The Ising Model of a Ferromagnet from 1920 to 2020
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The Ising Model
The Ising Model Today we will switch topics and discuss one of the most studied models in statistical physics the Ising Model • Some applications: – Magnetism (the original application) – Liquid-gas transition – Binary alloys (can be generalized to multiple components) • Onsager solved the 2D square lattice (1D is easy!) • Used to develop renormalization group theory of phase transitions in 1970’s. • Critical slowing down and “cluster methods”. Figures from Landau and Binder (LB), MC Simulations in Statistical Physics, 2000. Atomic Scale Simulation 1 The Model • Consider a lattice with L2 sites and their connectivity (e.g. a square lattice). • Each lattice site has a single spin variable: si = ±1. • With magnetic field h, the energy is: N −β H H = −∑ Jijsis j − ∑ hisi and Z = ∑ e ( i, j ) i=1 • J is the nearest neighbors (i,j) coupling: – J > 0 ferromagnetic. – J < 0 antiferromagnetic. • Picture of spins at the critical temperature Tc. (Note that connected (percolated) clusters.) Atomic Scale Simulation 2 Mapping liquid-gas to Ising • For liquid-gas transition let n(r) be the density at lattice site r and have two values n(r)=(0,1). E = ∑ vijnin j + µ∑ni (i, j) i • Let’s map this into the Ising model spin variables: 1 s = 2n − 1 or n = s + 1 2 ( ) v v + µ H s s ( ) s c = ∑ i j + ∑ i + 4 (i, j) 2 i J = −v / 4 h = −(v + µ) / 2 1 1 1 M = s n = n = M + 1 N ∑ i N ∑ i 2 ( ) i i Atomic Scale Simulation 3 JAVA Ising applet http://physics.weber.edu/schroeder/software/demos/IsingModel.html Dynamically runs using heat bath algorithm. -
Arxiv:1511.03031V2
submitted to acta physica slovaca 1– 133 A BRIEF ACCOUNT OF THE ISING AND ISING-LIKE MODELS: MEAN-FIELD, EFFECTIVE-FIELD AND EXACT RESULTS Jozef Streckaˇ 1, Michal Jasˇcurˇ 2 Department of Theoretical Physics and Astrophysics, Faculty of Science, P. J. Saf´arikˇ University, Park Angelinum 9, 040 01 Koˇsice, Slovakia The present article provides a tutorial review on how to treat the Ising and Ising-like models within the mean-field, effective-field and exact methods. The mean-field approach is illus- trated on four particular examples of the lattice-statistical models: the spin-1/2 Ising model in a longitudinal field, the spin-1 Blume-Capel model in a longitudinal field, the mixed-spin Ising model in a longitudinal field and the spin-S Ising model in a transverse field. The mean- field solutions of the spin-1 Blume-Capel model and the mixed-spin Ising model demonstrate a change of continuous phase transitions to discontinuous ones at a tricritical point. A con- tinuous quantum phase transition of the spin-S Ising model driven by a transverse magnetic field is also explored within the mean-field method. The effective-field theory is elaborated within a single- and two-spin cluster approach in order to demonstrate an efficiency of this ap- proximate method, which affords superior approximate results with respect to the mean-field results. The long-standing problem of this method concerned with a self-consistent deter- mination of the free energy is also addressed in detail. More specifically, the effective-field theory is adapted for the spin-1/2 Ising model in a longitudinal field, the spin-S Blume-Capel model in a longitudinal field and the spin-1/2 Ising model in a transverse field. -
An Introduction to the Ising Model Barry A. Cipra the American
An Introduction to the Ising Model Barry A. Cipra The American Mathematical Monthly, Vol. 94, No. 10. (Dec., 1987), pp. 937-959. Stable URL: http://links.jstor.org/sici?sici=0002-9890%28198712%2994%3A10%3C937%3AAITTIM%3E2.0.CO%3B2-V The American Mathematical Monthly is currently published by Mathematical Association of America. Your use of the JSTOR archive indicates your acceptance of JSTOR's Terms and Conditions of Use, available at http://www.jstor.org/about/terms.html. JSTOR's Terms and Conditions of Use provides, in part, that unless you have obtained prior permission, you may not download an entire issue of a journal or multiple copies of articles, and you may use content in the JSTOR archive only for your personal, non-commercial use. Please contact the publisher regarding any further use of this work. Publisher contact information may be obtained at http://www.jstor.org/journals/maa.html. Each copy of any part of a JSTOR transmission must contain the same copyright notice that appears on the screen or printed page of such transmission. JSTOR is an independent not-for-profit organization dedicated to and preserving a digital archive of scholarly journals. For more information regarding JSTOR, please contact [email protected]. http://www.jstor.org Mon Apr 30 12:49:36 2007 An Introduction to the Ising Model BARRYA. CIPRA,St. Olu/College, Northfield, Minnesotu 55057 Burry Cipru received a Ph.D, in mathematics from the University of Maryland in 1980. He has been an instructor at M.I.T. and at the Ohio State University, and is currently an assistant professor of mathematics at St. -
Statistical Field Theory University of Cambridge Part III Mathematical Tripos
