Applications of Fractional Dimensional Space in Statistical Mechanics
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On the Origin and Early History of Functional Analysis
U.U.D.M. Project Report 2008:1 On the origin and early history of functional analysis Jens Lindström Examensarbete i matematik, 30 hp Handledare och examinator: Sten Kaijser Januari 2008 Department of Mathematics Uppsala University Abstract In this report we will study the origins and history of functional analysis up until 1918. We begin by studying ordinary and partial differential equations in the 18th and 19th century to see why there was a need to develop the concepts of functions and limits. We will see how a general theory of infinite systems of equations and determinants by Helge von Koch were used in Ivar Fredholm’s 1900 paper on the integral equation b Z ϕ(s) = f(s) + λ K(s, t)f(t)dt (1) a which resulted in a vast study of integral equations. One of the most enthusiastic followers of Fredholm and integral equation theory was David Hilbert, and we will see how he further developed the theory of integral equations and spectral theory. The concept introduced by Fredholm to study sets of transformations, or operators, made Maurice Fr´echet realize that the focus should be shifted from particular objects to sets of objects and the algebraic properties of these sets. This led him to introduce abstract spaces and we will see how he introduced the axioms that defines them. Finally, we will investigate how the Lebesgue theory of integration were used by Frigyes Riesz who was able to connect all theory of Fredholm, Fr´echet and Lebesgue to form a general theory, and a new discipline of mathematics, now known as functional analysis. -
Interconversion of Hydrated Protons at the Interface Between Liquid Water and Platinum
Electronic Supplementary Material (ESI) for Physical Chemistry Chemical Physics. This journal is © the Owner Societies 2019 Supporting Information: Interconversion of Hydrated Protons at the Interface between Liquid Water and Platinum Peter S. Rice, Yu Mao, Chenxi Guo and P. Hu* School of Chemistry and Chemical Engineering, The Queen’s University of Belfast, Belfast BT9 5AG, N. Ireland Email: [email protected] Contents Page S1. Ab Initio Molecular Dynamics (AIMD) based Umbrella Sampling (US) ................. 14 S2. Unit Cell Conversion ................................................................................................ 17 S3. Atomic Density Profile ............................................................................................. 17 S4. Radial Pair Distribution Function, (g(r)) ................................................................. 18 S5. Coordination Number (CN) ..................................................................................... 18 S6. Charge Density Difference ....................................................................................... 19 S7. Self-Diffusion Coefficient (D0) .................................................................................. 21 S8. Dipole Orientation Analysis ..................................................................................... 22 13 S1. Ab Initio Molecular Dynamics (AIMD) based Umbrella Sampling (US) x To study the interchange of species at the Pt(111)/H2n+1On interface, MD simulations based on umbrella sampling were used to investigate -
History of Nonlinear Oscillations Theory in France (1880–1940)
Archimedes 49 New Studies in the History and Philosophy of Science and Technology Jean-Marc Ginoux History of Nonlinear Oscillations Theory in France (1880–1940) History of Nonlinear Oscillations Theory in France (1880–1940) Archimedes NEW STUDIES IN THE HISTORY AND PHILOSOPHY OF SCIENCE AND TECHNOLOGY VOLUME 49 EDITOR JED Z. BUCHWALD, Dreyfuss Professor of History, California Institute of Technology, Pasadena, USA. ASSOCIATE EDITORS FOR MATHEMATICS AND PHYSICAL SCIENCES JEREMY GRAY, The Faculty of Mathematics and Computing, The Open University, UK. TILMAN SAUER, Johannes Gutenberg University Mainz, Germany ASSOCIATE EDITORS FOR BIOLOGICAL SCIENCES SHARON KINGSLAND, Department of History of Science and Technology, Johns Hopkins University, Baltimore, USA. MANFRED