Chapter-2 Maxwell-Boltzmann Statistics.

Slides:



Advertisements
Similar presentations
Classical and Quantum Gases
Advertisements

Statistical Mechanics
Statistical Mechanics
Statistical Thermodynamics
We’ve spent quite a bit of time learning about how the individual fundamental particles that compose the universe behave. Can we start with that “microscopic”
13.4 Fermi-Dirac Distribution
CHAPTER 14 THE CLASSICAL STATISTICAL TREATMENT OF AN IDEAL GAS.
The Maxwell-Boltzmann Distribution Valentim M. B. Nunes ESTT - IPT April 2015.
Chapter 3 Classical Statistics of Maxwell-Boltzmann
1.The Statistical Basis of Thermodynamics 1.The Macroscopic & the Microscopic States 2.Contact between Statistics & Thermodynamics: Physical Significance.
SOME BASIC IDEAS OF STATISTICAL PHYSICS Mr. Anil Kumar Associate Professor Physics Department Govt. College for Girls, Sector -11, Chandigarh.
Statistical Physics 2.
Chapter 2 Statistical Thermodynamics. 1- Introduction - The object of statistical thermodynamics is to present a particle theory leading to an interpretation.
Introduction to Thermostatics and Statistical Mechanics A typical physical system has N A = X particles. Each particle has 3 positions and.
Thermo & Stat Mech - Spring 2006 Class 18 1 Thermodynamics and Statistical Mechanics Statistical Distributions.
The Statistical Interpretation of Entropy The aim of this lecture is to show that entropy can be interpreted in terms of the degree of randomness as originally.
Thermo & Stat Mech - Spring 2006 Class 17 1 Thermodynamics and Statistical Mechanics Entropy.
Statistical Mechanics Physics 313 Professor Lee Carkner Lecture 23.
Maxwell - boltzmann statistics
12.3 Assembly of distinguishable particles
ELEMENTS OF STATISTICAL THERMODYNAMICS AND QUANTUM THEORY
MSEG 803 Equilibria in Material Systems 6: Phase space and microstates Prof. Juejun (JJ) Hu
Statistical Thermodynamics Chapter Introduction The object: to present a particle theory which can interpret the equilibrium thermal properties.
Principles of Equal a Priori Probability  All distributions of energy are equally probable  If E = 5 and N = 5 then                 
Statistical mechanics How the overall behavior of a system of many particles is related to the Properties of the particles themselves. It deals with the.
STATISTICAL MECHANICS. MICROSCOPIC AND MACROSCOPIC SYSTEM.
The Kinetic Theory of Gases
Chapter 19 Statistical thermodynamics: the concepts Statistical Thermodynamics Kinetics Dynamics T, P, S, H, U, G, A... { r i},{ p i},{ M i},{ E i} … How.
Entropy Change (at Constant Volume) For an ideal gas, C V (and C P ) are constant with T. But in the general case, C V (and C P ) are functions of T. Then.
Chapter 7 Bose and Fermi statistics. §7-1 The statistical expressions of thermodynamic quantities 1 、 Bose systems: Define a macrocanonical partition.
An Introduction to Statistical Thermodynamics. ( ) Gas molecules typically collide with a wall or other molecules about once every ns. Each molecule has.
Statistical Physics. Statistical Distribution Understanding the distribution of certain energy among particle members and their most probable behavior.
Byeong-Joo Lee Byeong-Joo Lee POSTECH - MSE Statistical Thermodynamic s.
Basic ideas of statistical physics
The Quantum Mechanical Picture of the Atom
Department of Electronics
Chapter 6 Applications of
Chapter 13 Classical & Quantum Statistics
The average occupation numbers
The units of g(): (energy)-1
Ideal Bose and Fermi gas
Maxwell-Boltzmann velocity distribution
6. The Theory of Simple Gases
Electrons in a Crystal Chapter 6: 3
Equilibrium Carrier Statistics
The tricky history of Black Body radiation.
Lecture 41 Statistical Mechanics and Boltzmann factor
Maxwell-Boltzmann velocity distribution
Lecture 22. Ideal Bose and Fermi gas (Ch. 7)
Density of States (DOS)
The Kinetic Theory of Gases
ENTROPY SEM 3RD.
Classical and Quantum Gases
Classical Statistics What is the speed distribution of the molecules of an ideal gas at temperature T? Maxwell speed distribution This is the probabilitity.
The Kinetic Theory of Gases
Chapter 1: Statistical Basis of Thermodynamics
Lecture 23. Systems with a Variable Number of Particles
Quantum mechanics II Winter 2012
Lecture 1 Introduction to statistical mechanics.
Total Energy is Conserved.
Fermi statistics and Bose Statistics
The Basic (Fundamental) Postulate of Statistical Mechanics
Section 2.2: Statistical Ensemble
Statistical Thermodynamics
The First 100 Years of Quantum Physics
Phase space.
Statistical Mechanics and Canonical Ensemble
Density of States (DOS)
STATISTICAL MECHANICS
Density of States (DOS)
Presentation transcript:

Chapter-2 Maxwell-Boltzmann Statistics

Phase Space A combination of position and momentum space is known as phase space. We need 6n co-ordinates to describe the behavior of dimensional space. So, if a system consists of n particles then the system in the phase space. The concept of phase space is very useful since it describe the behavior of a dynamic system.

The volume available in phase space can be divide into a large no The volume available in phase space can be divide into a large no. of compartments, each compartment is further divided into a large no. of elementary cells of equal volumes. Volume of elementary cell in phase space is given by Let

According to uncertainty principle Total no. of elementary cells in phase space

Three kinds of statistics Quantum Statistics Classical Statistics Maxwell-Boltzmann Statistics Bose-Einstein Statistics Fermi-Dirac Statistics

CLASSICAL OR M-B STATISTICS BOSE-EINSTEIN STATISTICS PARAMETER CLASSICAL OR M-B STATISTICS BOSE-EINSTEIN STATISTICS FERMI-DIRAC STATISTICS Particles Particles are distinguishable Particles are indistinguishable Size of phase space cell The size of phase space cell can be as small as we require The size of the phase space cell cannot be less than h3 The size cannot be less than h3 Number of cells If ni be the number of particles and gi the number of cells then gi>>ni so ni/gi<<1. Thus,number of cells can be made as large as possible The number of cells is less than or comparable to the number of particles gi < ni ni/gi  1 The number of cells has to be greater or equal to the number of particles so ni /gi  1 Restriction on particles No restriction Restriction due to Pauli Exclusion Principle Two particle distribution in two cells The particles are distinguishable and can be arranged in four ways The particles are indistinguishable and can be arranged in three ways No two particles can occupy the same cell. Hence, only one arrangement

Basic Approach in three Statistics In any dynamic isolated system, the total number of particles (n) and the total energy (U) has to remain constant When the system is in equilibrium then it exists only in the most probable state. In the most probable state of the system W must be maximum. For all natural systems W is a very large number. We, therefore, deal with log W.

The three equations (1), (2) and (3) must be simultaneously satisfied by the system irrespective of the kind of statistics to be applied. These three conditions can be incorporated into a single eq. by the method of Lagrange’s undetermined multipliers. We multiply eq. (1) with - , eq. (2) by - and add to eq. (3)

Maxwell – Boltzmann statistics applied to an ideal gas in Equilibrium The total energy (U) is divided into 1,2,3…..k intervals (compartments) of magnitude in 1,2,3……k. Let represent the no. of molecules in these energy intervals 1,2,3….k. The thermodynamic prob. for macrostate

Taking logarithm Using stirling’s formula

Differentiating as For most probable state W= maximum therefore

Putting this in This is Maxwell Boltzmann distribution law

In Maxwell Boltzmann distribution

Momentum of particle is related with the kinetic energy as From eqn. (5)

where n(p) is number of molecules in the range Therefore total no. of molecules in the range p and (p+dp) where g(p)dp is the no. of cells in momentum interval p and p+dp

Number of cells in phase space corresponding to momentum interval p and (p+dp)

Substituting eq (x) in eq (2)

Using standard integral

Substituting these in (7)

Total energy of the system

Using standard integral Substituting this in (8)

Putting in (9)