Molecular Theory and Modeling Chemical Engineering, 698D

Total Page:16

File Type:pdf, Size:1020Kb

Molecular Theory and Modeling Chemical Engineering, 698D Molecular Theory and Modeling Chemical Engineering, 698D Edward J. Maginn University of Notre Dame Notre Dame, IN 46556 USA ­c 1997 Edward Maginn 2 Contents Preface iii 1 Outline and Scope 1 1.1Definitions................................................ 1 1.2 Synopsis ................................................. 1 1.3 Outline of Statistical Mechanics Section . ............................. 2 1.4 Outline of Molecular Simulation Section . ............................. 3 2 Introduction 5 2.1HistoricalPerspective.......................................... 5 2.2LinkBetweenMicroscopicandMacroscopic............................. 6 2.3PracticalProblems........................................... 6 2.3.1 MaterialDesign......................................... 6 2.3.2 Thermophysical Property Estimation ............................. 9 2.4ReviewofSomeMathematicsandStatistics.............................. 9 2.4.1 Probability . ........................................ 9 2.4.2 Counting............................................ 12 2.4.3 Distributions . ........................................ 14 2.4.4 Stirling’s Approximation . .................................. 17 2.4.5 Lagrange Multipliers ...................................... 18 3 Elementary Concepts in Mechanics and Phase Space 21 3.1GeneralizedCoordinates........................................ 21 3.2 Review of Classical Mechanics . .................................. 22 3.2.1 NewtonianMechanics..................................... 22 3.2.2 LagrangianMechanics..................................... 24 3.2.3 HamiltonianMechanics.................................... 25 3.3 Phase Space and Ergodicity ....................................... 26 3.4 Probability Density and the Liouville Equation ............................ 27 3.4.1 Probability Density ....................................... 28 3.4.2 Evolution of Probability Density – Engineering Approach .................. 29 3.5 Ergodicity and Mixing in Phase Space ................................. 30 3.5.1 Ergodic Flow . ........................................ 31 3.5.2 MixingFlow.......................................... 33 4 Equilibrium Ensembles 35 4.1BasicPostulates............................................. 35 4.2 Microcanonical Ensemble ....................................... 35 i ii CONTENTS 4.2.1 Connection With Thermodynamics . ............................. 37 4.2.2 Second Law of Thermodynamics . ............................. 38 4.2.3 Third Law of Thermodynamics . ............................. 40 4.3 Canonical Ensemble . ........................................ 40 4.3.1 Relationship Between the Canonical Ensemble and Thermodynamics ............ 43 4.3.2 Using the Canonical Ensemble ................................. 45 4.4ElementaryStatisticalMechanicsofFluids.............................. 46 4.4.1 Thermophysical Properties of Ideal Gases ........................... 51 4.4.2 Thermodynamic Properties from Ensemble Averages . .................. 53 4.5OtherEnsembles............................................ 58 4.5.1 Grand Canonical Ensemble . .................................. 58 4.5.2 Isothermal–Isobaric(NPT)Ensemble............................. 62 4.6EquivalenceofEnsembles-Preliminaries............................... 62 4.6.1 EquivalenceofEnsembles-AnExample........................... 64 5 Application of Ensemble Theory: Mean Field Theories 65 5.1 Introduction and Motivation ...................................... 65 5.2MeanFieldApproximations...................................... 65 5.3RegularSolutionTheory........................................ 66 5.4Quasi–ChemicalApproximation.................................... 71 5.4.1 QCAAssumptions....................................... 71 5.4.2 Outline of QCA Derivation . .................................. 71 5.5vanderWaalsEquationofState.................................... 73 5.6Solids:EinsteinModel......................................... 79 5.7 Adsorption: Lattice Gas Models . .................................. 80 5.8PolymerChains............................................. 87 5.8.1 MeanFieldPolymerFormulation............................... 88 6 Intermolecular Interactions 93 6.1 Introduction . ............................................. 93 6.2ConfigurationalEnergy......................................... 