LAUBICHLER, Arizona State University, USA ADVISORY BOARD FOR MATHEMATICS, PHYSICAL SCIENCES AND TECHNOLOGY HENK BOS, University of Utrecht, The Netherlands MORDECHAI FEINGOLD, California Institute of Technology, USA ALLAN D. FRANKLIN, University of Colorado at Boulder, USA KOSTAS GAVROGLU, National Technical University of Athens, Greece PAUL HOYNINGEN-HUENE, Leibniz University in Hannover, Germany TREVOR LEVERE, University of Toronto, Canada JESPER LÜTZEN, Copenhagen University, Denmark WILLIAM NEWMAN, Indiana University, Bloomington, USA LAWRENCE PRINCIPE, The Johns Hopkins University, USA JÜRGEN RENN, Max Planck Institute for the History of Science, Germany ALEX ROLAND, Duke University, USA ALAN SHAPIRO, University of Minnesota, USA NOEL SWERDLOW, California Institute of Technology, -
Thermodynamic Temperature
Thermodynamic temperature Thermodynamic temperature is the absolute measure 1 Overview of temperature and is one of the principal parameters of thermodynamics. Temperature is a measure of the random submicroscopic Thermodynamic temperature is defined by the third law motions and vibrations of the particle constituents of of thermodynamics in which the theoretically lowest tem- matter. These motions comprise the internal energy of perature is the null or zero point. At this point, absolute a substance. More specifically, the thermodynamic tem- zero, the particle constituents of matter have minimal perature of any bulk quantity of matter is the measure motion and can become no colder.[1][2] In the quantum- of the average kinetic energy per classical (i.e., non- mechanical description, matter at absolute zero is in its quantum) degree of freedom of its constituent particles. ground state, which is its state of lowest energy. Thermo- “Translational motions” are almost always in the classical dynamic temperature is often also called absolute tem- regime. Translational motions are ordinary, whole-body perature, for two reasons: one, proposed by Kelvin, that movements in three-dimensional space in which particles it does not depend on the properties of a particular mate- move about and exchange energy in collisions. Figure 1 rial; two that it refers to an absolute zero according to the below shows translational motion in gases; Figure 4 be- properties of the ideal gas. low shows translational motion in solids. Thermodynamic temperature’s null point, absolute zero, is the temperature The International System of Units specifies a particular at which the particle constituents of matter are as close as scale for thermodynamic temperature. -
Ideal Gas with a Varying (Negative Absolute) Temperature
Ideal gas with a varying (negative absolute) temperature: An alternative to dark energy? Subhajit Saha1, Anindita Mondal2 and Christian Corda3 February 5, 2018 1 Department of Mathematics, Panihati Mahavidyalaya, Kolkata 700110, West Bengal, India, e-mail: [email protected]. 2Department of Astrophysics and Cosmology, S. N. Bose National Centre for Basic Sciences, JD Block, Sector III, Salt Lake City, Kolkata 700106, India, e-mail: [email protected]. 3 Research Institute for Astronomy and Astrophysics of Maragha (RIAAM), P.O. Box 55134-441, Maragha, Iran, e-mail: [email protected]. Abstract The present work is an attempt to investigate whether the evolutionary history of the Universe from the offset of inflation can be described by assuming the cosmic fluid to be an ideal gas with a specific gas constant but a varying negative absolute temperature (NAT). The motivation of this work is to search for an alternative to the "exotic" and "supernatural" dark energy (DE). In fact, the NAT works as an “effective quintessence” and there is need to deal neither with exotic matter like DE nor with modified gravity theories. For the sake of completeness, we release some clarifications on NATs in Section 3 of the paper. Keywords: Negative absolute temperature; Cosmic accel- eration; Ideal gas law; Dark energy arXiv:1802.00742v1 [physics.gen-ph] 26 Jan 2018 PACS Numbers: 98.80.-k 1 Introduction Since the intriguing discovery of the late time cosmic acceleration in 1998, which was expected by the Indian physicist B. Sidharth [1] before the cosmological observations of the High-Z Supernova Search Team [2] and of the Supernova 1 Cosmology Project [3], there have been rigorous attempts to incorporate this unexpected observations into standard cosmology. -
