Statistical Mechanics Homework 7

Similar documents
PHYS 352 Homework 2 Solutions

Homework 9 Solution Physics Spring a) We can calculate the chemical potential using eq(6.48): µ = τ (log(n/n Q ) log Z int ) (1) Z int =

First law of thermodynamics (Jan 12, 2016) page 1/7. Here are some comments on the material in Thompkins Chapter 1

Phase transition. Asaf Pe er Background

Simplifications to Conservation Equations

Chapter 1. Introduction

LECTURE 3 BASIC QUANTUM THEORY

Physics 607 Exam 2. ( ) = 1, Γ( z +1) = zγ( z) x n e x2 dx = 1. e x2

University of Illinois at Chicago Department of Physics SOLUTIONS. Thermodynamics and Statistical Mechanics Qualifying Examination

Gases and the Virial Expansion

Mathematics as the Language of Physics.

The Second Law: The Machinery

Physics 576 Stellar Astrophysics Prof. James Buckley. Lecture 14 Relativistic Quantum Mechanics and Quantum Statistics

(# = %(& )(* +,(- Closed system, well-defined energy (or e.g. E± E/2): Microcanonical ensemble

df da df = force on one side of da due to pressure

Part II Statistical Physics

i=1 n i, the canonical probabilities of the micro-states [ βǫ i=1 e βǫn 1 n 1 =0 +Nk B T Nǫ 1 + e ǫ/(k BT), (IV.75) E = F + TS =

Chapter 4 Phase Transitions. 4.1 Phenomenology Basic ideas. Partition function?!?! Thermodynamic limit Statistical Mechanics 1 Week 4

ZEEMAN EFFECT: p...(1). Eigenfunction for this Hamiltonian is specified by

5.4 Phase Equilibrium in Microscale Interfacial System Ultra-Thin Liquid Films, Disjoining Pressure

Adsorption of Atoms and Molecules. Physisorption Chemisorption Surface Bonding Kinetics of Adsorption/Diffusion/Desorption (Scattering Dynamics)

Chapter 2 Experimental sources of intermolecular potentials

Physics 4230 Final Examination 10 May 2007

MET 4302 Midterm Study Guide 19FEB18

Central Force Motion Challenge Problems

Theoretical Statistical Physics

Accelerator School Transverse Beam Dynamics-2. V. S. Pandit

Physics 607 Final Exam

Exam TFY4230 Statistical Physics kl Wednesday 01. June 2016

Chemical Kinetics and Equilibrium - An Overview - Key

Low field mobility in Si and GaAs

Homework Hint. Last Time

Waves and Particles. Photons. Summary. Photons. Photoeffect (cont d) Photoelectric Effect. Photon momentum: V stop

Maximum Entropy and the Stress Distribution in Soft Disk Packings Above Jamming

dn i where we have used the Gibbs equation for the Gibbs energy and the definition of chemical potential

Chapter 6. Thermodynamics and the Equations of Motion

pp physics, RWTH, WS 2003/04, T.Hebbeker

Theory of turbomachinery. Chapter 1

Thermal and Statistical Physics Department Exam Last updated November 4, L π

Find the equation of a plane perpendicular to the line x = 2t + 1, y = 3t + 4, z = t 1 and passing through the point (2, 1, 3).

The Role of Water Vapor. atmosphere (we will ignore the solid phase here) Refer to the phase diagram in the web notes.

CHAPTER 25. Answer to Checkpoint Questions

All-fiber Optical Parametric Oscillator

Lecture contents. Metals: Drude model Conductivity frequency dependence Plasma waves Difficulties of classical free electron model

Computer arithmetic. Intensive Computation. Annalisa Massini 2017/2018

Chapter 2: Equation of State

Physics 505 Homework No.2 Solution

Quark spin polarization and spontaneous magnetization in high density quark matter

Chapter 8: Coulomb blockade and Kondo physics

3. Show that if there are 23 people in a room, the probability is less than one half that no two of them share the same birthday.

Physics 607 Final Exam

Participation Factors. However, it does not give the influence of each state on the mode.

CET PHYSICS 2011 VERSION CODE: A 4

Lecture 10. Central potential

Slides Prepared by JOHN S. LOUCKS St. Edward s s University Thomson/South-Western. Slide

Chapter 18 Thermal Properties of Matter

Physics Dec The Maxwell Velocity Distribution

FUGACITY. It is simply a measure of molar Gibbs energy of a real gas.

