Übungen zur Theoretischen Physik Fa WS 17/18

Similar documents
Electromagnetism Notes, NYU Spring 2018

a) Read over steps (1)- (4) below and sketch the path of the cycle on a P V plot on the graph below. Label all appropriate points.

MATH34032: Green s Functions, Integral Equations and the Calculus of Variations 1. 1 [(y ) 2 + yy + y 2 ] dx,

16z z q. q( B) Max{2 z z z z B} r z r z r z r z B. John Riley 19 October Econ 401A: Microeconomic Theory. Homework 2 Answers

Math 32B Discussion Session Week 8 Notes February 28 and March 2, f(b) f(a) = f (t)dt (1)

Physics 202, Lecture 14

Chapter Gauss Quadrature Rule of Integration

HOMEWORK SOLUTIONS MATH 1910 Sections 7.9, 8.1 Fall 2016

Solutions to Assignment 1

Chem Homework 11 due Monday, Apr. 28, 2014, 2 PM

Chemistry 431 Problem Set 9 Fall 2018 Solutions

for all x in [a,b], then the area of the region bounded by the graphs of f and g and the vertical lines x = a and x = b is b [ ( ) ( )] A= f x g x dx

Matrices SCHOOL OF ENGINEERING & BUILT ENVIRONMENT. Mathematics (c) 1. Definition of a Matrix

Particle Physics. Michaelmas Term 2011 Prof Mark Thomson. Handout 3 : Interaction by Particle Exchange and QED. Recap

Lecture 1 - Introduction and Basic Facts about PDEs

CHM Physical Chemistry I Chapter 1 - Supplementary Material

Physics 3323, Fall 2016 Problem Set 7 due Oct 14, 2016

INTEGRATION. 1 Integrals of Complex Valued functions of a REAL variable

Applications of Definite Integral

First Law of Thermodynamics. Control Mass (Closed System) Conservation of Mass. Conservation of Energy

Numbers and indices. 1.1 Fractions. GCSE C Example 1. Handy hint. Key point

ECE Microwave Engineering. Fall Prof. David R. Jackson Dept. of ECE. Notes 8. Waveguides Part 5: Coaxial Cable

Sections 5.3: Antiderivatives and the Fundamental Theorem of Calculus Theory:

] dx (3) = [15x] 2 0

Definition of Continuity: The function f(x) is continuous at x = a if f(a) exists and lim

The Double Integral. The Riemann sum of a function f (x; y) over this partition of [a; b] [c; d] is. f (r j ; t k ) x j y k

, g. Exercise 1. Generator polynomials of a convolutional code, given in binary form, are g. Solution 1.

(a) A partition P of [a, b] is a finite subset of [a, b] containing a and b. If Q is another partition and P Q, then Q is a refinement of P.

ON THE INEQUALITY OF THE DIFFERENCE OF TWO INTEGRAL MEANS AND APPLICATIONS FOR PDFs

Overview of Calculus I

y z A left-handed system can be rotated to look like the following. z

1.3 SCALARS AND VECTORS

April 8, 2017 Math 9. Geometry. Solving vector problems. Problem. Prove that if vectors and satisfy, then.

Part I: Basic Concepts of Thermodynamics

Magnetically Coupled Coil

Space Curves. Recall the parametric equations of a curve in xy-plane and compare them with parametric equations of a curve in space.

AQA Further Pure 2. Hyperbolic Functions. Section 2: The inverse hyperbolic functions

Strategy: Use the Gibbs phase rule (Equation 5.3). How many components are present?

T b a(f) [f ] +. P b a(f) = Conclude that if f is in AC then it is the difference of two monotone absolutely continuous functions.

Classical Mechanics. From Molecular to Con/nuum Physics I WS 11/12 Emiliano Ippoli/ October, 2011

ECE 451 Automated Microwave Measurements. TRL Calibration

Math RE - Calculus II Area Page 1 of 12

Partial Derivatives. Limits. For a single variable function f (x), the limit lim

(h+ ) = 0, (3.1) s = s 0, (3.2)

Core 2 Logarithms and exponentials. Section 1: Introduction to logarithms

Tutorial Worksheet. 1. Find all solutions to the linear system by following the given steps. x + 2y + 3z = 2 2x + 3y + z = 4.

System Validation (IN4387) November 2, 2012, 14:00-17:00

CHAPTER 20: Second Law of Thermodynamics

The Emission-Absorption of Energy analyzed by Quantum-Relativity. Abstract

arxiv: v1 [math.ca] 21 Aug 2018

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Statistical Physics I Spring Term Solutions to Problem Set #1

Math Calculus with Analytic Geometry II

- 5 - TEST 2. This test is on the final sections of this session's syllabus and. should be attempted by all students.