94 6.3TypesofIntermolecularInteraction................................... 95 6.4Short–RangeRepulsionInteraction................................... 96 6.5DispersionInteractions......................................... 97 6.6 Composite Potential Energy Functions for Non–Polar Molecules . .................. 98 7 Distribution Functions in Classical Monatomic Liquids 101 7.1 Introduction and Physical Interpretations . .............................101 7.2 Development of Equations Describing Distribution Functions . ..................102 7.3 The Pair Distribution Function . ..................................104 ´Ö µ 7.3.1 Physical Interpretation of g .................................104 ´Ö µ 7.4 Experimental Measurement of g ...................................107 7.5 Thermodynamics From the Radial Distribution Function .......................108 7.5.1 InternalEnergy.........................................109 7.5.2 Pressure .............................................110 7.5.3 Compressibility Equation . ..................................111 7.5.4 PotentialofMeanForce–TheReversibleWorkTheorem..................111 ´Ö µ 7.6 Getting Thermodynamics From g ..................................112 7.6.1 Low Density Limit of the Pair Distribution Function . ..................114 CONTENTS iii 7.6.2 IntegralEquationApproach–BGYEquation.........................115 7.6.3 AnotherApproach–TheDirectCorrelationFunction.....................117 7.6.4 Solving the OZ Equation – The Percus–Yevick and Hyper–netted Chain Approximations . 118 7.6.5 ThePYSolutionForHardSpheres..............................120 8 Introduction to Molecular Simulation Techniques 125 8.1ConstructionofaMolecularModel...................................125 8.2 Model System Size and Periodic Boundary Conditions . .......................129 9 Monte Carlo Methods 133 9.1 Historical Background . ........................................133 9.2MonteCarloasanIntegrationMethod.................................134 9.3ImportanceSampling..........................................138 9.3.1 MarkovChains.........................................138 9.3.2 The Metropolis Monte Carlo Algorithm ............................140 9.3.3 FlowofCalculationsinMetropolisMonteCarlo.......................142 9.3.4 Example: Canonical Ensemble MC of a Simple Liquid . ..................143 9.3.5 Metropolis Method: Implementation Specifics . .......................144 9.3.6 OtherTechnicalConsiderations................................145 9.4 Application of Metropolis Monte Carlo: Ising Lattice . .......................146 9.5 Grand Canonical Monte Carlo Simulations . .............................147 9.6GibbsEnsembleMonteCarlo......................................150 9.6.1 GeneralizationoftheGibbsTechnique.............................153 9.6.2 AdditionalComputationalDetailsforMonteCarloSimulations...............154 10 Molecular Dynamics Methods 157 10.1 Introduction . .............................................157 10.2FormulationoftheMolecularDynamicsMethod...........................157 10.3SomeGeneralFeaturesoftheEquationsofMotion..........................159 10.4 Difference Methods for the Integration of Dynamical Equations . ..................159 10.4.1 Algorithmic Considerations in MD . .............................160 10.4.2 Gear Predictor–Corrector Methods . .............................161 10.4.3 The Verlet Algorithm ......................................162 10.4.4 The Leap–Frog Verlet Algorithm . .............................163 10.5MolecularDynamicsofRigidNon-LinearPolyatomicMolecules...................164 10.5.1ConstraintDynamics......................................167 10.5.2 General Comments on the Choice of Algorithms .......................170 10.6MolecularDynamicsInOtherEnsembles...............................170 10.6.1 Stochastic Methods .......................................171 10.6.2 Extended System Methods . ..................................171 10.6.3 Constraint Methods .......................................172 10.7StructuralInformationFromMD(andMC)..............................173 10.7.1 Pair Distribution Functions . ..................................173 10.7.2MolecularOrientation.....................................175 10.8 Dynamical Information From Equilibrium MD ............................175 10.9TransportCoefficientsFromCorrelationFunctions..........................178 10.9.1TransportCoefficientsFromMD................................179 