Maxwell's Contributions to Thermal Physics

Total Page:16

File Type:pdf, Size:1020Kb

Maxwell's Contributions to Thermal Physics GENERAL I ARTICLE Maxwell's Contributions to Thermal Physics Sisir Bhanja Introduction James Clerk Maxwell (1831-1879) was one of the great­ est theoretIcal physicists of the nineteenth century. He is remembered for his pioneering contributions to di­ verse fields of mathematical physics. His work in ther­ Sisir Bhanja did his Ph D mal physics bears two distinct approaches: from the Indian Associa­ tion for the Cultivation of 1. Thermodynamics or the macroscopic description, Science, Kolkata. Apart from his doctoral work on and the physics of molecular collisions, he did some 2. Kinetic theory or the molecular and statistical ap­ work on Mossbauer proach. effect. He retired some time back from the We discuss both these approaches in this article. Department of Physics, St Xavier's College, Kolkata, Maxwell's Work in Thermodynamics where he taught for a number of years. Maxwell's main work in the field of thermodynamics ~urrently, he is pursuing consists of the group of thermodynamic relations (in­ studies in gravitation and volving the entropy'S', the volume 'V' and the temper­ cosmology. ature 'T') which are named after him. He derived these relations by combining the two laws of thermodynamics, namely, a) The First Law: dQ = dU + PdV and b) the Second Law: dQ = TdS, where dU is the change in the internal energy U. Com­ bining these two laws, we have dU = TdS - PdV. Keywords Maxwell's thermodynamic re- . Maxwell noted that since dU is a perfect differential, lations, velocity distribution law, coefficient of viscosity. -RE-S-O-N-A-N-C-E--I-M-a-y-2-0-03--------------~-----------------------------~- GENERAL I ARTICLE for U = U(x, y), where x, yare two independent vari­ ables, from which we obtain J (T, S) = J (P, V) , x,y x,y where the Jacobian J(T,S) = 8(T,S) = (8T/8X 8T/8Y) x, y 8(x, y) 8S/8x 8S/8y . The four relations then appear as follows: Relation 1 : Putting x = T and y = V, (8S/8V)T = (8P/aT)v· Relation 2 : Putting x = T and y = P, (8S/8P)T = -(8V/8T)p. Relation 3 : Putting x = Sand y = V, (aT/8V)s = -(8P/8S)v. Relation 4 : Putting x = Sand y == P, (aT/8P)s = (8V/8S)p. These relations due to Maxwell are enormously useful in providing relationship "between measurable quanti­ ties and those which either cannot be measured or are difficult to measure", as is shown with two illustrations given below. From Relation 2 we have, on multiplying through by T and noting that T dS = dQ, (8Q/8P)T = -T(8V/aT)p = - V-I (8V/aT)p VT, = -0 VT, I where 0 = V- (8V/8T)p is the isobaric coefficient of volume expansion. -58------------------------~------------RE-S-O-NA-N-C-E-I-M-a-Y-2-00-3 GENERAL I ARTICLE Thus, for substances which expand on heating, a > 0, so that (8Q/8P)T < 0 which implies that an amount of heat must be taken away from the substance when the pressure is increased in order that the process re­ mains isothermal. In other words, when a substance with a positive expansion coefficient is compressed, heat is generated. For substances which contract on heat­ ing, cooling should take place. Nature is replete with such examples and Maxwell's relations provide the due explanations. Our second illustration follows from Relation 1 multi­ plying through by T which leads to (8Q/8V)T = T(8P/aT)v. The left-hand side describes a process in which supply of heat does not change the temperature but alters the volume isothermally, as is seen in a change of state. The above relation thus tells us where 112 and VI are the respective volumes and L, the latent heat of fusion. The quantities on the left-hand side are easily observable experimentally and allow us to calculate (8P/aT)v. As an example, we calculate the change in the freezing point of water due to change in the pressure. We note the following: freezing point of water under normal conditions is 273.16K, L, the latent heat of fusion of ice is SOcal/gm = SO x 4.1S6 x 107erg/gm, the specific volumes V2 = 1.0001cm3 /gm for water and Vi = 1.090Scm3/gm for ice. For a change of pressure 8P = 1atmosph~re = 1.013 x 106dynescm -2, the consequent change of the melting -RE-S-O-N-A-NC-E--I-M-a-Y-2-00-3------------~~-------------------------5-9 GENERAL I ARTICLE point 8T = -O.0075°C, i.e., the melting point is lowered for substances such as water which contract on melting. In the reverse case, i.e., for substances which contract on solidification, the melting point rises consequent to an increase of pressure. These relations are of immense use not only