Problem Set 3 Solutions

Thermodynamics. Question 1. Question 2. Question 3 3/10/2010. Practice Questions PV TR PV T R

Theoretische Physik 2: Elektrodynamik (Prof. A.-S. Smith) Home assignment 4

ISOTHERMAL REACTOR DESIGN (4) Marcel Lacroix Université de Sherbrooke

Physics 505 Homework No. 11 Solutions S11-1

( ) 1. 1) Let f( x ) = 10 5x. Find and simplify f( 2) and then state the domain of f(x).

u t = k 2 u x 2 (1) a n sin nπx sin 2 L e k(nπ/l) t f(x) = sin nπx f(x) sin nπx dx (6) 2 L f(x 0 ) sin nπx 0 2 L sin nπx 0 nπx

f (z) dz = 0 f(z) dz = 2πj f(z 0 ) Generalized Cauchy Integral Formula (For pole with any order) (n 1)! f (n 1) (z 0 ) f (n) (z 0 ) M n!

Summary: Method of Separation of Variables

MAT187H1F Lec0101 Burbulla

CHAPTER 4: DETERMINANTS

Fig. 1. Open-Loop and Closed-Loop Systems with Plant Variations

Assignment 6. 1 Kadar Ch. 5 Problem 6. Tyler Shendruk April 5, Part a)

Chapter 6 Notes, Larson/Hostetler 3e

Problems set # 3 Physics 169 February 24, 2015

Logarithms LOGARITHMS.

ERT 316: REACTION ENGINEERING CHAPTER 3 RATE LAWS & STOICHIOMETRY

18.06 Problem Set 4 Due Wednesday, Oct. 11, 2006 at 4:00 p.m. in 2-106

A5682: Introduction to Cosmology Course Notes. 4. Cosmic Dynamics: The Friedmann Equation. = GM s

Kinematic Waves. These are waves which result from the conservation equation. t + I = 0. (2)

AP Calculus BC Chapter 8: Integration Techniques, L Hopital s Rule and Improper Integrals

University of Sioux Falls. MAT204/205 Calculus I/II

W = Fdz = mgdz = mg dz = mgz. dv F = ma = m dt = =

Section 3.6. Definite Integrals

Practice Problems Solution

X Z Y Table 1: Possibles values for Y = XZ. 1, p

ILLUSTRATING THE EXTENSION OF A SPECIAL PROPERTY OF CUBIC POLYNOMIALS TO NTH DEGREE POLYNOMIALS

The Wave Equation I. MA 436 Kurt Bryan

Phys 7221, Fall 2006: Homework # 6

Unit 5. Integration techniques

Polynomial Approximations for the Natural Logarithm and Arctangent Functions. Math 230

Lecture 20: Numerical Integration III

F / x everywhere in some domain containing R. Then, + ). (10.4.1)

SOLUTIONS TO MATH38181 EXTREME VALUES EXAM

Chapter 9 Definite Integrals

Math 124A October 04, 2011

Lecture Summaries for Multivariable Integral Calculus M52B

A REVIEW OF CALCULUS CONCEPTS FOR JDEP 384H. Thomas Shores Department of Mathematics University of Nebraska Spring 2007

8 THREE PHASE A.C. CIRCUITS

Parabola and Catenary Equations for Conductor Height Calculation

Study Guide Final Exam. Part A: Kinetic Theory, First Law of Thermodynamics, Heat Engines

Higher Checklist (Unit 3) Higher Checklist (Unit 3) Vectors

Module 2: Rate Law & Stoichiomtery (Chapter 3, Fogler)

U Q W The First Law of Thermodynamics. Efficiency. Closed cycle steam power plant. First page of S. Carnot s paper. Sadi Carnot ( )

Functions. mjarrar Watch this lecture and download the slides

Physics 215 Quantum Mechanics 1 Assignment 2

HT Module 2 Paper solution. Module 2. Q6.Discuss Electrical analogy of combined heat conduction and convection in a composite wall.

Transcription:

Krlsruher Institut für ehnologie Institut für heorie der Kondensierten Mterie Übungen zur heoretishen Physik F WS 17/18 Prof Dr A Shnirmn Bltt 4 PD Dr B Nrozhny Lösungsvorshlg 1 Nihtwehselwirkende Spins: () Sttionry sttes re hrterized by the sets of quntum numbers σ } with the orresponding energies Eσ } = µ σ z = M ere M is the mgnetiztion in the diretion of the field, whih we hve hosen s the z xis σ = ±1 re the z-omponents of the individul spins We hoose units with k B = 1 (b) he sttistil sum is Z = σ } e Eσ}/ = σ } N e µσ/ = =1 N e µσ/ = =1 σ } 2 osh µ ] N he free energy is the logrithm of the sttistil sum F = ln Z = N ln 2 osh µ ] () he entropie: ( ) F S = = N ln 2 osh µ ] µn tnh µ he mgnetiztion: he speifi het: M = = ( ) S = = µn tnh µ µ 2 2 2 osh 2 µ he speifi het for onstnt mgnetiztion n be lulted inverting the funtion M(, ): ( ) S(, (M, )) M = M ( ) ( ) ( ) S(, (M, )) S(, (M, )) (M, ) = + = M