Preprint typeset in JHEP style - HYPER VERSION Michaelmas Term, 2017 Statistical Field Theory University of Cambridge Part III Mathematical Tripos David Tong Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 OBA, UK http://www.damtp.cam.ac.uk/user/tong/sft.html [email protected] –1– Recommended Books and Resources There are a large number of books which cover the material in these lectures, although often from very di↵erent perspectives. They have titles like “Critical Phenomena”, “Phase Transitions”, “Renormalisation Group” or, less helpfully, “Advanced Statistical Mechanics”. Here are some that I particularly like Nigel Goldenfeld, Phase Transitions and the Renormalization Group • Agreatbook,coveringthebasicmaterialthatwe’llneedanddelvingdeeperinplaces. Mehran Kardar, Statistical Physics of Fields • The second of two volumes on statistical mechanics. It cuts a concise path through the subject, at the expense of being a little telegraphic in places. It is based on lecture notes which you can find on the web; a link is given on the course website. John Cardy, Scaling and Renormalisation in Statistical Physics • Abeautifullittlebookfromoneofthemastersofconformalfieldtheory.Itcoversthe material from a slightly di↵erent perspective than these lectures, with more focus on renormalisation in real space. Chaikin and Lubensky, Principles of Condensed Matter Physics • Shankar, Quantum Field Theory and Condensed Matter • Both of these are more all-round condensed matter books, but with substantial sections on critical phenomena and the renormalisation group. Chaikin and Lubensky is more traditional, and packed full of content. Shankar covers modern methods of QFT, with an easygoing style suitable for bedtime reading. Anumberofexcellentlecturenotesareavailableontheweb.Linkscanbefoundon the course webpage: http://www.damtp.cam.ac.uk/user/tong/sft.html. -
Lecture 8: the Ising Model Introduction
Lecture 8: The Ising model Introduction I Up to now: Toy systems with interesting properties (random walkers, cluster growth, percolation) I Common to them: No interactions I Add interactions now, with significant role I Immediate consequence: much richer structure in model, in particular: phase transitions I Simulate interactions with RNG (Monte Carlo method) I Include the impact of temperature: ideas from thermodynamics and statistical mechanics important I Simple system as example: coupled spins (see below), will use the canonical ensemble for its description The Ising model I A very interesting model for understanding some properties of magnetic materials, especially the phase transition ferromagnetic ! paramagnetic I Intrinsically, magnetism is a quantum effect, triggered by the spins of particles aligning with each other I Ising model a superb toy model to understand this dynamics I Has been invented in the 1920's by E.Ising I Ever since treated as a first, paradigmatic model The model (in 2 dimensions) I Consider a square lattice with spins at each lattice site I Spins can have two values: si = ±1 I Take into account only nearest neighbour interactions (good approximation, dipole strength falls off as 1=r 3) I Energy of the system: P E = −J si sj hiji I Here: exchange constant J > 0 (for ferromagnets), and hiji denotes pairs of nearest neighbours. I (Micro-)states α characterised by the configuration of each spin, the more aligned the spins in a state α, the smaller the respective energy Eα. I Emergence of spontaneous magnetisation (without external field): sufficiently many spins parallel Adding temperature I Without temperature T : Story over. -
Arxiv:1504.02898V2 [Cond-Mat.Stat-Mech] 7 Jun 2015 Keywords: Percolation, Explosive Percolation, SLE, Ising Model, Earth Topography
Recent advances in percolation theory and its applications Abbas Ali Saberi aDepartment of Physics, University of Tehran, P.O. Box 14395-547,Tehran, Iran bSchool of Particles and Accelerators, Institute for Research in Fundamental Sciences (IPM) P.O. Box 19395-5531, Tehran, Iran Abstract Percolation is the simplest fundamental model in statistical mechanics that exhibits phase transitions signaled by the emergence of a giant connected component. Despite its very simple rules, percolation theory has successfully been applied to describe a large variety of natural, technological and social systems. Percolation models serve as important universality classes in critical phenomena characterized by a set of critical exponents which correspond to a rich fractal and scaling structure of their geometric features. We will first outline the basic features of the ordinary model. Over the years a variety of percolation models has been introduced some of which with completely different scaling and universal properties from the original model with either continuous or discontinuous transitions depending on the control parameter, di- mensionality and the type of the underlying rules and networks. We will try to take a glimpse at a number of selective variations including Achlioptas process, half-restricted process and spanning cluster-avoiding process as examples of the so-called explosive per- colation. We will also introduce non-self-averaging percolation and discuss correlated percolation and bootstrap percolation with special emphasis on their recent progress. Directed percolation process will be also discussed as a prototype of systems displaying a nonequilibrium phase transition into an absorbing state. In the past decade, after the invention of stochastic L¨ownerevolution (SLE) by Oded Schramm, two-dimensional (2D) percolation has become a central problem in probability theory leading to the two recent Fields medals. -
