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Lecture 2 – The First Law (Ch. 1) Wednesday January 9 th Statistical mechanics What will we cover (cont...) Chapter 1 Equilibrium The zeroth law Temperature and equilibrium Temperature scales and thermometers Reading: All of chapter 1 (pages 1 - 23) 1st homework set due next Friday (18th). Homework assignment available on web page. Assigned problems: 2, 6, 8, 10, 12
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Statistical Mechanics What will we cover?
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Probability and Statistics PHY 3513 (Fall 2006)
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Probability and Statistics Probability distribution function Input parameters:Quality of teacher and level of difficulty Abilities and study habits of the students Gaussian statistics:
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Input parameters:Quality of teacher and level of difficulty Abilities and study habits of the students Probability and Statistics Probability distribution function Gaussian statistics:
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The connection to thermodynamics Maxwell-Boltzmann speed distribution function Equation of state: Input parameters: Temperature and mass (T/m)
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Probability and Entropy Suppose you toss 4 coins. There are 16 (2 4 ) possible outcomes. Each one is equally probably, i.e. probability of each result is 1/16. Let W be the number of configurations, i.e. 16 in this case, then: Boltzmann’s hypothesis concerning entropy: where k B = 1.38 × 10 23 J/K is Boltzmann’s constant.
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The bridge to thermodynamics through Z j s represent different configurations
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Quantum statistics and identical particles Indistinguishable events Heisenberg uncertainty principle The indistinguishability of identical particles has a profound effect on statistics. Furthermore, there are two fundamentally different types of particle in nature: bosons and fermions. The statistical rules for each type of particle differ!
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The connection to thermodynamics Maxwell-Boltzmann speed distribution function Input parameters: Temperature and mass (T/m) Consider T 0
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Energy # of bosons 11 10 9 8 7 6 5 4 3 2 1 0 Bose particles (bosons) Internal energy = 0 Entropy = 0
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Energy # of fermions 1 0 Fermi-Dirac particles (fermions) Pauli exclusion principle EFEF Internal energy ≠ 0 Free energy = 0 Entropy = 0 Particles are indistinguishable
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Applications Insulating solidDiatomic molecular gas Specific heats: Fermi and Bose gases
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The zeroth & first Laws Chapter 1
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Thermal equilibrium System 1 System 2 Heat P i, V i P e, V e If P i = P e and V i = V e, then system 1 and systems 2 are already in thermal equilibrium.
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Different aspects of equilibrium 1 kg Mechanical equilibrium: P e, V e Piston gas Already in thermal equilibrium When P e and V e no longer change (static) mechanical equilibrium
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P, n l, V l P, n v, V v Different aspects of equilibrium Chemical equilibrium: Already in thermal and mechanical equilibrium liquid vapor n l ↔ n v n l + n v = const. When n l, n v, V l & V v no longer change (static) chemical equilibrium
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A, B & AB Different aspects of equilibrium Chemical reaction: A + B ↔ AB # molecules ≠ const. Already in thermal and mechanical equilibrium When n A, n B & n AB no longer change (static) chemical equilibrium
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Different aspects of equilibrium If all three conditions are met: Thermal Mechanical Chemical Then we talk about a system being thermodynamic equilibrium. Question: How do we characterize the equilibrium state of a system? In particular, thermal equilibrium.....
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The Zeroth Law ACCB a)b) V A, P A V C, P C V B, P B “If two systems are separately in thermal equilibrium with a third system, they are in equilibrium with each other.” AB c) V A, P A V B, P B
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The Zeroth Law ACCB a)b) V A, P A V C, P C V B, P B “If two systems are separately in thermal equilibrium with a third system, they are in equilibrium with each other.” This leads to an equation of state, f(P,V ), where the parameter, (temperature), characterizes the equilibrium. Even more useful is the fact that this same value of also characterizes any other system which is in thermal equilibrium with the first system, regardless of its state.
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More on thermal equilibrium characterizes (is a measure of) the equilibrium. Continuum of different mechanical equilibria (P,V) for each thermal equilibrium, . Experimental fact: for an ideal, non-interacting gas, PV = constant (Boyle’s law). Why not have PV proportional to ; Kelvin scale. Each equilibrium is unique. Erases all information on history.
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Equations of state An equation of state is a mathematical relation between state variables, e.g. P, V & . This reduces the number of independent variables to two. General form: f (P,V, ) = 0 or = f (P,V) Example:PV = nR (ideal gas law) Defines a 2D surface in P-V- state space. Each point on this surface represents a unique equilibrium state of the system. f (P,V, ) = 0 Equilibrium state
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Temperature Scales
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P = a[T( o C) + 273.15] Gas Pressure Thermometer Celsius scale Steam point Ice point LN 2
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PT 17.779 13.80 3.63-195.97 An experiment that I did in PHY3513
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T(K) = T( o C) + 273.15 The ‘absolute’ kelvin scale Triple point of water: 273.16 K
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Other Types of Thermometer Thermocouple: E = aT + bT 2 Metal resistor: R = aT + b Semiconductor: logR = a blogT How stuff works How stuff works Low Temperature Thermometry Low Temperature Thermometry
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