to physics, also in engineering practices. Kinetic Theory The thermodynamic approach does not allow a calcula­ tion of the quantities involved, based on the first princi­ ples e.g., to calculate U, we must know the mechanism that contributes to U. The microscopic description of molecular motion, as given in the pioneering work of Maxwell, really solves these problems. Maxwell's work in this area provided a breakthrough by demonstrat­ ing the real importance of molecular motion (which still had its sceptics) in understanding thermal phenomena and the importance of statistics. Maxwell deduced the law of distribution of velocities from considerations of probabilities "far in advance of anything previously at­ tempted on the subject" H~s ideas, though simplified, did hit upon some of the essentials, as are elaborated below. (a) The gas molecules are point masses. The system is considered to be in equilibrium, external disturbances being totally absent. (In fact, the equilibrium follows from the elastic collisions between molecules which are in continual motion, as was pointed out by L Boltz­ mann, another great player in this field who was almost contemporary to Maxwell). (b) To meet the requirements of statistical considera­ tions, the system must be assumed to be made up of a very large number of molecules; there should be an equal number of molecules in any given volume 8V within the system. In other words, the system should be homoge- --------~-------- 60 RESONANCE I May 2003 GENERAL I ARTICLE ( c) The motion of the molecules is totally random such that the molecules have the same velocities in all direc­ tions. As a consequence of this isotropy the components of velocities along any system of coordinates are equal and it is immaterial which coordinate system the results are expressed in. (d) The velocity components (u, v, w) along any three coordinates (x, y, z) are uncorrelated to each other. The quantities (u, v, w) being uncorrelated, their probabili­ ties are also independent of each other. (e) The probability function describing the molecules with a particular velocity component v in the interval v to v + dv is dependent only on v and the element dv. All these assumptions were obviously consistent with the observed facts about the randomness of molecular motion leading to uniform bulk properties like density, temperature, etc. throughout the entire volume of the gaseous system in equilibrium. Now, with 0 as the origin of a rectangular Cartesian system of coordiantes (x, y, z) and (u, v, w) as the corresponding triad of ve­ locity components, the resultant velocity c is related to (u, v, w) by (1) To calculate the probability of a molecule to have a ve­ locity between c and c + dc, the same can be calculated component-wise. If dnu be the number of molecules per unit volume which have the x-component of velocity be­ tween u and u + du, then the corresponding probability function P(u, du) = dnu/n = f{u) du, (2) where n is the total number of molecules per unit vol­ ume. On similar considerations, the corresponding pro b­ abilities for a molecule to have the y-component of veloc­ ity between v and v+dv and the z-component of velocity -RE-S-O-N-A-N-C-E-I-M-a-Y-2-0-0-3------------~-----------------------------61 GENERAL I ARTICLE between wand w + dw may be written respectively as P(v, dv) = dnv/n = f(v) dv and P(w, dw) = dnw/n = f(w) dw. (2a) The functional form has been taken the same for all three velocity components by virtue of assumption (c). So, the effective probability of a molecule having its ve­ locity components between u and u + du, v and v + dv and wand w + dw simultaneously, is given by P(u, v, w, du, dv, dw) = dnu,v,w/n = f(u) f(v) f(w) du dv dw (3) so that the number of molecules within the specified velocity ranges will be dnu,v,w = n f(u) f(v) f(w) du dv dw. (4) The same set of velocity components make a single re­ sultant velocity vector c. All the velocity vectors start from a common origin O. The lengths of these vectors give the magnitudes and their directions are the direc­ tions of motion of the molecules at any given time. If spheres of radii e and e + de are drawn centred at 0, the origin, the vectors ending between these two con­ centric spheres would represent all the velocities present that have values between e and e + de. The chance that this single velocity vector c ends in the volume element du dv dw is, by assumption (e), ¢(e) du dv dw, which may be alternatively written as F(e2)du dv dw = f(u) f(v) f(w) du dv dw (5) valid for any arbitrary range of values of du, dv, dw, i.e.
