well as in mathematics. Nu- merical evidence in mathematics is related to the problem of induction; the occur- rence of straightforward inductive reasoning in the purely logical material of pure mathematics casts light on the nature of induction as well as of mathematical rea- soning. -
On the Existence and Temperedness of Cusp Forms for SL3(Z)
On the Existence and Temperedness of Cusp Forms for SL3(Z) Stephen D. Miller∗ Department of Mathematics Yale University P.O. Box 208283 New Haven, CT 06520-8283 [email protected] Abstract We develop a partial trace formula which circumvents some tech- nical difficulties in computing the Selberg trace formula for the quo- tient SL3(Z) SL3(R)/SO3(R). As applications, we establish the Weyl asymptotic law\ for the discrete Laplace spectrum and prove that al- most all of its cusp forms are tempered at infinity. The technique shows there are non-lifted cusp forms on SL3(Z) SL3(R)/SO3(R) as well as non-self-dual ones. A self-contained description\ of our proof for SL2(Z) H is included to convey the main new ideas. Heavy use is made of truncation\ and the Maass-Selberg relations. 1 Introduction In the 1950s A. Selberg ([Sel1]) developed his trace formula to prove the ex- istence of non-holomorphic, everywhere-unramified, cuspidal “Maass” forms. These are real-valued functions on the upper-half plane H = x + iy y > 0 { | } which are invariant under the action of SL2(Z) by fractional linear trans- formations. Unlike the holomorphic cusp forms, which can all be explicitly ∗The author was supported by an NSF Postdoctoral Fellowship during this work. 1 2 Stephen D. Miller described, no Maass form for SL2(Z) has ever been constructed and they are believed to be intrinsically transcendental. 2 The non-constant Laplace eigenfunctions in L (SL2(Z) H) are all Maass \ forms. Since SL2(Z) H is noncompact, their existence is no triviality; they very likely do not exist\ on the generic finite-volume quotient of H (see [Sarnak]). -
Bolles E.B. Einstein Defiant.. Genius Versus Genius in the Quantum
Selected other titles by Edmund Blair Bolles The Ice Finders: How a Poet, a Professor, and a Politician Discovered the Ice Age A Second Way of Knowing: The Riddle of Human Perception Remembering and Forgetting: Inquiries into the Nature of Memory So Much to Say: How to Help Your Child Learn Galileo’s Commandment: An Anthology of Great Science Writing (editor) Edmund Blair Bolles Joseph Henry Press Washington, DC Joseph Henry Press • 500 Fifth Street, NW • Washington, DC 20001 The Joseph Henry Press, an imprint of the National Academies Press, was created with the goal of making books on science, technology, and health more widely available to professionals and the public. Joseph Henry was one of the founders of the National Academy of Sciences and a leader in early American science. Any opinions, findings, conclusions, or recommendations expressed in this volume are those of the author and do not necessarily reflect the views of the National Academy of Sciences or its affiliated institutions. Library of Congress Cataloging-in-Publication Data Bolles, Edmund Blair, 1942- Einstein defiant : genius versus genius in the quantum revolution / by Edmund Blair Bolles. p. cm. Includes bibliographical references. ISBN 0-309-08998-0 (hbk.) 1. Quantum theory—History—20th century. 2. Physics—Europe—History— 20th century. 3. Einstein, Albert, 1879-1955. 4. Bohr, Niels Henrik David, 1885-1962. I. Title. QC173.98.B65 2004 530.12′09—dc22 2003023735 Copyright 2004 by Edmund Blair Bolles. All rights reserved. Printed in the United States of America. To Kelso Walker and the rest of the crew, volunteers all. -
ZETA FUNCTIONS of GRAPHS Graph Theory Meets Number Theory in This Stimulating Book