Table of Contents [ttc]

Uniform Law on the Unit Sphere of a Banach Space

Phase Equilibria and Molecular Solutions Jan G. Korvink and Evgenii Rudnyi IMTEK Albert Ludwig University Freiburg, Germany

d 3 r d 3 vf( r, v) = N (2) = CV C = n where n N/V is the total number of molecules per unit volume. Hence e βmv2 /2 d 3 rd 3 v (5)

Last Time. A new conjugate pair: chemical potential and particle number. Today

NONRELATIVISTIC STRONG-FIELD APPROXIMATION (SFA)

summary of statistical physics

Indiana University Physics P331: Theory of Electromagnetism Review Problems #3

Phase Equilibrium Calculations by Equation of State v2

(a) Write down the total Hamiltonian of this system, including the spin degree of freedom of the electron, but neglecting spin-orbit interactions.

Curves I: Curvature and Torsion. Table of contents

1. Thermodynamics 1.1. A macroscopic view of matter

Quantization of the Photon Field QED

Distribution is a competition between these two effects: decreasing exponential, growing c 2 term. [This is actually an energy versus entropy effect!

Statistical Thermodynamics Solution Exercise 8 HS Solution Exercise 8

Landau Theory of the Fermi Liquid

9.1 System in contact with a heat reservoir

University of North Carolina-Charlotte Department of Electrical and Computer Engineering ECGR 4143/5195 Electrical Machinery Fall 2009

Caltech Ph106 Fall 2001

Waveguide Coupler I. Class: Integrated Photonic Devices Time: Fri. 8:00am ~ 11:00am. Classroom: 資電 206 Lecturer: Prof. 李明昌 (Ming-Chang Lee)

Day 3. Fluid Statics. - pressure - forces

ε tran ε tran = nrt = 2 3 N ε tran = 2 3 nn A ε tran nn A nr ε tran = 2 N A i.e. T = R ε tran = 2

The Equipartition Theorem

Unit-3. Question Bank

where (E) is the partition function of the uniform ensemble. Recalling that we have (E) = E (E) (E) i = ij x (E) j E = ij ln (E) E = k ij ~ S E = kt i

Quantum Game Beats Classical Odds Thermodynamics Implications

Physics 408 Final Exam

Recent flow results at RHIC

Phys 622 Problems Chapter 5

The individual electric and magnetic waves are in phase. The fields peak at the same position at the same time.

5.62 Physical Chemistry II Spring 2008

Basic statistical models

PHY331 Magnetism. Lecture 4

Meshless Methods for Scientific Computing Final Project

Problem set 6 for Quantum Field Theory course

The Big Picture. Thomas Schaefer. North Carolina State University

28 Lecture 28: Transfer matrix, Symmetry breaking

Chapter 6: Sound Wave Equation

THE FIRST LAW OF THERMODYNAMICS

Chapter III: Statistical mechanics

Design Constraint for Fine Grain Supply Voltage Control LSI

Transcription:

Georgia Institute of Technology Statistical Mechanics Homework 7 Conner Herndon March 26, 206 Problem : Consider a classical system of N interacting monoatomic molecules at temerature T with Hamiltonian H ({r i }, { i }) K ({ i }) + U ({r i }), (.) where K is the kinetic energy and U is the interaction otential energy. (a) Show that the robability distribution for observing the system at hase sace oint ({r i }, { i }) factors into a osition-deendent art and a momentum-deendent art. Recall that the robability distribution for observing the system at hase sace oint ({r i }, { i }) is defined in terms of the hase sace density ρ ({r i }, { i }) as f ({r i }, { i }) ρ ({r i }, { i }) ρ ({ri }, { i }) d 3N rd 3N. (.2) (b) From here, show that the single-article momentum distribution function is { ( } 2 φ ( x, y, z ) (2πmkT ) ex x + 2 y + 2 z), (.3) where m is the molecule mass. This is usually called the Maxwell-Boltzmann distribution. It is the correct momentum distribution function for a article of mass m in a thermally equilibrated system. The system can be in any hase (gas, liquid, or crystal), and the distribution is still valid rovided classical mechanics is accurate. One consequence is that the average seed (or momentum) of a article is the same in a liquid and a gas, rovided the temerature is the same. Of course, the frequency of collisions in a liquid is much higher than in a gas. For this reason, a molecule will travel much farther er unit time in a gas hase than in a condensed hase even though the single-molecule velocity distributions are identical in the two hases.