Recommended publications
  • Statistics of a Free Single Quantum Particle at a Finite
    STATISTICS OF A FREE SINGLE QUANTUM PARTICLE AT A FINITE TEMPERATURE JIAN-PING PENG Department of Physics, Shanghai Jiao Tong University, Shanghai 200240, China Abstract We present a model to study the statistics of a single structureless quantum particle freely moving in a space at a finite temperature. It is shown that the quantum particle feels the temperature and can exchange energy with its environment in the form of heat transfer. The underlying mechanism is diffraction at the edge of the wave front of its matter wave. Expressions of energy and entropy of the particle are obtained for the irreversible process. Keywords: Quantum particle at a finite temperature, Thermodynamics of a single quantum particle PACS: 05.30.-d, 02.70.Rr 1 Quantum mechanics is the theoretical framework that describes phenomena on the microscopic level and is exact at zero temperature. The fundamental statistical character in quantum mechanics, due to the Heisenberg uncertainty relation, is unrelated to temperature. On the other hand, temperature is generally believed to have no microscopic meaning and can only be conceived at the macroscopic level. For instance, one can define the energy of a single quantum particle, but one can not ascribe a temperature to it. However, it is physically meaningful to place a single quantum particle in a box or let it move in a space where temperature is well-defined. This raises the well-known question: How a single quantum particle feels the temperature and what is the consequence? The question is particular important and interesting, since experimental techniques in recent years have improved to such an extent that direct measurement of electron dynamics is possible.1,2,3 It should also closely related to the question on the applicability of the thermodynamics to small systems on the nanometer scale.4 We present here a model to study the behavior of a structureless quantum particle moving freely in a space at a nonzero temperature.
    [Show full text]
  • Physics 357 – Thermal Physics - Spring 2005
    Physics 357 – Thermal Physics - Spring 2005 Contact Info MTTH 9-9:50. Science 255 Doug Juers, Science 244, 527-5229, [email protected] Office Hours: Mon 10-noon, Wed 9-10 and by appointment or whenever I’m around. Description Thermal physics involves the study of systems with lots (1023) of particles. Since only a two-body problem can be solved analytically, you can imagine we will look at these systems somewhat differently from simple systems in mechanics. Rather than try to predict individual trajectories of individual particles we will consider things on a larger scale. Probability and statistics will play an important role in thinking about what can happen. There are two general methods of dealing with such systems – a top down approach and a bottom up approach. In the top down approach (thermodynamics) one doesn’t even really consider that there are particles there, and instead thinks about things in terms of quantities like temperature heat, energy, work, entropy and enthalpy. In the bottom up approach (statistical mechanics) one considers in detail the interactions between individual particles. Building up from there yields impressive predictions of bulk properties of different materials. In this course we will cover both thermodynamics and statistical mechanics. The first part of the term will emphasize the former, while the second part of the term will emphasize the latter. Both topics have important applications in many fields, including solid-state physics, fluids, geology, chemistry, biology, astrophysics, cosmology. The great thing about thermal physics is that in large part it’s about trying to deal with reality.
