Thermodynamics Flashcards

(58 cards)

1
Q

making bonds is ___
breaking bonds is ___

A

make = exothermic
break = endothermic

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2
Q

Second Law of Thermodynamics

A

In a spontaneous process, the entropy of the Universe increases

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3
Q

molecular interpretation of entropy

A

randomness = how do molecules distribute themselves amongst available energy levels
–> statistical analysis

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4
Q

in statistical analysis, what does the weight of a distribution refer to?

A

the total number of ways a particular configuration can be achieved

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5
Q

what is the most probable distribution?

A

the one configuration with a larger value W than all the others
= the Boltzmann Distribution

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6
Q

Boltzmann Distribution eqn for population of level i, n(i), with energy ε(i)
+ interpret

A

n(i) = n(0) exp (-ε(i) / kT)

where k is Boltzmann’s constant
T is temperature

ie. as the energy of a level increases, its population decreases
as Temp raised, molecules move to higher energy levels

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7
Q

Eqn relating entropy to number of ways W

A

S = k lnW

k: Boltzmann’s constant
W: weight, ways

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8
Q

molecular energy level distribution when a system is heated

A

energy is supplied, some molecules move to higher energy levels
–> more spread out amongst energy levels so more ways of achieving the distribution, hence entropy increases

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9
Q

molecular energy level distribution when a system expands

A

when a system expands, the spacing of translational energy levels DECREASES
hence more energy levels available to the molecules
distributed over more levels, W increases, S increases

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10
Q

how does the size of entropy change depend on the T of a system?

A

the increase in entropy resulting from a certain amount of heat being supplied is GREATER the LOWER the temperature of the system

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11
Q

eqn classical definition of entropy

differential form

A

dS = 𝛿q(rev) / T

NOTE: even if the process itself is not reversible, must work out what the heat would be if we were to go by a reversible path!

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12
Q

eqn calculate entropy change of surroundings

A

surroundings are so large that all heat transfers are seen as reversible

∆S(surr) = q(surr) / T(surr) = -q(sys) / T(sys)
for a finite change

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13
Q

relate spontaneity of a process to ∆S(univ)

A

+ve = spontaneous (entropy of universe increases)
-ve = not spontaneous
= 0 is equilibrium, no tendency for further change

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14
Q

The First Law of Thermodynamics + eqn

A

energy cannot be created or destroyed but is transformed from one form into another

∆U = q + w

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15
Q

what are the different “forms” of energy?

A

heat, work and internal energy

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16
Q

key different between internal energy and heat/work

A

internal energy is a STATE function
heat/work are PATH functions

note that the symbol ‘∆’ is only appropriate for state functions

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17
Q

derive eqn for work done on an ideal gas by expansion

A

piston with area A experiences p(external)
force on the piston due to external pressure is p(ext) * A

small amount of work done BY the gas is force x distance dx (piston moved out)
δw = p(ext) * A dx = p(ext) dV

work done ON the gas: δw = - p(ext) dV

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18
Q

when a gas expands, what happens to the internal energy?

A

work is done so Internal energy falls

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19
Q

derive expression for expansion work done against CONSTANT external pressure

A

integrate p(ext) dV for an expansion between Vi and Vf
p(ext) constant, move out of integral

w = - p(ext) [Vf-Vi]

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20
Q

what must p(ext) be to do maximum expansion work for a gas in a cylinder?

A

to maximise work done, external pressure needs to be as high as possible but cannot exceed internal pressure (or else compression would occur, not expansion)
–> p(ext) infinitesimally smaller than p(int)

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21
Q

define reversible reaction

A

a process whose direction can be changed by an infinitesimal change in some variable

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22
Q

reversible vs spontaneous reactions

A

reversible:
infinitely slow
at equilibrium
do max work

irreversible = spontaneous:
finite rate
not at equilibrium
less than max work

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23
Q

how to find the expression for work done in a finite expansion for an ideal gas expanding reversibly

A

essentially, p(ext) = p(int)
work = integral of p(int) dV between Vi and Vf

for ideal gas, p(int)V=nRT –> sub for p(int)
Assume isothermal (constant T)

w(rev) = - nRT ln(Vf/Vi)

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24
Q

what is an indicator diagram?