A Monte Carlo Simulation of Locally Nonchaotic Barrier
Production of Useful Work in an Isothermal Cycle: A Monte Carlo Simulation of a Locally Nonchaotic Energy Barrier Y. Qiao,1,2,* Z. Shang1 1 Program of Materials Science and Engineering, University of California – San Diego, La Jolla, CA 92093, U.S.A. 2 Department of Structural Engineering, University of California – San Diego, La Jolla, CA 92093-0085, U.S.A. * Corresponding author (Email: [email protected]; phone: 858-534-3388) Abstract: A Monte Carlo simulation is performed on a billiard-type model system, which contains a locally nonchaotic energy barrier. Without extensive particle collision across the energy barrier, the system steady state is nonequilibrium; that is, the particles follow a non-Boltzmann distribution. Remarkably, as the energy barrier varies in an isothermal cycle, the total produced work is greater than the total consumed work, because of the asymmetry in the cross-influence of the thermally correlated thermodynamic driving forces. Such a phenomenon cannot be explained by the second law of thermodynamics. Similar anomalous effects may be achieved if the barrier is switchable or asymmetric. In essence, the energy barrier is a spontaneously nonequilibrium dimension. It is fundamentally different from Maxwell’s demon, unrelated to the physical nature of information. KEYWORDS: Nonequilibrium; Nonchaotic; The second law of thermodynamics; Energy barrier; Monte Carlo simulation 1. Introduction Randomness is a fundamental concept in statistical mechanics [1,2]. An ergodic and chaotic system always reaches thermodynamic equilibrium, while a nonergodic or nonchaotic system may not [e.g., 3-5]. The latter should be analyzed in the framework of nonequilibrium stochastic thermodynamics [6]. 1 Figure 1. -
Selvi Afstudeerverslag
Eindhoven University of Technology MASTER On the reservoir model for CO2-laser amplification Selvi, S.C. Award date: 2018 Link to publication Disclaimer This document contains a student thesis (bachelor's or master's), as authored by a student at Eindhoven University of Technology. Student theses are made available in the TU/e repository upon obtaining the required degree. The grade received is not published on the document as presented in the repository. The required complexity or quality of research of student theses may vary by program, and the required minimum study period may vary in duration. General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. • Users may download and print one copy of any publication from the public portal for the purpose of private study or research. • You may not further distribute the material or use it for any profit-making activity or commercial gain On the reservoir model for CO2-laser amplification S.C. Selvi November 15, 2018 2 Abstract In many technological applications, such as extreme ultraviolet lithography, high-intensity CO2- laser pulses are used, which are created in a CO2-laser amplification system. Research concerned with CO2-laser amplification tries to describe the dynamics of such amplifications systems to be able to make predictions about its characteristics and performance. The system under consider- ation is a single plasma cell of the amplification system having a pre-mixture of CO2-CO-N2-He and infra-red radiation with a wavelength of 10:58 µm and 10:206 µm. -
HARDY SPACES the Theory of Hardy Spaces Is a Cornerstone of Modern Analysis