    [Show full text]
  • Physics, M.S. 1
    Physics, M.S. 1 PHYSICS, M.S. DEPARTMENT OVERVIEW The Department of Physics has a strong tradition of graduate study and research in astrophysics; atomic, molecular, and optical physics; condensed matter physics; high energy and particle physics; plasma physics; quantum computing; and string theory. There are many facilities for carrying out world-class research (https://www.physics.wisc.edu/ research/areas/). We have a large professional staff: 45 full-time faculty (https://www.physics.wisc.edu/people/staff/) members, affiliated faculty members holding joint appointments with other departments, scientists, senior scientists, and postdocs. There are over 175 graduate students in the department who come from many countries around the world. More complete information on the graduate program, the faculty, and research groups is available at the department website (http:// www.physics.wisc.edu). Research specialties include: THEORETICAL PHYSICS Astrophysics; atomic, molecular, and optical physics; condensed matter physics; cosmology; elementary particle physics; nuclear physics; phenomenology; plasmas and fusion; quantum computing; statistical and thermal physics; string theory. EXPERIMENTAL PHYSICS Astrophysics; atomic, molecular, and optical physics; biophysics; condensed matter physics; cosmology; elementary particle physics; neutrino physics; experimental studies of superconductors; medical physics; nuclear physics; plasma physics; quantum computing; spectroscopy. M.S. DEGREES The department offers the master science degree in physics, with two named options: Research and Quantum Computing. The M.S. Physics-Research option (http://guide.wisc.edu/graduate/physics/ physics-ms/physics-research-ms/) is non-admitting, meaning it is only available to students pursuing their Ph.D. The M.S. Physics-Quantum Computing option (http://guide.wisc.edu/graduate/physics/physics-ms/ physics-quantum-computing-ms/) (MSPQC Program) is a professional master's program in an accelerated format designed to be completed in one calendar year..
    [Show full text]
  • Physics Ph.D
    THE UNIVERSITY OF VERMONT PHYSICS PH.D. PHYSICS PH.D. consists of a Ph.D. dissertation proposal given after the start of a dissertation research project. All students must meet the Requirements for the Doctor of Philosophy Degree (http:// Requirements for Advancement to Candidacy for the catalogue.uvm.edu/graduate/degreerequirements/ Degree of Doctor of Philosophy requirementsforthedoctorofphilosophydegree/). Successful completion of all required courses and the comprehensive exam. OVERVIEW The Department of Physics offers research opportunities in theoretical and experimental condensed matter physics, astronomy and astrophysics, and soft condensed matter physics and biophysics. SPECIFIC REQUIREMENTS Requirements for Admission to Graduate Studies for the Degree of Doctor of Philosophy Undergraduate majors in physics are considered for admission to the program. Satisfactory scores on the Graduate Record Examination (general) are required. Minimum Degree Requirements 75 credits, including: 6 Core Graduate Courses PHYS 301 Mathematical Physics 3 PHYS 311 Advanced Dynamics 3 PHYS 313 Electromagnetic Theory 3 PHYS 323 Contemporary Physics 3 PHYS 362 Quantum Mechanics II 3 PHYS 365 Statistical Mechanics 3 All of these courses must be completed with a grade B or better within the first 2 years of graduate study. To accommodate the needs of the specific subfields in physics such as astrophysics, biological physics, condensed- matter physics and materials physics, 3 elective courses (9 credits) have to be chosen to fulfill the breadth requirement with a grade of B or higher. Elective courses must be completed within the first 3 years of the program, as the fourth year (and beyond if needed) should be dedicated to progress towards the Ph.D.
    [Show full text]
  • Department of Physics and Geosciences 1
    Department of Physics and Geosciences 1 Department of Physics and Geosciences Contact Information Chair: Brent Hedquist Phone: 361-593-2618 Email: [email protected] Building Name: Hill Hall Room Number: 113 The Department of Physics and Geosciences serves the needs of three types of students: 1. those majoring in geology or physics and those minoring in geography, geology, GIS, geophysics, or physics 2. technical or pre-professional students; and 3. students who take physics and geoscience courses out of interest or to satisfy science requirements. The department seeks to prepare students who are majoring in geology or physics; minoring in geography, geology, Geographic Information Systems (GIS), geophysics, or physics to compete with graduates from other institutions for industrial and governmental positions, follow a career in science education, or pursue a higher level degree. It does this through fundamental courses in the respective disciplines and through specialized programs in GIS, energy, hydrogeology, groundwater modeling, certification in GIS, certification in Geophysics, and certification in nuclear power plant (NPP) operations. For students in technical areas, the department endeavors to provide the background necessary for success in their chosen profession. For non-technical majors, the department strives to enlighten students concerning some of the basic realities of our universe and to instill in them an appreciation of the methods of scientific inquiry and the impact of science on our modern world. In addition to our undergraduate degrees and minors, we also offer an interdisciplinary graduate program in Petrophysics. Students majoring or minoring in the Department of Physics and Geosciences should plan the course work so that it will best support their career and educational goals.
