Partition Functions. Chris Clark July 18, 2006

Similar documents
Single Particle State AB AB

The second law of thermodynamics - II.

763620SS STATISTICAL PHYSICS Solutions 2 Autumn 2012

Lecture 2 - Thermodynamics Overview

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx.

11) A thin, uniform rod of mass M is supported by two vertical strings, as shown below.

4/18/2005. Statistical Learning Theory

On a quantity that is analogous to potential and a theorem that relates to it

Appendix B The Relativistic Transformation of Forces

Appendix A. Appendices. A.1 ɛ ijk and cross products. Vector Operations: δ ij and ɛ ijk

Chem 453/544 Fall /08/03. Exam #1 Solutions

Classical Mechanics Homework set 7, due Nov 8th: Solutions

Physics 2A Chapter 10 - Moment of Inertia Fall 2018

Preliminary Exam: Quantum Physics 1/14/2011, 9:00-3:00

B. Spherical Wave Propagation

12.1 INTRODUCTION: STATES OF MANY-PARTICLE SYSTEMS

Related Rates - the Basics

Qualifying Examination Electricity and Magnetism Solutions January 12, 2006

ASTR415: Problem Set #6

Section 11. Timescales Radiation transport in stars

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3.

On the integration of the equations of hydrodynamics

Lecture 8 - Gauss s Law

But for simplicity, we ll define significant as the time it takes a star to lose all memory of its original trajectory, i.e.,

Nuclear and Particle Physics - Lecture 20 The shell model

Three dimensional flow analysis in Axial Flow Compressors

c n ψ n (r)e ient/ h (2) where E n = 1 mc 2 α 2 Z 2 ψ(r) = c n ψ n (r) = c n = ψn(r)ψ(r)d 3 x e 2r/a0 1 πa e 3r/a0 r 2 dr c 1 2 = 2 9 /3 6 = 0.

Problem 1. Part b. Part a. Wayne Witzke ProblemSet #1 PHY 361. Calculate x, the expected value of x, defined by

Scattering in Three Dimensions

Chapter 13 Gravitation

I. CONSTRUCTION OF THE GREEN S FUNCTION

Classical Worm algorithms (WA)

Hopefully Helpful Hints for Gauss s Law

A thermodynamic degree of freedom solution to the galaxy cluster problem of MOND. Abstract

Review: Electrostatics and Magnetostatics

A New Approach to General Relativity

Question 1: The dipole

ON INDEPENDENT SETS IN PURELY ATOMIC PROBABILITY SPACES WITH GEOMETRIC DISTRIBUTION. 1. Introduction. 1 r r. r k for every set E A, E \ {0},

d 2 x 0a d d =0. Relative to an arbitrary (accelerating frame) specified by x a = x a (x 0b ), the latter becomes: d 2 x a d 2 + a dx b dx c

-Δ u = λ u. u(x,y) = u 1. (x) u 2. (y) u(r,θ) = R(r) Θ(θ) Δu = 2 u + 2 u. r = x 2 + y 2. tan(θ) = y/x. r cos(θ) = cos(θ) r.

Auchmuty High School Mathematics Department Advanced Higher Notes Teacher Version

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925)

Pressure Calculation of a Constant Density Star in the Dynamic Theory of Gravity

Mobility of atoms and diffusion. Einstein relation.

Lecture 7: Angular Momentum, Hydrogen Atom

Black Body Radiation and Radiometric Parameters:

Revision of Lecture Eight

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum

Math 124B February 02, 2012

Lecture 23. Representation of the Dirac delta function in other coordinate systems

you of a spring. The potential energy for a spring is given by the parabola U( x)

Numerical Integration

Hawking Radiation Seminar Talk

Voltage ( = Electric Potential )

Physics 121 Hour Exam #5 Solution

The Substring Search Problem

Homework 7 Solutions

Lecture 28: Convergence of Random Variables and Related Theorems

EM-2. 1 Coulomb s law, electric field, potential field, superposition q. Electric field of a point charge (1)

The Poisson bracket and magnetic monopoles

Compactly Supported Radial Basis Functions

Practice Integration Math 120 Calculus I Fall 2015

5.61 Physical Chemistry Lecture #23 page 1 MANY ELECTRON ATOMS

Practice Integration Math 120 Calculus I D Joyce, Fall 2013

ESCAPING FROM EARNSHAW THEOREM

Physics 221 Lecture 41 Nonlinear Absorption and Refraction

Quantum Mechanics II

EN40: Dynamics and Vibrations. Midterm Examination Thursday March

What molecular weight polymer is necessary to provide steric stabilization? = [1]

1) (A B) = A B ( ) 2) A B = A. i) A A = φ i j. ii) Additional Important Properties of Sets. De Morgan s Theorems :

ATMO 551a Fall 08. Diffusion

EM Boundary Value Problems

Chapter 2: Basic Physics and Math Supplements

Class #16 Monday, March 20, 2017

Physics 506 Winter 2006 Homework Assignment #9 Solutions

When a mass moves because of a force, we can define several types of problem.

