Section 7: Statistical Thermodynamics Flashcards

(61 cards)

1
Q

consider balloon of volume V held within thermally-isolated vacuum chamber of volume 2V, although the gas expands in volume,

A

no work is done on the surroundings

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2
Q

entropy in a joule-free expansion: balloon bursts and

A

the gas is free to expand

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3
Q

entropy in a joule free expansion: for adiabatic walls

A

δQ is also zero so Uf=Ui

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4
Q

entropy in a joule free expansion - for an ideal as, U=

A

U(T) so there is no temperature change

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5
Q

entropy in a joule free expansion - in practice most gases

A

cool slightly and we can measure the joule coefficient

uj=(dT/dV)u

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6
Q

joule free expansion - initial and final states are

A

equilibria so delta s is well defined

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7
Q

joule free expansion - for an ideal gas with s(T,V), delta s=

A

cvlnT2/T1 + Rln V2/V1 = Rln2

so can have a change of entropy without heat input or thermal changes

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8
Q

in the context of the kinetic theory of gases, entropy is often described as

A

the disorder of the particles

hard to quantify

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9
Q

consider two dice, each with six degenerate states or microstates.

the macrostate in this scenario is

A

the sum of the dice

eg for macrostates =3 can have microstates (1,2) or (2,1)

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10
Q

in a fluctuating system which macrostate is the most probable

A

the one with the largest number of microstates

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11
Q

the joule free expansion suggests that entropy depends on

A

how a gas is distributed

boltzmann then formulated the link as S=S(omega)

where omega = number of microstates

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12
Q

as entropy is extensive, the entropy of the total system should be

A

the sum of the two entropies SAB=SA+SB

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13
Q

if the two systems are independent then the number of microstates should be

A

the product of the individual numbers

omegaAB=omegaAomegaB

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14
Q

for the composite system, Boltzmann’s hypothesis should obey

A

S(ΩAB) = S(ΩAΩB) = S(ΩA)+S(ΩB)

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15
Q

S=

A

KB ln Ω

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16
Q

microstates for monatomic gas

A

for gas particles in a box, each particle has position r and momentum p

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17
Q

the likeliness of a microstate i is proportional to its

A

boltzmann factor e^-Bei

B is the thermodynamic beta used to simplify notation

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18
Q

lower energy states are more likely since

A

the exponent is negative

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19
Q

the actual probability of each state is also correlated to

A

how many states the system has

this means the probability is given by Pi=e^-Bei /Z

Z norm const

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20
Q

to quantify the normalsiation constant, use

A

the property that all probabilities have to sum to unity

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21
Q

normalisation constant Z is called

A

the partition function

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22
Q

the expectation value for a property A can be found by

A

averaging over the allowed microstates

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23
Q

if you interpret different microstates as fluctuations, then you could consider this average as a

A

time-average over the fluctuations

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24
Q

link between thermodynamic potential and the partition function

A

F=-KBT ln Z

from F we can derive most other thermodynamic properties

link between statistical and classical approaches

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25
calculation strategy
identify energy levels determine partition function determine helmholtz function use standard relations to obtain U,S,P etc
26
a change in internal energy can be achieved by
changing the probabilities or the energy levels
27
energy levels of a system are goverend by
external parameters such as volume and applied fields
28
when energy levels are fixed (dei=0 for all i) the only way to change the internal energy is
change the distribution
29
adding heat or adding thermal energy,
shifts the probabilities and hence the population of the energy levels
30
a classical particle in a parabolic potential executes
simple harmonic motion
31
spacing of energy levels in QHO
evenly spaced
32
energy of the ground state of QHO
not=0 e0=1/2 h bar w even at T=0K, QHO is not motionless - compatible with the uncertainty principle
33
the harmonic oscillator is the basis for
models of molecular vibrations
34
anharmonic terms can be added to the potential to improve
the approximation
35
if the separation of energy levels is much larger than KBT
populating upper levels is unlikely would expect to have heat capacity CV tending to zero
36
einstein model of heat capacity
modelling the bonds between atoms in a crystal lattice as springs so that each atom can undergo harmonic oscillations in 3D
37
heating the crystal raises
vibrational energy which characerises frequency wE
38
in the limit T approaching infinity, CV=
3R agrees with the Dulong-Petit law
39
two critical limitations of the einstein model
there is a single frequency of oscillation the vibrational modes are independent
40
debye model fixes limitations by considering
a spectrum of frequencies that describe coupled vibrations of atoms known as phonons
41
einstein model made the assumption that
only single frequency of oscillations inside the crystal but higher harmonic frequencies would also be supported by the lattice structure
42
beware! for particle in a box
only for a single particle gibbs paradox problem with particle indistinguishability
43
Gibbs paradox
whilst the pressure of N particles is just a multiple, neither U nor S for a gas are N times the above resutls
44
counting many particles states is impractical - its simpler to
consider energy levels
45
in a small system, the number of states of a givn energy is
the degeneracy
46
in a large systemm it is better to move to
integrating over a density of states
47
blackbody radiation has the following characteristics
absorbs all incient photon radiation without reflection at eqbm radiates as much energy as it absorbs re-radiates at energies characterised by the body's temp
48
main problem with classical approach
every mode and hence every energy is assumed to have the same probability
49
when N=1 it is easy to
assign independent quantum states and if atoms are locked in a crystal lattice, it's still easy to distinguish different states
50
unconstrained atoms or molecules of the same type are
indistinguishable
51
a system of N particles ultimately has
one combined wavefunction
52
for two particles, Ψ(x1,x2) describes
particle 1 at position x1 and particle 2 at position x2 exchanging the particles gives Ψ(x2,x1)
53
we measure |Ψ|^2 and if the particles are indistinguishable the measurement should give
the same result under a swap of the particles
54
for theta=pi, the wavefunction is
antisymmetric under exchange of the particles fermions all with half-integer spin
55
for theta=0, the wavefunction is
symmetric under exchange of particles bosons integer spin
56
the N-particle wavefunction can be expressed as
a combination of one-particle wavefunctions
57
setting i=j yeilds what for fermnions
zero pauli exclusion principle
58
is i=j allowed for bosons
yes
59
for non-interacting particles, the energy eigenvalue is
jsut the summation of the individual one-particle energies
60
changes to the partition function
1. there is only one i,j quantum state so need to avoid double counting 2. fermions can't all be in the same quantum state
61