    [Show full text]
  • Case Western Reserve University
    CASE WESTERN RESERVE UNIVERSITY DEPARTMENT OF PHYSICS Cleveland, Ohio 44106-7079 http://physics.cwru.edu General University Information TOEFL requirements President: Barbara Snyder The TOEFL exam is required for students from non-English- Dean of Graduate School: Charles E. Rozek speaking countries. University website: http://www.cwru.edu PBT score: 557 Control: Private iBT score:90 Setting: Urban Other admissions information Total Faculty: 2,745 Additional requirements: No minimum acceptable GRE score is Total number of Students: 9,837 specified. Total number of Graduate Students: 5,610 Undergraduate preparation assumed: Taylor, Classical Mechan- ics; Griffiths, Electrodynamics; Kittel, Thermal Physics; Grif- Department Information fiths, Quantum Mechanics; or equivalent textbooks; one or Department Chairman: Kathleen Kash, Chair two years of advanced laboratory courses. Department Contact: Corbin E. Covault, Director of the Graduate Program Total full-time faculty:25 TUITION Total number of full-time equivalent positions:22 Tuition year 2012–13: Full-Time Graduate Students:60 Tuition for out-of-state residents First-Year Graduate Students:12 Full-time students: $27,828 annual Female First-Year Students:3 Part-time students: $1,546 per credit Total Post Doctorates:15 Credit hours per semester to be considered full-time:9 Deferred tuition plan: Yes Department Address Health insurance: Available at the cost of $1,452 per year. Rockefeller Building Academic term: Semester 2076 Adelbert Road Number of first-year students who receive full tuition
    [Show full text]
  • Module Code SP-1203 Module Title Thermal Physics and Optics Degree
    Module code SP-1203 Module Title Thermal Physics and Optics Degree/Diploma Bachelor of Science (Applied Physics) Type of Module Major Core Modular Credits 4 Total student workload 10 hours/week Contact hours 4 hours/week Prerequisite A-level Physics or equivalent Anti-requisite SP-1303 Thermal Physics and Optics Aims This module aims to provide students with a logical presentation of the basic concepts and principles of thermal physics and optics in physics and strengthen the understanding of the concepts and principles through a range of real-life applications. Learning Outcomes: On successful completion of this module, a student will be expected to be able to: Lower order : 30% - recognise the three phases of matter: solid, liquid and gas, how their properties depends on thermal motion and the forces between atoms and molecules - describe the fundamental concepts related to various forms of energy: internal, enthalpy, entropy, free internal energy and free enthalpy - describe the basic concept of thermal equilibrium - describe the basic phenomena due to light matter interaction. Middle order : 60% - describe polarization and the properties of polarizing components - describe the concept of quantum nature of light and discuss the limitations of classical optics, derive the thermodynamic temperature scale from the operation of an ideal Carnot heat engine -recognise the fundamental limits for the efficiency of heat engine Higher order: 10% - describe interferometer principles and its applications. - describe and apply the basic principles of geometrical optics. - describe the kinetic theory of gases and how this theory can be applied to what is actually observed in real gases - explain and use laws of thermodynamics to solve simple problems related with heat and work changes to practical systems.