(c) Show that the fraction of molecules with momentum between and + d is 4π 2 } φ () d { (2πmkT ) ex 2 d. (.4) (d) Prove that the most robable molecular seed is v 2kT/m. (.5) (e) Prove that the mean seed is Note that v v. v 8kT πm. (.6) (f) Show that the mean square fluctuation of the seed is v 2 v 2 kt ( 3 8 ). (.7) m π Note that ( v) 2 α v 2, with α 0.8. Hence, the mean square fluctuation of the seed is comarable to the mean square seed. (g) Show that the artition function for the N-article system factors in such a way that Q (N, V, T ) Q ideal Q con, where Q ideal is the ideal gas artition function and Q con V N d 3N re βu({r i}) (.8) is the so-called configurational artition function. The hase sace density is roortional to the Boltzmann weight ρ ({r i }, { i }) e βh ({r i},{ i }). (.9) Then the robability distribution for observing the system at hase sace oint ({r i }, { i }) is e βh ({r i},{ i }) f ({r i }, { i }) e βh ({r i },{ i }) d 3N rd 3N ( ) ( ) e βk({ i }) e βu{ri} d 3N rd 3N e βk({i}) e βu{r i} ( ) ( ) e βk({ i}) e βu{r i} e βk({ i }) d 3N e βu{r i } d 3N r (.0) We have then broken the robability density into momentum- and osition-deendent arts.

(b) Letting K 2 /2m, β /kt, and 2 2 x + 2 y + 2 z, The momentum-deendent art is φ ( x, y, z ) e ( 2 x +2 y +2 z). (.) e (2 x +2 y +2 z) d x d y d z The denominator integral may be slit into the roduct of three identical integrals with the value e s2 /α ds απ, (.2) giving the single-article momentum distribution function { ( } 2 φ ( x, y, z ) (2πmkT ) ex x + 2 y + 2 z). (.3) (c) To find the fraction of articles ossessing between momentum and + d, we consider a sace sanned by x, y, and z. The number of articles with momentum between and + d is equal to the number of articles contained within the ball of radius. Then the fraction of articles is equal to the single-article momentum distribution function multilied by the solid angle and radial differential element ( { ( φ () d 4π 2 2 ) }) (2πmkT ) ex d 4π 2 (2πmkT ) ex { 2 } d. (.4) (d) The most robably velocity v may be found by taking the maximum of φ (), 0 φ () 8πe 2 /( ) + ( 4π 2) ( 2 2, ) e 2 /( ) (.5) giving and therefore v 2kT m m. (.6) (e) On the other hand, the mean seed is

v m ( ) φ () d m φ () d ( ) 3 e 2 / d m 2 e 2 / d (.7) 8 m π mkt 8kT πm. (f) To get the mean square fluctuation, we also need to mean squared momentum v 2 m 2 2 ( ) 4 e 2 / d m 2 2 e 2 / d m 2 (3mkT ) 3kT m. (.8) Then the mean square fluctuation of seed is v 2 v 2 3kT m 8kT πm kt ( 3 8 ). m π (.9) (g) The artition function is Q (N, V, T ) N!h 3N N!h 3N N e βh d 3 r i d 3 i i e βu({ri}) d 3N r e i 2 i (2πkT )3N/2 e βu({ri}) d 3N r N!h3N Q ideal e βu({ri}) d 3N r V N Q ideal Q con. N d 3 i i (.20)

Problem 2: Consider a system of N non-interacting dioles,, in an external magnetic field B Bẑ. (a) Obtain the artition function using classical statistical mechanics. Note that in this case, all - orientations are allowed. (b) Obtain al z. Comare the result with that obtained using the quantum mechanical treatment and discuss what you learn from the comarison. The energy of a diole is E B B cos θ. (2.) Then the single-diole artition function is Q (V, T ) 2π π 0 0 e βb cos θ sin θdθdφ 4π sinh (βb). βb (2.2) Since the dioles are noninteracting, the N diole artition function is the single-diole artition function raised to the ower N Q (N, V, T ) N! The average z-comonent of magnetic moment may be found by ( ) 4π N sinh N (βb). (2.3) βb z N z. (2.4) By the Gibbs equation de T ds + z db, (2.5) and by Legendre transform the Helmholtz is da SdT z db, (2.6) meaning z ( ) A. (2.7) B T By the micro-macro connection A kt log Q, so

( [ 4π z kt B log βb kt B sinh (βb) B kt B sinh (βb) ]) sinh (βb) [ sinh (βb) B [ β sinh (βb) + cos (βb) B2 B ] T ] (2.8) Then the al mean magnetic moment is coth (βb) kt B. In the quantum mechanical treatment, we had {( z QM Ng BJ + ) coth 2J NkT z N coth (βb) B. (2.9) [( + 2J ) ] βg B JB [ ]} 2J coth 2 βg BB. (2.0) If we hold constant while letting J (meaning g 0), then the two functions are the same this fact reflects the classical limit of quantum mechanics when the sin degrees of freedom reach a continuum. In the limit where the field is much greater than the temerature, z classical N z QM Ng BJ. (2.) On the other hand, in the limit when the temerature is much greater than the external field, z classical N2 B 3kT z QM Ng2 2 B J (J + ) B 3kT N2 B 3kT. (2.2) This high temerature limit reflects Curie s law, and the quantum mechanical treatment secifies the form of Curie s constant when taking the artial ( ) z χ T lim C B 0 B T. (2.3) T