CAMBRIDGE STUDIES IN ADVANCED MATHEMATICS 179 Editorial Board B. BOLLOBAS,´ W. FULTON, F. KIRWAN, P. SARNAK, B. SIMON, B. TOTARO HARDY SPACES The theory of Hardy spaces is a cornerstone of modern analysis. It combines techniques from functional analysis, the theory of analytic functions, and Lesbesgue integration to create a powerful tool for many applications, pure and applied, from signal processing and Fourier analysis to maximum modulus principles and the Riemann zeta function. This book, aimed at beginning graduate students, introduces and develops the classical results on Hardy spaces and applies them to fundamental concrete problems in analysis. The results are illustrated with numerous solved exercises which also introduce subsidiary topics and recent developments. The reader’s understanding of the current state of the field, as well as its history, are further aided by engaging accounts of the key players and by the surveys of recent advances (with commented reference lists) that end each chapter. Such broad coverage makes this book the ideal source on Hardy spaces. Nikola¨ı Nikolski is Professor Emeritus at the Universite´ de Bordeaux working primarily in analysis and operator theory. He has been co-editor of four international journals and published numerous articles and research monographs. He has also supervised some 30 PhD students, including three Salem Prize winners. Professor Nikolski was elected Fellow of the AMS in 2013 and received the Prix Ampere` of the French Academy of Sciences in 2010. CAMBRIDGE STUDIES IN ADVANCED MATHEMATICS Editorial Board B. Bollobas,´ W. Fulton, F. Kirwan, P. Sarnak, B. Simon, B. Totaro All the titles listed below can be obtained from good booksellers or from Cambridge University Press. -
Essay Review
HISTORIA MATHEMATICA 23, (1996), 74±84 ARTICLE NO. 0006 ESSAY REVIEW Edited by CATHERINE GOLDSTEIN AND PAUL R. WOLFSON All books, monographs, journal articles, and other publications (including ®lms and other multisensory materials) relating to the history of mathematics are abstracted in the Abstracts Department. The Reviews Department prints extended reviews of selected publications. Materials for review, except books, should be sent to the Abstracts Editor, Professor David E. Zitarelli, Department of Mathematics, Temple University, Philadelphia, Pennsylvania 19122, U.S.A. Books in English for review should be sent to Professor Paul R. Wolfson, Department of Mathematics, West Chester University, West Chester, Pennsylvania 19383, U.S.A. Books in other languages for review should be sent to Professor Catherine Goldstein, BaÃtiment 425, MatheÂmatiques, UniversiteÂde Paris-Sud, F-91405 Orsay Cedex, France. Most reviews are solicited. However, colleagues wishing to review a book are invited to make their wishes known to the appropriate Book Review Editor. (Requests to review books written in the English language should be sent to Prof. Paul R. Wolfson at the above address; requests to review books written in other languages should be sent to Prof. Catherine Goldstein at the above address.) We also welcome retrospective reviews of older books. Colleagues interested in writing such reviews should consult ®rst with the appropriate Book Review Editor (as indicated above, according to the language in which the book is written) to avoid duplication. A History of Complex Dynamics, from SchroÈ der to Fatou and Julia. By Daniel S. Alexander. Wiesbaden (Vieweg). 1994. REVIEWED BY T. W. GAMELIN Mathematics Department, University of California at Los Angeles, Los Angeles, California 90024 The book under review is a readable and engaging account of the development of complex iteration theory over half a century, from Ernst SchroÈ der's landmark pair of papers of 1870±1871 to the work of Pierre Fatou and Gaston Julia appearing in 1917±1920. -
A Spin-Half System As a Working Substance of a Heat Engine: Exploring Its finite-Time Thermodynamic Quantities
A spin-half system as a working substance of a heat engine: exploring its finite-time thermodynamic quantities A Dissertation Submitted to the Department of Physics Addis Ababa University in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy (in Physics) By Tolasa Adugna Dima Advisor Dr. Mulugeta Bekele (Assoc. Professor), Addis Ababa University June 27, 2017 Declaration I hereby declare that except where specific reference is made to the work of others,the contents of this dissertation are original and have not been submitted in whole or in part for consideration for any other degree or qualification in this, or any other University. This dissertation is the result of my own work and that all sources of material used for the dissertation have been duly acknowledged. Name: Tolasa Adugna Dima Signature: Date: This PhD dissertation has been submitted for examination