    [Show full text]
  • Equations of State of Solids for Geophysics and Ceramic Science
    EQUATIONS OF STATE OF SOLIDS FOR GEOPHYSICS AND CERAMIC SCIENCE ORSON L. ANDERSON Institute of Geophysics and Planetary Physics University of California at Los Angeles New York Oxford OXFORD UNIVERSITY PRESS 1995 CONTENTS PART I. THERMAL PHYSICS, 1 1. THE FREE ENERGY AND THE GRUNEISEN PARAMETER, 3 1.1. Introduction, 3 1.2. The Helmholtz free energy, 3 1.3. Pressure: the equation of state, 5 1.4. The Griineisen parameters, 6 1.5. The bulk modulus K, 18 1.6. The Debye temperature 9: a lower bound for high T, 24 1.7. The Debye temperature of the earth and the moon, 26 1.8. jjj: the Debye approximation to 7, 28 1.9. Electronic heat capacity contribution to 7 for iron, 29 1.10. Problems, 30 2. STATISTICAL MECHANICS AND THE QUASI- HARMONIC THEORY, 31 2.1. Introduction, 31 2.2. The vibrational energy and the thermal energy, 32 2.3. The quasiharmonic approximation, 34 2.4. The Mie-Griineisen equation of state, 35 2.5. The high-temperature limit of the quasiharmonic approxi- mation, 36 2.6. Anharmonic corrections to the Helmholtz energy, 45 2.7. The free energy and its physical properties at very low temperature, 49 2.8. The Debye theory interpolation , 52 2.9. Thermodynamic functions from the partition function, 55 2.10. Problems, 56 XIV 3. THERMOELASTIC PARAMETERS AT HIGH COMPRESSION, 57 3.1. Thermodynamic identities, 57 3.2. The mean atomic mass, fi = M/p, 61 3.3. The cases for (dKT/dT)v = 0 and (d (aKT) /dT)p = 0, 62 3.4.
    [Show full text]
  • Thermal Physics
    PHYS 1001: Thermal Physics Stream 1: Streams 2: Dr Helen Johnston Dr Pulin Gong Rm 213 Physics Rm 434 Madsen [email protected] [email protected] Module Outline • Lectures • Lab + tutorials + assignments • “University Physics”, Young & Freedman • Ch. 17: Temperature and heat • Ch. 18: Thermal properties of matter • Ch. 19: The first law of thermodynamics • Ch. 20: The second law of thermodynamics Module Outline 1. Temperature and heat 2. Thermal expansion 3. Heat capacity and latent heat 4. Methods of heat transfer 5. Ideal gases and the kinetic theory model 6, 7. The first law of thermodynamics 8, 9. 2nd Law of Thermodynamics and entropy 10. Heat engines, and Review What is temperature? • “Hotness” and “coldness” • How do we measure it? Thermodynamic systems State variables (macroscopic): T, p, V, M, ρ etc. A thermodynamic system is a quantity of matter of fixed identity, with surroundings and a boundary. Thermodynamic systems Systems can be • open – mass and energy can flow through boundary • closed – only energy can flow through boundary • isolated – nothing gets through boundary Thermal equilibrium • If two objects are in thermal contact, the hotter object cools and the cooler object warms until no further changes take place è the objects are in thermal equilibrium. What is temperature? Temperature is the value of the property that is same for two objects, after they’ve been in contact long enough and are in thermal equilibrium. Zeroth law of thermodynamics If A and B are each in thermal equilibrium with C, then A and B are in thermal equilibrium with each other.
    [Show full text]
  • Thermodynamics & Statistical Mechanics
    Thermodynamics & Statistical Mechanics: An intermediate level course Richard Fitzpatrick Associate Professor of Physics The University of Texas at Austin 1 INTRODUCTION 1 Introduction 1.1 Intended audience These lecture notes outline a single semester course intended for upper division undergraduates. 1.2 Major sources The textbooks which I have consulted most frequently whilst developing course material are: Fundamentals of statistical and thermal physics: F.Reif (McGraw-Hill, New York NY, 1965). Introduction to quantum theory: D. Park, 3rd Edition (McGraw-Hill, New York NY, 1992). 1.3 Why study thermodynamics? Thermodynamics is essentially the study of the internal motions of many body systems. Virtually all substances which we encounter in everyday life are many body systems of some sort or other (e.g., solids, liquids, gases, and light). Not surprisingly, therefore, thermodynamics is a discipline with an exceptionally wide range of applicability. Thermodynamics is certainly the most ubiquitous subfield of Physics outside Physics Departments. Engineers, Chemists, and Material Scien- tists do not study relatively or particle physics, but thermodynamics is an integral, and very important, part of their degree courses. Many people are drawn to Physics because they want to understand why the world around us is like it is. For instance, why the sky is blue, why raindrops are spherical, why we do not fall through the floor, etc. It turns out that statistical 2 1.4 The atomic theory of matter 1 INTRODUCTION thermodynamics can explain more things about the world around us than all of the other physical theories studied in the undergraduate Physics curriculum put together.