Surveillance Points in High Dimensional Spaces

1 Fundamental Solutions to the Wave Equation

9.1 The multiplicative group of a finite field. Theorem 9.1. The multiplicative group F of a finite field is cyclic.

Adiabatic evolution of the constants of motion in resonance (I)

= 4 3 π( m) 3 (5480 kg m 3 ) = kg.

European Journal of Basic and Applied Sciences Vol. 3 No. 1, 2016 ISSN

? this lecture. ? next lecture. What we have learned so far. a Q E F = q E a. F = q v B a. a Q in motion B. db/dt E. de/dt B.

AP Physics Electric Potential Energy

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1

3. Electromagnetic Waves II

PHYSICS 151 Notes for Online Lecture #36

Tutorial Exercises: Central Forces

The physics of induction stoves

PHYSICS 4E FINAL EXAM SPRING QUARTER 2010 PROF. HIRSCH JUNE 11 Formulas and constants: hc =12,400 ev A ; k B. = hf " #, # $ work function.

KEPLER S LAWS OF PLANETARY MOTION

Stellar Structure and Evolution

Solving Problems of Advance of Mercury s Perihelion and Deflection of. Photon Around the Sun with New Newton s Formula of Gravity

An Exact Solution of Navier Stokes Equation

Fifth force potentials, compared to Yukawa modification of Gravity for massive Gravitons, to link Gravitation, and NLED modified GR

Fall 2016 Semester METR 3113 Atmospheric Dynamics I: Introduction to Atmospheric Kinematics and Dynamics

Physics 505 Homework No. 9 Solutions S9-1

10/04/18. P [P(x)] 1 negl(n).

PHYS 301 HOMEWORK #10 (Optional HW)

OSCILLATIONS AND GRAVITATION

Transcription:

Patition Functions Chis Clak July 18, 2006 1 Intoduction Patition functions ae useful because it is easy to deive expectation values of paametes of the system fom them. Below is a list of the mao examples. E = ln(z p = kt ln(z S = k ln(z kβ ln(z C V = kβ 2 2 ln(z 2 F = kt ln(z α = ln(z N µ = kt ln(z N You can see that evey paamete can be expessed in tems of ln(z and this is the simplest expession fo most paametes. Be caeful when deiving the expession fo pessue, it is not the deivative of E as is often the case. p = ( E S ( E T,V,N We will deive these in a systematic way in this pape. 1

2 Boltzmann Facto and Patition Function Conside a system A in themal contact with a esevoi at tempeatue T with combined enegy E o. et subscipt efe to the esevoi, o efe to the total system and no subscipt efe to the system A. 1 P = ω (E o E ω o (E o = es(eo E/k e So(Eo/k By expanding the entopy in powes of a small enegy, the top exponent becomes S (E o E = S (E o E + E E = S (E o E + (E E S E = S (E o E + (E E /T Eo E=E And by the additivity of entopy the bottom exponent can be witten as Theefoe S o (E o = S(E + S o (E o E P = es(eo E/k+(E E/kT e S(E/k+S(Eo E/k = e(e E/kT e S(E/k = e (E T S/kT e E/kT = e βf e βe So when we apply the nomalization condition P = 1 e βf e βe = 1 we see that the quantity defined by Z e βe which we call the patition function, satisfies Z = e βf The patition function is so named accoding to Wikipedia because it encodes how the pobabilities ae patitioned among the diffeent micostates, 1 This section is fom Callen Page 350. 2

