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445lec8

Course: PHYS 445, Spring 2008
School: Simon Fraser
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445 PHYS Lecture 8 - Interacting systems Lecture 8 - Interacting systems What's Important: equilibrium and reversibility systems in interaction Text: Reif 8-1 Constraints and (Reif, Sec. 3.1; not covered in class) Suppose that two systems are brought in contact, and a constraint that isolated them is removed. How do we describe theoretically what happens? For example, consider what happens when a thermal...

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445 PHYS Lecture 8 - Interacting systems Lecture 8 - Interacting systems What's Important: equilibrium and reversibility systems in interaction Text: Reif 8-1 Constraints and (Reif, Sec. 3.1; not covered in class) Suppose that two systems are brought in contact, and a constraint that isolated them is removed. How do we describe theoretically what happens? For example, consider what happens when a thermal barrier between two gases is removed, but the volume of their container is not altered. Remove the barrier Once the barrier has been removed, the number of accessible states must be the same, or larger: f i. That is, removing a constraint cannot decrease the number of accessible states. As the probability of the system being in a particular state is proportional to , then the probability of a system returning to its initial state is i / f. Reversible and irreversible processes (Reif, Sec. 3.2; not covered in class) If the number of accessible states doesn't change during a process, that is f = i, then equilibrium can be maintained during the process and it is reversible. If the number of accessible states increases during a process, f i, then the process is irreversible. For example, if a gas expands to occupy a larger volume by removing a barrier, then it will not go back to its original state if the barrier is reinserted: 2001 by David Boal, Simon Fraser University. All rights reserved; further resale or copying is strictly prohibited. PHYS 445 Lecture 8 - Interacting systems 8-2 Remove the barrier Systems in interaction (thermal contact) Note: the following argument uses discrete energies, but goes over to continuous energies without modification) Next, consider what happens when we place two systems in thermal contact, but not mechanical contact (i.e., systems can exchange energy, but not volume or material). A A' Ao Two systems A and A' combine to form Ao, which is isolated. Because Ao is isolated, the total energy of Ao is constant, even as the subsystems exchange energy. Denoting the energies of A, A' and Ao as E, E' and Eo, then E + E' = Eo = constant (Ao is isolated) Denote the number of accessible states in each system as (E), '(E') and o(Eo). What is the probability P(E) of system A having energy E? In the isolated system A before contact, it is (E ) (E) PA(E) = = (8.1) TOT What about the combined system? Call PAo(E) the probability of system A having energy E once the systems are in contact. Then 0 (E) 0 PA (E) = (8.2) 0 TOT with 0 TOT = E 0 (E ) (8.3) What about o(E)? For every state in the collection (E), a total of 1 x '(E') combined states can be formed (where E' = Eo-E). Hence, for a specific energy division E and E', there must be a total of (E) '(E') states. We sum over all of these combinations to obtain oTOT. 2001 by David Boal, Simon Fraser University. All rights reserved; further resale or copying is strictly prohibited. PHYS 445 Lecture 8 - Interacting systems 8-3 Numerical example Let systems 1 and 2 have allowed energies E = 1,2 and E' = 1,2, with accessible states according to # of states E # of states E' Combined states E' = 1 E= 1 16 2 32 2 1 8 1 2 4 8 4 2 2 2 total energy E' = E= 1 2 Eo 1 2 3 2 3 4 Combined states as a function of Eo: # of states 16 32+4 8 Eo 2 3 4 o for a total of TOT = 60 states. Fractional distribution of combined fraction states of states 0.27 0.6 0.13 Eo 2 3 4 Now, let's see the effects of constraints. If we ask, what are the number of states of the combined system o as a function of the energy E of the subsystem, we would find (add rows in the "combined states" table): o (E) 20 40 E 1 2 (no constraint on Eo) As expected, the fractional distribution of combined states is the same, as a function of E, as the uncombined subsystem. The same would be true if we calculated o as a function of E' (by adding columns). BUT, if we place a constraint on Eo, the fractional distributions of the subsystems changes. Say we demand Eo = 3. Then the number of states o as a function of E of the subsystem changes to (cross diagonal in the table) o (E) 4 32 E 1 2 (constraint Eo = 3). Hence, once the systems are put in thermal contact, and constraints are placed on the energy of the combined system, then the probability distribution in a subsystem may be changed. The value of E to which subsystem A changes once the systems are placed in thermal contact (and the total energy is constrained!) can be calculated from the distribution of total states Po, as a function of E. Let's move away from our numerical example, and consider the problem in general. 