10.9.2ComputingCorrelationFunctionsFromMDRuns......................181 10.9.3 General Considerations For Writing an MD Code .......................182 iv CONTENTS 10.9.4StructuringtheProgram....................................183 Preface If, in some cataclysm, all of scientific knowledge were to be destroyed, and only one sentence passed on to the next generations of creatures, what statement would contain the most information in the fewest words? I believe it is the atomic hypothesis (or the atomic fact, or whatever you wish to call it) that all things are made of atoms-little particles that move around in perpetual motion, attracting each other when they are a little distance apart, but repelling upon being squeezed into one another. In that one sentence, you will see, there is an enormous amount of information
Recommended publications
  • 2D Potts Model Correlation Lengths
    KOMA Revised version May D Potts Mo del Correlation Lengths Numerical Evidence for = at o d t Wolfhard Janke and Stefan Kappler Institut f ur Physik Johannes GutenbergUniversitat Mainz Staudinger Weg Mainz Germany Abstract We have studied spinspin correlation functions in the ordered phase of the twodimensional q state Potts mo del with q and at the rstorder transition p oint Through extensive Monte t Carlo simulations we obtain strong numerical evidence that the cor relation length in the ordered phase agrees with the exactly known and recently numerically conrmed correlation length in the disordered phase As a byproduct we nd the energy moments o t t d in the ordered phase at in very go o d agreement with a recent large t q expansion PACS numbers q Hk Cn Ha hep-lat/9509056 16 Sep 1995 Introduction Firstorder phase transitions have b een the sub ject of increasing interest in recent years They play an imp ortant role in many elds of physics as is witnessed by such diverse phenomena as ordinary melting the quark decon nement transition or various stages in the evolution of the early universe Even though there exists already a vast literature on this sub ject many prop erties of rstorder phase transitions still remain to b e investigated in detail Examples are nitesize scaling FSS the shap e of energy or magnetization distributions partition function zeros etc which are all closely interrelated An imp ortant approach to attack these problems are computer simulations Here the available system sizes are necessarily
    [Show full text]
  • Full and Unbiased Solution of the Dyson-Schwinger Equation in the Functional Integro-Differential Representation
    PHYSICAL REVIEW B 98, 195104 (2018) Full and unbiased solution of the Dyson-Schwinger equation in the functional integro-differential representation Tobias Pfeffer and Lode Pollet Department of Physics, Arnold Sommerfeld Center for Theoretical Physics, University of Munich, Theresienstrasse 37, 80333 Munich, Germany (Received 17 March 2018; revised manuscript received 11 October 2018; published 2 November 2018) We provide a full and unbiased solution to the Dyson-Schwinger equation illustrated for φ4 theory in 2D. It is based on an exact treatment of the functional derivative ∂/∂G of the four-point vertex function with respect to the two-point correlation function G within the framework of the homotopy analysis method (HAM) and the Monte Carlo sampling of rooted tree diagrams. The resulting series solution in deformations can be considered as an asymptotic series around G = 0 in a HAM control parameter c0G, or even a convergent one up to the phase transition point if shifts in G can be performed (such as by summing up all ladder diagrams). These considerations are equally applicable to fermionic quantum field theories and offer a fresh approach to solving functional integro-differential equations beyond any truncation scheme. DOI: 10.1103/PhysRevB.98.195104 I. INTRODUCTION was not solved and differences with the full, exact answer could be seen when the correlation length increases. Despite decades of research there continues to be a need In this work, we solve the full DSE by writing them as a for developing novel methods for strongly correlated systems. closed set of integro-differential equations. Within the HAM The standard Monte Carlo approaches [1–5] are convergent theory there exists a semianalytic way to treat the functional but suffer from a prohibitive sign problem, scaling exponen- derivatives without resorting to an infinite expansion of the tially in the system volume [6].