    [Show full text]
  • Thermodynamics and Statistical Mechanics
    Thermodynamics and Statistical Mechanics Richard Fitzpatrick Professor of Physics The University of Texas at Austin Contents 1 Introduction 7 1.1 IntendedAudience.................................. 7 1.2 MajorSources.................................... 7 1.3 Why Study Thermodynamics? ........................... 7 1.4 AtomicTheoryofMatter.............................. 7 1.5 What is Thermodynamics? . ........................... 8 1.6 NeedforStatisticalApproach............................ 8 1.7 MicroscopicandMacroscopicSystems....................... 10 1.8 Classical and Statistical Thermodynamics . .................... 10 1.9 ClassicalandQuantumApproaches......................... 11 2 Probability Theory 13 2.1 Introduction . .................................. 13 2.2 What is Probability? . ........................... 13 2.3 Combining Probabilities . ........................... 13 2.4 Two-StateSystem.................................. 15 2.5 CombinatorialAnalysis............................... 16 2.6 Binomial Probability Distribution . .................... 17 2.7 Mean,Variance,andStandardDeviation...................... 18 2.8 Application to Binomial Probability Distribution . ................ 19 2.9 Gaussian Probability Distribution . .................... 22 2.10 CentralLimitTheorem............................... 25 Exercises ....................................... 26 3 Statistical Mechanics 29 3.1 Introduction . .................................. 29 3.2 SpecificationofStateofMany-ParticleSystem................... 29 2 CONTENTS 3.3 Principle
    [Show full text]
  • Orson Anderson Eos of Solids
    OXFORD MONOGRAPHS ON GEOLOGY AND GEOPHYSICS Series Editors H. Charnock J. F. Dewey S. Conway Morris A. Navrotsky E. R. Oxburgh R. A. Price B. J. Skinner OXFORD MONOGRAPHS ON GEOLOGY AND GEOPHYSICS 1. DeVerle P. Harris: Mineral resources appraisal: mineral endowment, resources, and potential supply: concepts, methods, and cases 2. J. J. Veevers (ed.): Phanerozoic earth history of Australia 3. Yang Zunyi, Cheng Yuqi, and Wang Hongzhen (eds.): The geology of China 4. Lin-gun Liu and William A Bassett: Elements, oxides, and silicates: high- pressure phases with implications for the Earth's interior 5. Antoni Hoffman and Matthew H. Nitccki (eds.): Problematic fossil taxa 6. S. Mahmood Naqvi and John J. W. Rogers: Precambrian geology of India 7. Chih-Pei Chang and T. N. Krishnamurti (eds.): Monsoon meteorology 8. Zvi Ben-Avraham (ed.): The evolution of the Pacific Ocean margins 9. Ian McDougall and T. Mark Harrison: Geochronology and thermochronology by the 40Ar/39Ar method 10. Walter C. Sweet: The conodonta: morphology, taxonomy, paleoecology, and evolutionary history of a long-extinct animal phylum 11. H. J. Melosh: Impact cratering: a geologic process 12. J. W. Cowie and M. D. Brasier (eds.): The Precambrian-Cambrian boundary 13. C. S. Hutchinson: Geological evolution of south-east Asia 14. Anthony J. Naldrctt: Magmatic sulfide deposits 15. D. R. Prothero and R.M. Schoch (eds.): The evolution of perissodactyls 16. M. Menzies (ed.): Continental mantle 17. R. J. Tingey (ed.): Geology of the Antarctic 18. Thomas J. Crowley and Gerald R. North: Paleoclimatology 19. Gregory J. Retallack: Miocene paleosols and ape habitats in Pakistan and Kenya 20.
    [Show full text]