2001 by David Boal, Simon Fraser University. All rights reserved; further resale or copying is strictly prohibited. PHYS 445 Lecture 8 - Interacting systems 8-4 The number of states of A as a function of E generally increases rapidly with E: E The number of states ' of A' generally increases rapidly with E', and hence generally decreases rapidly with E = Eo-E' ' E Hence, the probability P oA for system A, once its in contact with A' and the total energy is constrained, looks like P oA E ~ E ~ The most likely energy of A is now at E , which can be found by the usual calculus procedure of setting a derivative equal to zero. In this case, we use the natural logarithm of P oA: P oA is a maximum when lnPA0(E) =0 E (ln E E E (E ) + ln '(E ') - ln E' E' 0 TOT (E )) = 0 (8.4) ( o TOT does not depend on E) ln (E ) - ln (E ) = ln '(E') - 0 = 0 ln '(E ') Note that a minus sign arises in changing from / E to / E'. 2001 by David Boal, Simon Fraser University. All rights reserved; further resale or copying is strictly prohibited. PHYS 445 Lecture 8 - Interacting systems 8-5 ~ This equation by itself does not specify E : rather, it gives a family of E-E' values for which the slopes of the two distributions agree. To determine which member of the family is the solution, one must impose the condition E' = Eo - E. At equilibrium, ln / E is the same for both systems in thermal contact, according to Eq. (8.4). Thus, ln / E is a very useful quantity, which we define as : ln 1 (8.5) E kBT Units: -1 has units of energy kB is a constant, with units of energy T is a dimensionless parameter, identified with temperature. As will be shown, ln is also a useful quantity. Using the same constant kB, we define another quantity called the entropy S kBln . (8.6) Hence, the temperature can alternately be extracted from S T= E At equilibrium, maximizing P implies that S + S' is a maximum T = T' (systems in thermal contact have the same temperature). (8.7) 2001 by David Boal, Simon Fraser University. All rights reserved; further resale or copying is strictly prohibited.
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Simon Fraser - PHYS - 445
PHYS 445 Lecture 9 - Temperature and specific heat Lecture 9 - Temperature and specific heat What's Important: thermal equilibrium temperature zeroth law of thermodynamics equipartition theorem specific heat of an ideal gas Text: Reif Approach to equilibr
Simon Fraser - PHYS - 445
PHYS 445 Lecture 10 - Systems in thermal contact Lecture 10 - Systems in thermal contact What's Important: heat flow heat reservoirs thermal contact mechanical contact Text: Reif Heat flow (not covered in class)10 - 1This result is rather intuitive, but
Simon Fraser - PHYS - 445
PHYS 445 Lecture 11 - Thermodynamics Lecture 11 - Thermodynamics What's Important: laws of thermodyncamics determination of kB why does thermodynamics work? Text: Reif Laws of thermodynamics11 - 1Starting with the microscopic picture of statistical mech
Simon Fraser - PHYS - 445
PHYS 445 Lecture 12 - Ensembles Lecture 12 - Ensembles12 - 1What's Important: ensembles spin - 1/2 particles in a magnetic field Text: Reif Demonstrations: magnet and compasses on an overhead projector magnetization and temperature - use Monel (Ni+Cu) a
Simon Fraser - PHYS - 445
PHYS 445 Lecture 13 - Partition function Z Lecture 13 - Partition function Z What's Important: partition function fluctuations and specific heat work and Z entropy and Z Text: Reif Partition function13 - 1The sum over the Boltzmann factors exp(-Er) appe
Simon Fraser - PHYS - 445
PHYS 445 Lecture 14 - Grand canonical ensemble Lecture 14 - Grand canonical ensemble What's Important: weakly interacting systems entropy and probability grand canonical ensemble Text: Reif14 - 1Secs. 6.7 and 6.8 on approximation techniques can be read
Simon Fraser - PHYS - 445
PHYS 445 Lecture 15 - Equipartition theorem Lecture 15 - Equipartition theorem What's Important: equipartition theorem applications: ideal gas, harmonic oscilator, 3D lattice Text: Reif Skip Secs. 7.1 to 7.4 Cheap tricks: equipartition theorem15 - 1A si
Simon Fraser - PHYS - 445
PHYS 445 Lecture 16 - Quantum oscillators Lecture 16 - Quantum oscillators What's Important: quantum oscillator at T > 0 continuous quantum states Text: Reif Quantum oscillators16 - 1In the previous lecture we used the classical equipartition theorem to
Simon Fraser - PHYS - 445
PHYS 445 Lecture 17 - Ideal gas in detail Lecture 17 - Ideal gas in detail What's Important: phase space of non-interacting particles Maxwell-Boltzmann distribution Text: Reif Phase space of non-interacting particles17 - 1An ideal gas is one in which pa
Simon Fraser - PHYS - 445
PHYS 445 Lecture 18 - Maxwell-Boltzmann distribution Lecture 18 - Maxwell-Boltzmann distribution What's Important: mean speeds molecular flux Text: Reif Mean speeds18 - 1The Maxwell-Boltzmann speed distribution that was derived in the previous lecture h
Simon Fraser - PHYS - 445
PHYS 445 Lecture 19 - MB continued Lecture 19 - MB continued What's Important: pressure of an ideal gas Text: Reif Pressure of an ideal gas Our picture of an ideal gas hitting a wall is19 - 1z - directionWith each collision, an amount of momentum 2mvz
Simon Fraser - PHYS - 445
PHYS 445 Lecture 20 - Quantum statistics Lecture 20 - Quantum statistics What's Important: quantum statistics Text: Reif Quantum statistics20 - 1The quantum approach to mechanics can be formulated in a statistical form using expectation values or means.