(d) In the limit of lrge fields, M(µ ) µn In the limit of smll fields, M(µ ) µ 2 N herefore the suseptibility is given by the Curie lw ( ) M χ( ) = lim = µ2 N 2 eisenberg Modell für 2 Gitterplätze: Aording to the generl rules of ddtion of ngulr momentum, the system of two moment n be desribed by set of four quntum numbers he two ommon possibilities re either (i) s 2 1, s 2 2, s z 1, s z 2, or (ii) s 2 1, s 2 2, S 2, S z, where S = s 1 + s 2 Suppose we hoose the first possibility hen for fixed s 2 1 = s 1 (s 1 +1), s 2 2 = s 2 (s 2 +1), the quntities s z i tke 2s i + 1 vlues eh, so tht the totl number of sttes being (2s 1 + 1)(2s 2 + 1) For two spins 1, s i = 1, we hve 9 possible sttes In this problem, it is more onvenient to hoose the seond representtion, sine s 1 s 2 = 1 2 S(S + 1) s 1(s 1 + 1) s 2 (s 2 + 1)] he 9 possible sttes orrespond to the following vlues (fixing s 1 = s 2 = 1): S =, S z =, s 1 s 2 = 2, S = 1, S z =, ±1, s 1 s 2 = 1, S = 2, S z =, ±1, ±2, s 1 s 2 = 1 () In the bsene of the field, the sttistil sum is given by Z = e Js 1 s 2 / = 5e J/ + 3e J/ + e 2J/ = 6 osh J/ + 2e J/ + e 2J/ S,S z } he free energy is he speifi het is C V = 2 F 2 = J 2 3 e 2J/ F = ln Z ( ) ( ) ( ) ] 2 2 4 J 1 + 3 J 1 e J/ 5 J + 1 e 3J/

(b) In the presene of the field, the sttistil sum is Z = e (Js 1 s 2 +µs z )/ = S,S z } = e J/ ( 1 + 2 osh µ ) ( 2µ + 2 osh + e J/ 1 + 2 osh µ ) + e 2J/ he free energy is he mgnetiztion is M = F = 4µ Z F = ln Z osh J sinh µ + ej/ sinh 2µ ] he suseptibility is χ( ) = 4µ2 Z osh J + 2eJ/ ], where Z is the bove sttistil sum in the bsene of the field his suseptibility beomes Curie-like only t high tempertures J 3 Msselose reltivistishe eilhen: () he sttistil sum of system of non-interting prtiles ftorizes: Z = ZN 1 N! he single-prtile sttistil sum is given by (here = = 1) Z 1 = V () 2 e p / = V pe p/ dp = V 2 2 ze z dz = V 2 2 ene, the sttistil sum is he free energy is F = ln Z = Z = V N N!() N 2N ln } V ln N! ( ) 2N = 2N ln ( ) ] } 1/2 V N ln N + N, or F = 2N ln ( ) ] 1/2 V N N

(b) he entropy is given by the derivtive S = V,N = F + 2N Similrly, the pressure is,n = N V () he eqution of stte reltes the internl energy of the system to temperture he internl energy is U = V () 2 pθ(p F p) = V p F p 2 dp = V p3 F 6π his should be relted to the prtile density N V = () θ(p 2 F p) = 1 p F pdp = p2 F 4π ene p F = 4πN/V nd the internl energy n be expressed s U = 4N 4πN 3 V he pressure n be evluted lso s ( ) U,N = U 2V Compring with the previous result, we find the eqution of stte 4 Ideles Gs: P V = N U = 2N () he sttistil sum of system of non-interting prtiles ftorizes: Z = ZN 1 N! he single-prtile sttistil sum is given by (here = = 1) Z 1 = V d 3 p / = V () 3 e p 4 2 p 2 e p4 / dp = V 3/4 2 3/4 z 2 e z4 dz = V ( ) 3/4 8π Γ(3/4) 2

ene, the sttistil sum is he free energy is Z = V N N! F = ln Z = Γ(3/4) N ln 3N = 4 ln = 3 4 N ln (b) he entropy is given by the derivtive S = Similrly, the pressure is ] N ( ) 3N/4 V Γ(3/4) ( V Γ(3/4) ( ) ] } 3/4 ln N! ) ] 4/3 ( ) ] 4/3 V Γ(3/4) N N V,N,N = F + 3 4 N = N V N ln N + N () he eqution of stte reltes the internl energy of the system to temperture he internl energy is U = V d 3 p () 3 p4 θ(p F p) = V 2 his should be relted to the prtile density ene N V = d 3 p () θ(p 3 F p) = 1 2 p F = 3 6π 2 N/V nd the internl energy n be expressed s U = 3N ( 6π 2 N 7 V he pressure n be evluted lso s ( ) U,N p F p F ) 4/3 = 4U 3V p 6 dp = V p7 F 14π 2 p 2 dp = p3 F 6π 2 Compring with the previous result, we find the eqution of stte P V = N U = 3 4 N },