    [Show full text]
  • Notes on Statistical Field Theory
    Lecture Notes on Statistical Field Theory Kevin Zhou [email protected] These notes cover statistical field theory and the renormalization group. The primary sources were: • Kardar, Statistical Physics of Fields. A concise and logically tight presentation of the subject, with good problems. Possibly a bit too terse unless paired with the 8.334 video lectures. • David Tong's Statistical Field Theory lecture notes. A readable, easygoing introduction covering the core material of Kardar's book, written to seamlessly pair with a standard course in quantum field theory. • Goldenfeld, Lectures on Phase Transitions and the Renormalization Group. Covers similar material to Kardar's book with a conversational tone, focusing on the conceptual basis for phase transitions and motivation for the renormalization group. The notes are structured around the MIT course based on Kardar's textbook, and were revised to include material from Part III Statistical Field Theory as lectured in 2017. Sections containing this additional material are marked with stars. The most recent version is here; please report any errors found to [email protected]. 2 Contents Contents 1 Introduction 3 1.1 Phonons...........................................3 1.2 Phase Transitions......................................6 1.3 Critical Behavior......................................8 2 Landau Theory 12 2.1 Landau{Ginzburg Hamiltonian.............................. 12 2.2 Mean Field Theory..................................... 13 2.3 Symmetry Breaking.................................... 16 3 Fluctuations 19 3.1 Scattering and Fluctuations................................ 19 3.2 Position Space Fluctuations................................ 20 3.3 Saddle Point Fluctuations................................. 23 3.4 ∗ Path Integral Methods.................................. 24 4 The Scaling Hypothesis 29 4.1 The Homogeneity Assumption............................... 29 4.2 Correlation Lengths.................................... 30 4.3 Renormalization Group (Conceptual)..........................
    [Show full text]
  • 10 Basic Aspects of CFT
    10 Basic aspects of CFT An important break-through occurred in 1984 when Belavin, Polyakov and Zamolodchikov [BPZ84] applied ideas of conformal invariance to classify the possible types of critical behaviour in two dimensions. These ideas had emerged earlier in string theory and mathematics, and in fact go backto earlier (1970) work of Polyakov [Po70] in which global conformal invariance is used to constrain the form of correlation functions in d-dimensional the- ories. It is however only by imposing local conformal invariance in d =2 that this approach becomes really powerful. In particular, it immediately permitted a full classification of an infinite family of conformally invariant theories (the so-called “minimal models”) having a finite number of funda- mental (“primary”) fields, and the exact computation of the corresponding critical exponents. In the aftermath of these developments, conformal field theory (CFT) became for some years one of the most hectic research fields of theoretical physics, and indeed has remained a very active area up to this date. This chapter focusses on the basic aspects of CFT, with a special emphasis on the ingredients which will allow us to tackle the geometrically defined loop models via the so-called Coulomb Gas (CG) approach. The CG technique will be exposed in the following chapter. The aim is to make the presentation self- contained while remaining rather brief; the reader interested in more details should turn to the comprehensive textbook [DMS87] or the Les Houches volume [LH89]. 10.1 Global conformal invariance A conformal transformation in d dimensions is an invertible mapping x x′ → which multiplies the metric tensor gµν (x) by a space-dependent scale factor: gµ′ ν (x′)=Λ(x)gµν (x).
    [Show full text]
  • Arxiv:1910.10745V1 [Cond-Mat.Str-El] 23 Oct 2019 2.2 Symmetry-Protected Time Crystals
    A Brief History of Time Crystals Vedika Khemania,b,∗, Roderich Moessnerc, S. L. Sondhid aDepartment of Physics, Harvard University, Cambridge, Massachusetts 02138, USA bDepartment of Physics, Stanford University, Stanford, California 94305, USA cMax-Planck-Institut f¨urPhysik komplexer Systeme, 01187 Dresden, Germany dDepartment of Physics, Princeton University, Princeton, New Jersey 08544, USA Abstract The idea of breaking time-translation symmetry has fascinated humanity at least since ancient proposals of the per- petuum mobile. Unlike the breaking of other symmetries, such as spatial translation in a crystal or spin rotation in a magnet, time translation symmetry breaking (TTSB) has been tantalisingly elusive. We review this history up to recent developments which have shown that discrete TTSB does takes place in periodically driven (Floquet) systems in the presence of many-body localization (MBL). Such Floquet time-crystals represent a new paradigm in quantum statistical mechanics — that of an intrinsically out-of-equilibrium many-body phase of matter with no equilibrium counterpart. We include a compendium of the necessary background on the statistical mechanics of phase structure in many- body systems, before specializing to a detailed discussion of the nature, and diagnostics, of TTSB. In particular, we provide precise definitions that formalize the notion of a time-crystal as a stable, macroscopic, conservative clock — explaining both the need for a many-body system in the infinite volume limit, and for a lack of net energy absorption or dissipation. Our discussion emphasizes that TTSB in a time-crystal is accompanied by the breaking of a spatial symmetry — so that time-crystals exhibit a novel form of spatiotemporal order.