This page intentionally left blank CAMBRIDGE STUDIES IN ADVANCED MATHEMATICS 128 Editorial Board B. BOLLOBAS,´ W. FULTON, A. KATOK, F. KIRWAN, P. SARNAK, B. SIMON, B. TOTARO ZETA FUNCTIONS OF GRAPHS Graph theory meets number theory in this stimulating book. Ihara zeta functions of finite graphs are reciprocals of polynomials, sometimes in several variables. Analogies abound with number-theoretic functions such as Riemann or Dedekind zeta functions. For example, there is a Riemann hypothesis (which may be false) and a prime number theorem for graphs. Explicit constructions of graph coverings use Galois theory to generalize Cayley and Schreier graphs. Then non-isomorphic simple graphs with the same zeta function are produced, showing that you cannot “hear” the shape of a graph. The spectra of matrices such as the adjacency and edge adjacency matrices of a graph are essential to the plot of this book, which makes connections with quantum chaos and random matrix theory and also with expander and Ramanujan graphs, of interest in computer science. Pitched at beginning graduate students, the book will also appeal to researchers. Many well-chosen illustrations and exercises, both theoretical and computer-based, are included throughout. Audrey Terras is Professor Emerita of Mathematics at the University of California, San Diego. CAMBRIDGE STUDIES IN ADVANCED MATHEMATICS Editorial Board: B. Bollobas,´ W. Fulton, A. Katok, F. Kirwan, P. Sarnak, B. Simon, B. Totaro All the titles listed below can be obtained from good booksellers of from Cambridge University Press. For a complete series listing visit: http://www.cambridge.org/series/sSeries.asp?code=CSAM Already published 78 V. -
Chao-Dyn/9402001 7 Feb 94
chao-dyn/9402001 7 Feb 94 DESY ISSN Quantum Chaos January Einsteins Problem of The study of quantum chaos in complex systems constitutes a very fascinating and active branch of presentday physics chemistry and mathematics It is not wellknown however that this eld of research was initiated by a question rst p osed by Einstein during a talk delivered in Berlin on May concerning Quantum Chaos the relation b etween classical and quantum mechanics of strongly chaotic systems This seems historically almost imp ossible since quantum mechanics was not yet invented and the phenomenon of chaos was hardly acknowledged by physicists in While we are celebrating the seventyfth anniversary of our alma mater the Frank Steiner Hamburgische Universitat which was inaugurated on May it is interesting to have a lo ok up on the situation in physics in those days Most I I Institut f urTheoretische Physik UniversitatHamburg physicists will probably characterize that time as the age of the old quantum Lurup er Chaussee D Hamburg Germany theory which started with Planck in and was dominated then by Bohrs ingenious but paradoxical mo del of the atom and the BohrSommerfeld quanti zation rules for simple quantum systems Some will asso ciate those years with Einsteins greatest contribution the creation of general relativity culminating in the generally covariant form of the eld equations of gravitation which were found by Einstein in the year and indep endently by the mathematician Hilb ert at the same time In his talk in May Einstein studied the -
Nima Arkani-Hamed, Juan Maldacena, Nathan Both Particle Physicists and Astrophysicists, We Are in an Ideal Seiberg, and Edward Witten
THE I NSTITUTE L E T T E R INSTITUTE FOR ADVANCED STUDY PRINCETON, NEW JERSEY · SUMMER 2008 PROBING THE DARK SIDE OF THE UNIVERSE ne of The remarkable dis - erTies of dark maTTer, and a Ocoveries in asTrophysics has more precise accounTing of The been The recogniTion ThaT The composiTion of The universe, maTerial we see and are familiar The Two fields of asTrophysics wiTh, which makes up The earTh, (The physics of The very large) The sun, The sTars, and everyday and parTicle physics (The objecTs, such as a Table, is only a physics of The very small) are small fracTion of all of The maTTer each providing some of The in The universe. The resT is dark mosT imporTanT new experi - maTTer, possibly a new form of menTal daTa and TheoreTical elemenTary parTicle ThaT does concepTs for The oTher. Re- noT emiT or absorb lighT, and can search aT The InsTiTuTe for only be deTecTed from iTs gravi - Advanced STudy has played a These three images created by Member Douglas Rudd show the various matter components in a simulation encompassing a volume 86 TaTional effecTs. Megaparsec on a side (for reference, the distance between the Milky Way and its nearest neighbor is 0.75 Mpc). The three compo - significanT role in This develop - In The lasT decade, asTro - nents are dark matter (blue), gas (green), and stars (orange). The stars form in galaxies which lie at the intersection of filaments as menT. The laTe InsTiTuTe Pro - nomical observaTions of several seen in the dark matter and gas profiles. -
2 Primes Numbers