based on thei individual enegies. The lette Z stands fo Zustandssumme, which is Geman fo sum of states. It is woth noting that the sum must be taken ove all quantum states and not ove all allowed enegies since thee may be degeneacies. It is extemely impotant to undestand that the whole patition function fomalism is built on the assumption of a canonical ensemble, which means that the system is in contact with a themal esevoi. Theefoe, if you want to use the patition function at all, then you must be sue that you system is in contact with some kind of themal esevoi, unless if the system emains in themal equilibium at a constant tempeatue. In that case the esevoi would have no effect and so it is not necessay. Themal esevois come in many foms. Fo example electomagnetic adiation can act as a themal esevoi, howeve usually themal inteactions occu via paticle collisions. 3 Deived Quantities Z is always a function of the complete set T, V, N, so you cannot detemine these paametes fom Z. You do not need to wite the notation fo keeping T,V, o N constant when taking deivatives of Z because these paametes ae aleady assumed constant. Since these paametes ae a complete set, no othe paametes may be held constant o the system would be ovedetemined. That is why we could not find the pessue by taking the volume deivative of enegy we could not hold entopy constant. Of the fou types of enegy (E, F, G, H, the Helmholtz fee enegy F is the one that consides T and V as independent paametes. Note that all fou conside N a constant paamete. Theefoe only in tems of F can we ceate a fundamental elation with Z. This fundamental elation 2 is Z e βe = e βf So what is the best way to emembe all of the expessions fo quantities deived fom the patition function? Memoize this fundamental elation and how to use the Helmholtz fee enegy to deive the est. Remembe that F = E T S and stat fom the fundamental themodynamic elation. 2 This is fom Callen Pg 352 de = T ds pdv de = d(t S SdT pdv d(e T S = df = SdT pdv ( ( df = dt + dv V T ( ( S = and p = V T 3

et s stating deiving the elations. We automatically get Using the new patial deivatives, F = kt ln(z (T ln(z S = k = k ln(z + kt ln(z = k ln(z + kβ ln(z ( Now we can get µ fom µ = Then α = βµ so, p = kt ln(z N T,V,N µ = kt ln(z N α = ln(z N We can even get the enegy if we use some tickey. E = F + T S = F 1 kβ = F + β = (βf = ln(z And finally the heat capacity at constant volume comes fom C V = ( E C V = kβ 2 2 ln(z 2 4 Pobability Explanation et s look at this fom anothe angle. The patition function fomalism woks because it poduces the pobabilities of states to make an expectation value summation. 3 P = Ce βe = e βe Similaly fo E 2, e βe e βe E = P E = Z E = 1 Z = 1 ( e βe 1 Z = Z Z 3 This section taken fom Reif Pg 212 E 2 = 1 Z 2 Z 2 = e βe Z e βe E = ln(z V. 4

This can be ewitten as E 2 = ( 1 Z Z + 1 Z 2 Theefoe the fluctuation in enegy is 5 Geneal Paamete ( 2 Z = E + E2 ( E 2 = E 2 E 2 = E = 2 ln(z 2 If the micostate enegies all depend on a paamete λ by whee E (0 E = E (0 + λa does not depend on λ, then the expectation value of A is A = 1 Z = 1 1 Z β Ae β(e(0 +λa λ e β(e (0 +λa = kt ln(z λ You can also be eally ticky and use this to find the expectation values of quantities that ae not in the Hamiltonian by atificially adding them in and setting λ 0 at the end. 4 6 Momentum Integal Appoximation Since momentum is found in evey Hamiltonian that efes to a paticle, it is vey common that you have to sum ove momentum states in a patition function. The eason that the sum is not infinite is because momentum is always quantized inside any containe. In themodynamics we always have a volume V, which tells us the size of ou containe. We want to appoximate the sum ove momentum states with an integal, which will be much easie to handle. Howeve, in ode to deive the integal, we will have to assume the containe is a cubical box. As it tuns out, the esult is independent of the shape of the containe, even though the only evidence I have is an equation fom classical themodynamics. p = hk = h (πnx 2 + ( πny 2 ( πnz 2 + 4 This section came fom Wikipedia s aticle: Patition Function 5

= hπ n 2 x + n 2 y + n 2 z So the patition function fo the simple Hamiltonian H = p 2 /2m is Z = e βe = e βp2 /2m = e β h2 π 2 (n x 2 /2m2 3 [ ] 3 = e β h2 π 2 n 2 x /2m2 dn x 0 [ ( ] 3 = e βp2 x /2m d 0 hπ p x = V [ ] 3 π 3 h 3 e βp2 x /2m dp x 0 = V 1 2π 3 h 3 e β(p2 x +p2 y +p2 z /2m dp x dp y dp z In the last line the momentum takes on its classical meaning as the components of the momentum vecto, wheeas befoe it was a positive quantity based on the quantum wave function. This esult is tue fo abitay shaped containes because the classical expession fo the patition function is 5 Z = 1 h 3 e βh dx dy dz dp x dp y dp z 7 Gand Canonical Patition Function Micocanonical Ensemble - ensemble of isolated systems, can be used to deive the expession fo entopy Canonical Ensemble - ensemble of systems that can exchange themal enegy with a esevoi, can be used to deive the Boltzmann facto and the patition function fomalism Gand Canonical Ensemble - ensemble of systems that can exchange both themal enegy and paticles with a esevoi 8 Quantum Statistics I think that you ae supposed to use the same expession fo the patition function when dealing with quantum statistics. 5 This is Callen (16.68 o Reif 7.12 6