    [Show full text]
  • Introduction to Two-Dimensional Conformal Field Theory
    Introduction to two-dimensional conformal field theory Sylvain Ribault CEA Saclay, Institut de Physique Th´eorique [email protected] February 5, 2019 Abstract We introduce conformal field theory in two dimensions, from the basic principles to some of the simplest models. From the representations of the Virasoro algebra on the one hand, and the state-field correspondence on the other hand, we deduce Ward identities and Belavin{Polyakov{Zamolodchikov equations for correlation functions. We then explain the principles of the conformal bootstrap method, and introduce conformal blocks. This allows us to define and solve minimal models and Liouville theory. We also introduce the free boson with its abelian affine Lie algebra. Lecture notes for the \Young Researchers Integrability School", Wien 2019, based on the earlier lecture notes [1]. Estimated length: 7 lectures of 45 minutes each. Material that may be skipped in the lectures is in green boxes. Exercises are in green boxes when their statements are not part of the lectures' text; this does not make them less interesting as exercises. 1 Contents 0 Introduction2 1 The Virasoro algebra and its representations3 1.1 Algebra.....................................3 1.2 Representations.................................4 1.3 Null vectors and degenerate representations.................5 2 Conformal field theory6 2.1 Fields......................................6 2.2 Correlation functions and Ward identities...................8 2.3 Belavin{Polyakov{Zamolodchikov equations................. 10 2.4 Free boson.................................... 10 3 Conformal bootstrap 12 3.1 Single-valuedness................................ 12 3.2 Operator product expansion and crossing symmetry............. 13 3.3 Degenerate fields and the fusion product................... 16 4 Minimal models 17 4.1 Diagonal minimal models...........................
    [Show full text]
  • 10. Interacting Matter 10.1. Classical Real
    10. Interacting matter The grand potential is now Ω= k TVω(z,T ) 10.1. Classical real gas − B We take into account the mutual interactions of atoms and (molecules) p Ω The Hamiltonian operator is = = ω(z,T ) kBT −V N p2 N ∂ω(z,T ) H(N) = i + v(r ), r = r r . ρ = = z . 2m ij ij | i − j | V ∂z i=1 i<j X X Eliminating z we can write the equation of state as For example, for noble gases a good approximation of the p = k T ϕ(ρ,T ). interaction potential is the Lennard-Jones 6–12 -potential B Expanding ϕ as the power series of ρ we end up with the σ 12 σ 6 v(r)=4ǫ . virial expansion. r − r Ursell-Mayer graphs V ( r ) Let’s write Q = dr r e−βv(rij ) N 1 · · · N i<j Z Y r 0 s r 6 = dr r (1 + f ), e 1 / r 1 · · · N ij Z i<j We evaluate the partition sums in the classical phase Y where space. The canonical partition function is f = f(r )= e−βv(rij ) 1 ij ij − −βH(N) ZN (T, V )= Z(T,V,N) = Tr N e is Mayer’s function. 1 V ( r ) dΓ e−βH . classical−→ N! limit, Maxwell- Z f ( r ) Boltzman Because the momentum variables appear only r quadratically, they can be integrated and we obtain - 1 1 1 The function f is bounded everywhere and it has the ZN = dp1 dpN dr1 drN same range as the potential v.