V55.0106 Quantitative Reasoning: Computers, Number Theory and Cryptography 2 Primes Numbers Definition 2.1 A number is prime is it is greater than 1, and its only divisors are itself and 1. A number is called composite if it is greater than 1 and is the product of two numbers greater than 1. Thus, the positive numbers are divided into three mutually exclusive classes. The prime numbers, the composite numbers, and the unit 1. We can show that a number is composite numbers by finding a non-trivial factorization.8 Thus, 21 is composite because 21 = 3 7. The letter p is usually used to denote a prime number. × The first fifteen prime numbers are 2, 3, 5, 7, 11, 13, 17, 19, 23, 29, 31, 37, 41 These are found by a process of elimination. Starting with 2, 3, 4, 5, 6, 7, etc., we eliminate the composite numbers 4, 6, 8, 9, and so on. There is a systematic way of finding a table of all primes up to a fixed number. The method is called a sieve method and is called the Sieve of Eratosthenes9. We first illustrate in a simple example by finding all primes from 2 through 25. We start by listing the candidates: 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23, 24, 25 The first number 2 is a prime, but all multiples of 2 after that are not. Underline these multiples. They are eliminated as composite numbers. The resulting list is as follows: 2, 3, 4,5,6,7,8,9,10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23, 24,25 The next number not eliminated is 3, the next prime. -
Prime Number Theorem
Prime Number Theorem Bent E. Petersen Contents 1 Introduction 1 2Asymptotics 6 3 The Logarithmic Integral 9 4TheCebyˇˇ sev Functions θ(x) and ψ(x) 11 5M¨obius Inversion 14 6 The Tail of the Zeta Series 16 7 The Logarithm log ζ(s) 17 < s 8 The Zeta Function on e =1 21 9 Mellin Transforms 26 10 Sketches of the Proof of the PNT 29 10.1 Cebyˇˇ sev function method .................. 30 10.2 Modified Cebyˇˇ sev function method .............. 30 10.3 Still another Cebyˇˇ sev function method ............ 30 10.4 Yet another Cebyˇˇ sev function method ............ 31 10.5 Riemann’s method ...................... 31 10.6 Modified Riemann method .................. 32 10.7 Littlewood’s Method ..................... 32 10.8 Ikehara Tauberian Theorem ................. 32 11ProofofthePrimeNumberTheorem 33 References 39 1 Introduction Let π(x) be the number of primes p ≤ x. It was discovered empirically by Gauss about 1793 (letter to Enke in 1849, see Gauss [9], volume 2, page 444 and Goldstein [10]) and by Legendre (in 1798 according to [14]) that x π(x) ∼ . log x This statement is the prime number theorem. Actually Gauss used the equiva- lent formulation (see page 10) Z x dt π(x) ∼ . 2 log t 1 B. E. Petersen Prime Number Theorem For some discussion of Gauss’ work see Goldstein [10] and Zagier [45]. In 1850 Cebyˇˇ sev [3] proved a result far weaker than the prime number theorem — that for certain constants 0 <A1 < 1 <A2 π(x) A < <A . 1 x/log x 2 An elementary proof of Cebyˇˇ sev’s theorem is given in Andrews [1]. -
Notes on the Prime Number Theorem
Notes on the prime number theorem Kenji Kozai May 2, 2014 1 Statement We begin with a definition. Definition 1.1. We say that f(x) and g(x) are asymptotic as x → ∞, f(x) written f ∼ g, if limx→∞ g(x) = 1. The prime number theorem tells us about the asymptotic behavior of the number of primes that are less than a given number. Let π(x) be the number of primes numbers p such that p ≤ x. For example, π(2) = 1, π(3) = 2, π(4) = 2, etc. The statement that we will try to prove is as follows. Theorem 1.2 (Prime Number Theorem, p. 382). The asymptotic behavior of π(x) as x → ∞ is given by x π(x) ∼ . log x This was originally observed as early as the 1700s by Gauss and others. The first proof was given in 1896 by Hadamard and de la Vall´ee Poussin. We will give an overview of simplified proof. Most of the material comes from various sections of Gamelin – mostly XIV.1, XIV.3 and XIV.5. 2 The Gamma Function The gamma function Γ(z) is a meromorphic function that extends the fac- torial n! to arbitrary complex values. For Re z > 0, we can find the gamma function by the integral: ∞ Γ(z)= e−ttz−1dt, Re z > 0. Z0 1 To see the relation with the factorial, we integrate by parts: ∞ Γ(z +1) = e−ttzdt Z0 ∞ z −t ∞ −t z−1 = −t e |0 + z e t dt Z0 = zΓ(z). ∞ −t This holds whenever Re z > 0.