Multiple Schramm-Loewner Evolutions and Statistical Mechanics Martingales
Multiple Schramm-Loewner Evolutions and Statistical Mechanics Martingales Michel Bauer a, Denis Bernard a 1, Kalle Kyt¨ol¨a b [email protected]; [email protected]; [email protected] a Service de Physique Th´eorique de Saclay CEA/DSM/SPhT, Unit´ede recherche associ´ee au CNRS CEA-Saclay, 91191 Gif-sur-Yvette, France. b Department of Mathematics, P.O. Box 68 FIN-00014 University of Helsinki, Finland. Abstract A statistical mechanics argument relating partition functions to martingales is used to get a condition under which random geometric processes can describe interfaces in 2d statistical mechanics at critical- ity. Requiring multiple SLEs to satisfy this condition leads to some natural processes, which we study in this note. We give examples of such multiple SLEs and discuss how a choice of conformal block is related to geometric configuration of the interfaces and what is the physical meaning of mixed conformal blocks. We illustrate the general arXiv:math-ph/0503024v2 21 Mar 2005 ideas on concrete computations, with applications to percolation and the Ising model. 1Member of C.N.R.S 1 Contents 1 Introduction 3 2 Basics of Schramm-L¨owner evolutions: Chordal SLE 6 3 A proposal for multiple SLEs 7 3.1 Thebasicequations ....................... 7 3.2 Archprobabilities......................... 8 4 First comments 10 4.1 Statistical mechanics interpretation . 10 4.2 SLEasaspecialcaseof2SLE. 10 4.3 Makingsense ........................... 12 4.4 A few martingales for nSLEs .................. 13 4.5 Classicallimit........................... 14 4.6 Relations with other work . 15 5 CFT background 16 6 Martingales from statistical mechanics 19 6.1 Tautological martingales . -
From Abraham De Moivre to Johann Carl Friedrich Gauss
International Journal of Engineering Science Invention (IJESI) ISSN (Online): 2319 – 6734, ISSN (Print): 2319 – 6726 www.ijesi.org ||Volume 7 Issue 6 Ver V || June 2018 || PP 28-34 A Brief Historical Overview Of the Gaussian Curve: From Abraham De Moivre to Johann Carl Friedrich Gauss Edel Alexandre Silva Pontes1 1Department of Mathematics, Federal Institute of Alagoas, Brazil Abstract : If there were only one law of probability to be known, this would be the Gaussian distribution. Faced with this uneasiness, this article intends to discuss about this distribution associated with its graph called the Gaussian curve. Due to the scarcity of texts in the area and the great demand of students and researchers for more information about this distribution, this article aimed to present a material on the history of the Gaussian curve and its relations. In the eighteenth and nineteenth centuries, there were several mathematicians who developed research on the curve, including Abraham de Moivre, Pierre Simon Laplace, Adrien-Marie Legendre, Francis Galton and Johann Carl Friedrich Gauss. Some researchers refer to the Gaussian curve as the "curve of nature itself" because of its versatility and inherent nature in almost everything we find. Virtually all probability distributions were somehow part or originated from the Gaussian distribution. We believe that the work described, the study of the Gaussian curve, its history and applications, is a valuable contribution to the students and researchers of the different areas of science, due to the lack of more detailed research on the subject. Keywords - History of Mathematics, Distribution of Probabilities, Gaussian Curve. ----------------------------------------------------------------------------------------------------------------------------- --------- Date of Submission: 09-06-2018 Date of acceptance: 25-06-2018 ----------------------------------------------------------------------------------------------------------------------------- ---------- I. -
Carl Friedrich Gauss Seminarski Rad
SREDNJA ŠKOLA AMBROZA HARAČIĆA PODRUČNI ODJEL CRES CARL FRIEDRICH GAUSS SEMINARSKI RAD Cres, 2014. SREDNJA ŠKOLA AMBROZA HARAČIĆA PODRUČNI ODJEL CRES CARL FRIEDRICH GAUSS SEMINARSKI RAD Učenice: Marina Kučica Giulia Muškardin Brigita Novosel Razred: 3.g. Mentorica: prof. Melita Chiole Predmet: Matematika Cres, ožujak 2014. II Sadržaj 1. UVOD .................................................................................................................................... 1 2. DJETINJSTVO I ŠKOLOVANJE ......................................................................................... 2 3. PRIVATNI ŽIVOT ................................................................................................................ 5 4. GAUSSOV RAD ................................................................................................................... 6 4.1. Prvi znanstveni rad .......................................................................................................... 6 4.2. Teorija brojeva ................................................................................................................ 8 4.3. Geodezija ......................................................................................................................... 9 4.4. Fizika ............................................................................................................................. 11 4.5. Astronomija ................................................................................................................... 12 4.6. Religija -