    [Show full text]
  • Lecture 6: Entropy
    Matthew Schwartz Statistical Mechanics, Spring 2019 Lecture 6: Entropy 1 Introduction In this lecture, we discuss many ways to think about entropy. The most important and most famous property of entropy is that it never decreases Stot > 0 (1) Here, Stot means the change in entropy of a system plus the change in entropy of the surroundings. This is the second law of thermodynamics that we met in the previous lecture. There's a great quote from Sir Arthur Eddington from 1927 summarizing the importance of the second law: If someone points out to you that your pet theory of the universe is in disagreement with Maxwell's equationsthen so much the worse for Maxwell's equations. If it is found to be contradicted by observationwell these experimentalists do bungle things sometimes. But if your theory is found to be against the second law of ther- modynamics I can give you no hope; there is nothing for it but to collapse in deepest humiliation. Another possibly relevant quote, from the introduction to the statistical mechanics book by David Goodstein: Ludwig Boltzmann who spent much of his life studying statistical mechanics, died in 1906, by his own hand. Paul Ehrenfest, carrying on the work, died similarly in 1933. Now it is our turn to study statistical mechanics. There are many ways to dene entropy. All of them are equivalent, although it can be hard to see. In this lecture we will compare and contrast dierent denitions, building up intuition for how to think about entropy in dierent contexts. The original denition of entropy, due to Clausius, was thermodynamic.
    [Show full text]
  • Spinning Test Particle in Four-Dimensional Einstein–Gauss–Bonnet Black Holes
    universe Communication Spinning Test Particle in Four-Dimensional Einstein–Gauss–Bonnet Black Holes Yu-Peng Zhang 1,2, Shao-Wen Wei 1,2 and Yu-Xiao Liu 1,2,3* 1 Joint Research Center for Physics, Lanzhou University and Qinghai Normal University, Lanzhou 730000 and Xining 810000, China; [email protected] (Y.-P.Z.); [email protected] (S.-W.W.) 2 Institute of Theoretical Physics & Research Center of Gravitation, Lanzhou University, Lanzhou 730000, China 3 Key Laboratory for Magnetism and Magnetic of the Ministry of Education, Lanzhou University, Lanzhou 730000, China * Correspondence: [email protected] Received: 27 June 2020; Accepted: 27 July 2020; Published: 28 July 2020 Abstract: In this paper, we investigate the motion of a classical spinning test particle in a background of a spherically symmetric black hole based on the novel four-dimensional Einstein–Gauss–Bonnet gravity [D. Glavan and C. Lin, Phys. Rev. Lett. 124, 081301 (2020)]. We find that the effective potential of a spinning test particle in this background could have two minima when the Gauss–Bonnet coupling parameter a is nearly in a special range −8 < a/M2 < −2 (M is the mass of the black hole), which means a particle can be in two separate orbits with the same spin-angular momentum and orbital angular momentum, and the accretion disc could have discrete structures. We also investigate the innermost stable circular orbits of the spinning test particle and find that the corresponding radius could be smaller than the cases in general relativity. Keywords: Gauss–Bonnet; innermost stable circular orbits; spinning test particle 1.
    [Show full text]
  • Dirty Tricks for Statistical Mechanics
    Dirty tricks for statistical mechanics Martin Grant Physics Department, McGill University c MG, August 2004, version 0.91 ° ii Preface These are lecture notes for PHYS 559, Advanced Statistical Mechanics, which I’ve taught at McGill for many years. I’m intending to tidy this up into a book, or rather the first half of a book. This half is on equilibrium, the second half would be on dynamics. These were handwritten notes which were heroically typed by Ryan Porter over the summer of 2004, and may someday be properly proof-read by me. Even better, maybe someday I will revise the reasoning in some of the sections. Some of it can be argued better, but it was too much trouble to rewrite the handwritten notes. I am also trying to come up with a good book title, amongst other things. The two titles I am thinking of are “Dirty tricks for statistical mechanics”, and “Valhalla, we are coming!”. Clearly, more thinking is necessary, and suggestions are welcome. While these lecture notes have gotten longer and longer until they are al- most self-sufficient, it is always nice to have real books to look over. My favorite modern text is “Lectures on Phase Transitions and the Renormalisation Group”, by Nigel Goldenfeld (Addison-Wesley, Reading Mass., 1992). This is referred to several times in the notes. Other nice texts are “Statistical Physics”, by L. D. Landau and E. M. Lifshitz (Addison-Wesley, Reading Mass., 1970) par- ticularly Chaps. 1, 12, and 14; “Statistical Mechanics”, by S.-K. Ma (World Science, Phila., 1986) particularly Chaps.
