Statistical Thermodynamics Flashcards

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1
Q

Number of ways of putting n different balls into n boxes

A

No. of microstates = n!

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2
Q

Number of ways of putting r different balls into n boxes (r<n)

A

No. of microstates = n!/(n-r)!

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3
Q

Number of ways of putting r identical balls into n boxes

A

No. of microstates = n!/r!(n-r)!

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4
Q

Ensemble average

A
  1. Take a single system and follow it over a long time; so that the system goes through all possible configurations
  2. Take a large number if identical but randomly configured systems and average over these at a single snapshot in time (this is the ensemble average)
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5
Q

Micro canonical ensemble

A

Isolated system with fixed U,V,N

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6
Q

Canonical ensemble

A

System is in contact with a thermal reservoir. V,N,T fixed for the system

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7
Q

Grand canonical ensemble

A

System can exchange heat and particles with the reservoir. V,T, mu fixed for the system

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8
Q

Principle of equal equilibrium probability

A

When a thermally isolated system comes into thermal equilibrium then the state probabilities of any set of mutually accessible states become equal. In a micro canonical ensemble there is equal probability of any state being occupied

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9
Q

Ergodic hypothesis

A

Given enough time the systems will explore all possible microstates and will spend an equal amount of time in each of them.
Implication: in equilibrium an isolated system will adopt the macro state with the most microstates

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10
Q

Boltzmann equation for entropy

A

S = kb * ln Omega

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11
Q

Boltzmann distribution function

A

P(Ei) proportional to exp(-Ei/kbT)

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12
Q

Properties of Boltzmann Distribution Function

A

Lower T- lower energy states more likely to be occupied
Infinite temperature- all states equally likely

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13
Q

Boltzmann-Gibbs Entropy

A

S = -Kb Sumi

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14
Q

In 3D the number of states between k and k+dk

A

g(k)dk = 4pik^2dk * V/(2pi)^3

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15
Q

The partition function for indistinguishable atoms: What conditions are required for the approximation of N! to hold?

A

As long as we can neglect any atoms which have the same quantum numbers. Okay as long as the number of possible states is much larger than the number of atoms

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16
Q

Sackur-Tetrode Equation

A

S = Nkb [ln(V/lambda^3 *N) +5/2]

17
Q

Gibbs Paradox (Question)

A

What if the particles have some property X which we can’t measure (but someone else could). So they appear to be identical but they are not. Would the entropy change when we are able to measure the difference.

18
Q

Gibbs Paradox (answer)

A

Yes, entropy depends on our knowledge of the system. The way to interpret the extra entropy is that after mixing A,B to return the system to its original state we would need to do work on the system equal to at least T*DeltaS

19
Q

Fermions

A

Particles with half integer spin

20
Q

Pauli Exclusion Principle

A

We can only have 1 fermion in any single quantum state

21
Q

Bosons

A

Particles with integer spin

22
Q

Classical limit

A

At low occupancy the fermi-Dirac, Bose-Einstein and Boltzmann distribution functions all become equal, because there is very little chance of multiple occupancy so the quantum nature of the particles is irrelevant