2 a Revolutionary Science
2 A Revolutionary Science When the Parisian crowds stormed the Bastille fortress and prison on 14 July 1789, they set in motion a train of events that revolutionized European political culture. To many contem- porary commentators and observers of the French Revolution, it seemed that the growing disenchantment with the absolutist regime of Louis XVI had been fostered in part by a particular kind of philosophy. French philosophes condemning the iniqui- ties of the ancien regime´ drew parallels between the organization of society and the organization of nature. Like many other En- lightenment thinkers, they took it for granted that science, or natural philosophy,could be used as a tool to understand society as well as nature. They argued that the laws of nature showed how unjust and unnatural the government of France really was. It also seemed, to some at least, that the French Revolution pro- vided an opportunity to galvanize science as well as society. The new French Republic was a tabula rasa on which the reform- ers could write what they liked. They could refound society on philosophical principles, making sure this time around that the organization of society really did mirror the organization of nature. Refounding the social and intellectual structures of sci- ence itself was to be part of this process. In many ways, therefore, the storming of the Bastille led to a revolution in science as well. To many in this new generation of radical French natu- ral philosophers, mathematics seemed to provide the key to 22 A Revolutionary Science 23 understanding nature. This was nothing new in itself, of course. -
Newton's Notebook
Newton’s Notebook The Haverford School’s Math & Applied Math Journal Issue I Spring 2017 The Haverford School Newton’s Notebook Spring 2017 “To explain all nature is too difficult a task for any one man or even for any one age. ‘Tis much better to do a little with certainty & leave the rest for others that come after you.” ~Isaac Newton Table of Contents Pure Mathematics: 7 The Golden Ratio.........................................................................................Robert Chen 8 Fermat’s Last Theorem.........................................................................Michael Fairorth 9 Math in Coding............................................................................................Bram Schork 10 The Pythagoreans.........................................................................................Eusha Hasan 12 Transfinite Numbers.................................................................................Caleb Clothier 15 Sphere Equality................................................................................Matthew Baumholtz 16 Interesting Series.......................................................................................Aditya Sardesi 19 Indirect Proofs..............................................................................................Mr. Patrylak Applied Mathematics: 23 Physics in Finance....................................................................................Caleb Clothier 26 The von Bertalanffy Equation..................................................................Will -
The Astronomical Work of Carl Friedrich Gauss
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector HISTORIA MATHEMATICA 5 (1978), 167-181 THE ASTRONOMICALWORK OF CARL FRIEDRICH GAUSS(17774855) BY ERIC G, FORBES, UNIVERSITY OF EDINBURGH, EDINBURGH EH8 9JY This paper was presented on 3 June 1977 at the Royal Society of Canada's Gauss Symposium at the Ontario Science Centre in Toronto [lj. SUMMARIES Gauss's interest in astronomy dates from his student-days in Gattingen, and was stimulated by his reading of Franz Xavier von Zach's Monatliche Correspondenz... where he first read about Giuseppe Piazzi's discovery of the minor planet Ceres on 1 January 1801. He quickly produced a theory of orbital motion which enabled that faint star-like object to be rediscovered by von Zach and others after it emerged from the rays of the Sun. Von Zach continued to supply him with the observations of contemporary European astronomers from which he was able to improve his theory to such an extent that he could detect the effects of planetary perturbations in distorting the orbit from an elliptical form. To cope with the complexities which these introduced into the calculations of Ceres and more especially the other minor planet Pallas, discovered by Wilhelm Olbers in 1802, Gauss developed a new and more rigorous numerical approach by making use of his mathematical theory of interpolation and his method of least-squares analysis, which was embodied in his famous Theoria motus of 1809. His laborious researches on the theory of Pallas's motion, in whi::h he enlisted the help of several former students, provided the framework of a new mathematical formu- lation of the problem whose solution can now be easily effected thanks to modern computational techniques.