    [Show full text]
  • Generalized Molecular Chaos Hypothesis and the H-Theorem: Problem of Constraints and Amendment of Nonextensive Statistical Mechanics
    Generalized molecular chaos hypothesis and the H-theorem: Problem of constraints and amendment of nonextensive statistical mechanics Sumiyoshi Abe1,2,3 1Department of Physical Engineering, Mie University, Mie 514-8507, Japan*) 2Institut Supérieur des Matériaux et Mécaniques Avancés, 44 F. A. Bartholdi, 72000 Le Mans, France 3Inspire Institute Inc., McLean, Virginia 22101, USA Abstract Quite unexpectedly, kinetic theory is found to specify the correct definition of average value to be employed in nonextensive statistical mechanics. It is shown that the normal average is consistent with the generalized Stosszahlansatz (i.e., molecular chaos hypothesis) and the associated H-theorem, whereas the q-average widely used in the relevant literature is not. In the course of the analysis, the distributions with finite cut-off factors are rigorously treated. Accordingly, the formulation of nonextensive statistical mechanics is amended based on the normal average. In addition, the Shore- Johnson theorem, which supports the use of the q-average, is carefully reexamined, and it is found that one of the axioms may not be appropriate for systems to be treated within the framework of nonextensive statistical mechanics. PACS number(s): 05.20.Dd, 05.20.Gg, 05.90.+m ____________________________ *) Permanent address 1 I. INTRODUCTION There exist a number of physical systems that possess exotic properties in view of traditional Boltzmann-Gibbs statistical mechanics. They are said to be statistical- mechanically anomalous, since they often exhibit and realize broken ergodicity, strong correlation between elements, (multi)fractality of phase-space/configuration-space portraits, and long-range interactions, for example. In the past decade, nonextensive statistical mechanics [1,2], which is a generalization of the Boltzmann-Gibbs theory, has been drawing continuous attention as a possible theoretical framework for describing these systems.
    [Show full text]
  • LECTURE 9 Statistical Mechanics Basic Methods We Have Talked
    LECTURE 9 Statistical Mechanics Basic Methods We have talked about ensembles being large collections of copies or clones of a system with some features being identical among all the copies. There are three different types of ensembles in statistical mechanics. 1. If the system under consideration is isolated, i.e., not interacting with any other system, then the ensemble is called the microcanonical ensemble. In this case the energy of the system is a constant. 2. If the system under consideration is in thermal equilibrium with a heat reservoir at temperature T , then the ensemble is called a canonical ensemble. In this case the energy of the system is not a constant; the temperature is constant. 3. If the system under consideration is in contact with both a heat reservoir and a particle reservoir, then the ensemble is called a grand canonical ensemble. In this case the energy and particle number of the system are not constant; the temperature and the chemical potential are constant. The chemical potential is the energy required to add a particle to the system. The most common ensemble encountered in doing statistical mechanics is the canonical ensemble. We will explore many examples of the canonical ensemble. The grand canon- ical ensemble is used in dealing with quantum systems. The microcanonical ensemble is not used much because of the difficulty in identifying and evaluating the accessible microstates, but we will explore one simple system (the ideal gas) as an example of the microcanonical ensemble. Microcanonical Ensemble Consider an isolated system described by an energy in the range between E and E + δE, and similar appropriate ranges for external parameters xα.
    [Show full text]