1. Multiplicity, Entropy, Second & Third Law Of Thermodynamics Flashcards

1
Q

Multiplicity of Einstein Solid

A

Ω(N, q) = (q + N - 1)! / q! (N- 1)!

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2
Q

Multiplicity of Two-State Paramagnet System

A

Ω(N up) = N! / N up! N down!

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3
Q

Fundamental Assumption of Statistical Mechanics

A

In an isolated system in thermal equilibrium, all accessible microstates are equally probable.

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4
Q

Second Law of Thermodynamics

A

For spontaneous processes, the entropy of the universe increases and approaching greater disorder and randomness.
A system will naturally evolve towards the macro state with the highest multiplicity (most possible arrangements of its micro states)

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5
Q

Multiplicity of Large Einstein Solid

A

lnΩ = ln((q + N)! / q!N1)

If q&raquo_space; N

Ω(N, q) = e^Nln(q/N)e^N = (eq/N)^N

If q &laquo_space;N

Ω(N, q) = (Ne/q)^q

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6
Q

Multiplicity of Mono-atomic Ideal Gas

A

In 3D:

Ω = V Vp / h^3
Ω N = 1/N! (V^N/ h^3N)

1D:
L Lp/ Δx Δpx = L Lp/h

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7
Q

Entropy
(Relationship between Entropy and Multiplicity)

A

S = klnΩ

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8
Q

Entropy of Large Einstein Solid

A

S = kln(eq/N)^N = Nk[ln(q/N) + 1]

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9
Q

Entropy of an Ideal Gas

A

S = Nk[ ln( V/N (4pimU/3Nh^2)^3/2) + 5/2] (Sackur-Tetrode Equation)

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10
Q

Change in Entropy of Ideal Gas

A

Change in S = Nkln(Vf/Vi) (General)

Change in S = Q/T (any Quasistatic process)

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11
Q

Entropy of Mixing

A

Change in Sa = Nkln(Vf/Vi) = Nkln2

Change in S total = Change in Sa + Change in Sb = 2Nkln2

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12
Q

Relationship between Temperature, Entropy, and Potential Energy

A

1/T = (dS/dU)N, V —> T = (dU/dS) N, V

Energy will always tend to close into Theo object with stepper S vs. U graph and out of object with shallows S vs. U graph. (Steep slope is low temp, shallow is high temp)

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13
Q

Thermodynamic Identity & How it’s derived

A

dU = TdS - PdV

S = f(U, V)
dS = dS/dU dU + dS/dV dV
dS = 1/T dU + P/T dV
dU = TdS - PdV

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14
Q

Change in Entropy

A

dS = Q/T (constant volume, no work)

dS = CvdT/T (T is changing)
- integrate for ΔS

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15
Q

Third Law of Thermodynamics

A

The entropy of a system approaches a constant value as the temperature approaches absolute zero. (System’s unique, lowest energy state)

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16
Q

Relationship between Pressure, Temperature, Entropy, Volume

A

P = T (dS/dV) N, U

17
Q

Diffusive Equilibrium & Grand Thermodynamic Identity

A

dSA/ dNA = dSB/dNB

-T dSA/dNA = -TdS/dNB at equilibrium —> this is chemical potential μ = -T (dS/dN) V, U

Thus we can write GTI:
S(U, V, N)
dS = dS/dU dU + dS/dV dV + dS/dN dN
dU = TdS - PdV + μdN
dS = 1/T dU + P/T dV - μ/T dN

For Diffusive Equilibrium:

μA = μB

System that has a larger dS/dN wants more particles because it has a smaller chemical potential.
Particles tend to flow toward lower values of chemical potential.

18
Q

Total Entropy at Equilibrium

A

(dS total/dUA) NA, VA = 0 and (dS total/ dNA) UA, VA = 0

(Total entropy at maximum)

19
Q

Chemical Potential

A

U & V Fixed:
0 = TdS + μdN —> μ = -T (dS/dN) U, V

S & V fixed:
dU = μdN —> μ = (dU/dN) S, V

μ had units of energy; amount by which system’s energy changes, when you add one particle and keep the entropy and volume fixed.

20
Q

Sacker Tetrode Equation

A

Describes partition function (statistical properties) of gas with indistinguishable particles.

Partition:
Z = (V/ λt^3)^N / N!

This is proportional to multiplicity as it represents number of accessible states for system.

Ω ~ Z ~ (V/ λt^3)^N / N!

Finding entropy of this gives:

S = kBln(1/N! (V/ λt^3)^N) = e/N (V/ λt^3)^N

Stirling Approximation which is lnN! =~ NlnN - N for large can be used to simplify to:

S = Nkb(ln (V/ Nλt^3) + 5/2)

Which represents third law of thermodynamics! (If gas cooled down to 0, entropy goes to 0)