Simon Fraser - PHYS - 445
PHYS 445 Lecture 21 - Indistinguishable particles Lecture 21 - Indistinguishable particles What's Important: number distributions for MB, photons. Text: Reif Secs. 9.4-9.7; skip 9.321 - 1In the previous lecture, we established that the mean number densi
Simon Fraser - PHYS - 445
PHYS 445 Lecture 22 - Bosons Lecture 22 - Bosons What's Important: partition function number distribution condensation Text: Reif Boson partition function22 - 1We now tackle the general problem of Bose-Einstein statistics. The situation is more difficul
Simon Fraser - PHYS - 445
PHYS 445 Lecture 23 - Fermions Lecture 23 - Fermions23 - 1What's Important: Fermi-Dirac statistics comparisons among distributions Fermi energy Text: ReifFermi-Dirac statistics The Fermi-Dirac distribution can be handled in a similar way to the Bose-Ei
Simon Fraser - PHYS - 445
PHYS 445 Lecture 24 - Density of states Lecture 24 - Density of states What's Important: density of states in phase space Text: Reif Counting quantum states24 - 1Some time back, we said that we needed to introduce a "density of states" factor in order t
Simon Fraser - PHYS - 445
PHYS 445 Lecture 25 - T = 0 Fermi gas Lecture 25 - T = 0 Fermi gas What's Important: T = 0 Fermi gas metals neutron stars Text: Reif T=0 Fermi gas25 - 1The previous lecture for the density of states in phase space dealt only with the energetics, not the
Simon Fraser - PHYS - 445
PHYS 445 Lecture 26 - Black-body radiation I Lecture 26 - Black-body radiation I What's Important: number density energy density Text: Reif26 - 1In our previous discussion of photons, we established that the mean number of photons with energy i is 1 ni
Simon Fraser - PHYS - 445
PHYS 445 Lecture 27 - Black-body radiation II Lecture 27 - Black-body radiation II What's Important: radiation pressure radiative power Text: Reif Radiation pressure The general definition of the mean force ln Z = h which for the mean pressure implies ln
Simon Fraser - PHYS - 445
PHYS 445 Lecture 28 - Superfluids Lecture 28 - Superfluids What's Important: 4 He condensation superfluids Bose-Einstein condensation Text: Reif428 - 1He condensationAs 4He is cooled, it undergoes a phase transition to a liquid state (referred to as H
Simon Fraser - PHYS - 445
PHYS 445 Lecture 29 - Heat capacities in metals Lecture 29 - Heat capacities in metals What's Important: electrons in metals heat capacities Text: Reif Sec. 19.7; Kittel Chap. 729 - 1Heat capacities in metals are covered in two lectures. Here, the exper
Simon Fraser - PHYS - 445
PHYS 445 Lecture 30 - Low temperature Fermi gas Lecture 30 - Low temperature Fermi gas What's Important: heat capacity for ideal Fermi gas Text: Reif Heat capacity for ideal Fermi gas30 - 1This lecture contains a somewhat lengthy mathematical examinatio
Simon Fraser - PHYS - 445
PHYS 445 Lecture 31 - Interactions: Phase transitions Lecture 31 - Interactions: Phase transitions What's Important: galaxy formation galactic evolution Text: Reif Phase transitions31 - 1Most of the systems considered so far in this course have consiste
Simon Fraser - PHYS - 445
PHYS 445 Lecture 32 - Ising model Lecture 32 - Ising model What's Important: Ising model in 3D Text: Reif Ising model32 - 1In the previous lecture, we considered the effects of dimensionality on the existence of phase transitions, using a spin system as
Simon Fraser - PHYS - 445
PHYS 445 Lecture 33 - Non-ideal classical gases Lecture 33 - Non-ideal classical gases What's Important: non-ideal classical gases virial coefficient Text: Reif Non-ideal classical gases33 - 1The previous two lectures on phase transitions have dealt wit
Simon Fraser - PHYS - 445
PHYS 445 Lecture 34 - Van der Waals equation Lecture 34 - Van der Waals equation What's Important: B2 for hard spheres B2 for attraction and repulsion van der Waals equation Text: Reif Second virial coefficient34 - 1At the end of the previous lecture, w
Simon Fraser - PHYS - 445
PHYS 445 Supplement - Quick and dirty quantum mechanics Supplement - Quick and dirty quantum mechanics for PHYS 445 What's Important: old quantum theory particle in a 1-D box rigid rotor harmonic oscillator Old quantum theoryS-1A very simple approach to
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University of Texas - M - 2326
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University of Texas - M - 2326
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