with my approval as uni- versity advisor. Advisor’s Name: Dr. Mulugeta Bekele Signature: Date: Approved by the Examination Committee Signature Date External Examiner: Prof. Purushotam D. Gujrati Internal Examiner: Dr. Lemi Demeyu Thesis Advisor: Dr. Mulugeta Bekele Chairman: Dr. Deribe Hirpo i This work is dedicated solely to Hawi B. Mosissa. ii Acknowledgements First and above all, I praise Waaqayyo, the almighty for providing me the opportunity to do this work. Next, my special thank goes to my advisor Dr. Mulugeta Bekele for his unreserved support throughout my study. From his friendly approach and fa- therhood advice, I have learned and shared lots of experiences. My sincere thanks also goes to Dr. Lemi Demeyu, course instructor and ex-head of physics Department, AAU, for his encouragement, valuable comments and support during my PhD study. -
David Elsing
Department of Physics and Astronomy University of Heidelberg Bachelor Thesis in Physics submitted by David Elsing born in Freiburg im Breisgau (Germany) 2018 Plasma screening effects in laser-generated plasmas This Bachelor Thesis has been carried out by David Elsing at the Max Planck Institute for Nuclear Physics in Heidelberg under the supervision of PD Dr. Adriana P´alffy-Bußand Dr. Yuanbin Wu Abstract Plasma screening effects affect the rate at which nuclear reactions occur in hot and dense astrophysical plasmas. Their direct measurement in the laboratory has not succeeded so far and is vital for our understanding of nuclear processes occurring in stellar nucle- osynthesis. A promising route for such measurements involve petawatt laser facilities capable of producing hot and dense plasmas in the laboratory. In this work, we consider and compare theoretically four plasma screening models originally introduced for astro- physical plasmas, and apply them to nuclear reactions in laser-generated plasmas for a large range of densities and temperatures. We consider two astrophysically relevant nuclear reactions, namely 13C(α; n) 16O, which is one of the important helium burning processes in advanced stellar phases as well as one of the interesting neutron sources for the slow neutron caption process of nucleosynthesis, and 7Li(d; α)α, which might be the key to explain the lithium production problem of the standard big bang nucle- osynthesis. Our results anticipate experiments on nuclear reactions in plasmas being rendered possible at high power laser facilities such as the Extreme Light Infrastructure under construction today, and shedding light on the validity of plasma screening models. -
Lucjan Emil Böttcher (1872‒1937) ‒ the Polish Pioneer of Holomorphic Dynamics
TECHNICAL TRANSACTIONS CZASOPISMO TECHNICZNE FUNDAMENTAL SCIENCES NAUKI PODSTAWOWE 1-NP/2014 MAŁGORZATA STAWISKA* LUCJAN EMIL BÖTTCHER (1872‒1937) ‒ THE POLISH PIONEER OF HOLOMORPHIC DYNAMICS LUCJAN EMIL BÖTTCHER (1872‒1937) ‒ POLSKI PIONIER DYNAMIKI HOLOMORFICZNEJ Abstract In this article I present Lucjan Emil Böttcher (1872‒1937), a little-known Polish mathematician active in Lwów. I outline his scholarly path and describe briefly his mathematical achievements. In view of later developments in holomorphic dynamics, I argue that, despite some flaws in his work, Böttcher should be regarded not only as a contributor to the area but in fact as one of its founders. Keywords: mathematics of the 19th and 20th century, holomorphic dynamics, iterations of rational functions Streszczenie W artykule tym przedstawiam Lucjana Emila Böttchera (1872‒1937), mało znanego matema- tyka polskiego działającego we Lwowie. Szkicuję jego drogę naukową oraz opisuję pokrótce jego osiągnięcia matematyczne. W świetle późniejszego rozwoju dynamiki holomorficznej do- wodzę, że mimo pewnych wad jego prac należy nie tylko docenić wkład Böttchera w tę dzie- dzinę, ale w istocie zaliczyć go do jej twórców. Słowa kluczowe: matematyka XIX i XX wieku, dynamika holomorficzna, iteracje funkcji wymiernych * Małgorzata Stawiska, Mathematical Reviews, 416 Fourth St., Ann Arbor, MI 48103, USA, email: [email protected]. 234 1. Introduction Holomorphic dynamics – in particular the study of iteration of rational maps on the Riemann sphere – is an active area of current mathematical