A

essentially a graph of p(ext) vs V
work done in a finite expansion is the integral of p(ext)dV between Vi and Vf, so work done is the area under the curve

25
what can be said about the magnitude of heat in a reversible process?
the magnitude of heat is a MAXIMUM because for any particular initial and final states, ∆U is constant as ∆U = q+w, if a path is changed such that w increases, q must change by the same amount to keep ∆U fixed hence q must also be at a maximum for such a path
26
internal energy of an ideal gas
depends ONLY on temperature because particles do not interact, if heat added it is only stored in Ek hence for isothermal expansion, ∆U=0 and w'=q
27
expression for heat for an isothermal, reversible expansion of ideal gas
q(rev) = w' = nRT ln(Vf/Vi)
28
expression for entropy change for any isothermal expansion of an ideal gas from Vi to Vf
∆S = nR ln(Vf/Vi) confirming entropy increases as volume increases from q(rev) = nRT ln(Vf/Vi) and ∆S=q(rev)/T
29
first law for infinitesimal changes
dU = 𝛿q + 𝛿w note: 𝛿 not d because d implies "a small change in" but heat and work are state functions hence must talk about "a small amount of" heat/work
30
first law for infinitesimal changes and expansion work only
dU = 𝛿q - p(ext)dV
31
expression for heat absorbed under conditions of constant volume
dU = 𝛿q(const vol) because p(ext)dV = 0, no expansion so to find ∆U, measure the heat under constant volume conditions
32
relationship between heat supplied and temperature change
q = c∆T where c is the heat capacity q = nC(m) ∆T where C(m) is molar heat capacity and n is moles
33
definition of heat capacity at constant volume
C(V,m) = (∂U(m) / ∂T)|V
34
what is enthalpy? give eqn
H = U + pV a state function whose value is equal to the heat supplied at constant pressure (sum of internal energy and pV work)
35
complete differential of the enthalpy equation
dH = dU + pdV + Vdp from H=U+pV
36
relate enthalpy change to heat
dH = 𝛿q(const.press) enthalpy change is equal to heat measured under conditions of constant pressure | by subbing dU=𝛿q-pdV and taking Vdp=0, const press
37
definition of heat capacity at constant pressure
C(p,m) = (∂H(m) / ∂T) |p
38
equation for converting enthalpy at one temperature to another
Hm(T2) = Hm(T1) + C(p,m) [T2-T1] from integrating the definition of heat cap at constant pressure, assuming constant C note C(p,m) is a molar quantity and as such gives change in molar enthalpy
39
how to express entropy S in terms of heat capacity (something you can actually measure!)
using dS = dH/T and dH(m) = C(p,m) dT over wide temp range, CANNOT assume constant C integrate C(T)/T wrt T over some wide temp range
40
justification for entropy at absolute zero = 0
at absolute 0, kT goes to 0 so all molecules in lowest energy level (ground state), only one way to arrange so W=1 and S=klnW=0.
41
absolute entropy S(T*) expression
= integral of Cp,m(T)/T wrt T + sum of entropy of phase changes
42
convert entropy S at T1 to T2
Sm(T2) = Sm(T1) + C(p,m) ln(T2/T1) from integrating Cp,m/T wrt dT assuming constant C over small T1 to T2
43
define Gibbs energy state function
∆G = ∆H - T∆S all for the SYSTEM
44
relate change in G to spontaneity
dG < 0 = spontaneous at equilibrium G reaches a minimum, dG =0
45
the first thermodynamic Master Equation
dU = TdS - pdV aka "First and Second Laws combined" dU = 𝛿q-𝛿W for pV work, and 𝛿q=TdS
46
the second thermodynamic Master Equation
dG = Vdp - SdT from the differential form of H=U+pV and sub in first master eqn then sub dH expression into differential form of G=H-TS
47
how does Gibbs energy vary with pressure (constant T)? for ideal gas
dG = Vdp (dT=0) sub V = nRT/p and integrate --> Gm(p) = Gm˚ + RT ln(p/p˚)
48
how does Gibbs vary with volume at constant T?
V inversely proportional to p p2/p1 = V1/V2 sub in expression for G(p) G(V2) - G(V1) = nRT ln(V1/V2)
49
Gibbs-Helmholtz equation
d/dT (G/T) = -H/T^2 at constant pressure
50
general method: how to find Gibbs energy of mixtures
using partial pressures of gases (for ideal gases)
51
partial pressure defintion
p(i) = x(i) p(tot) where x(i) is the mole fraction of I
52
equation for Gibbs energy of a mixture of ideal gases
G = sum of n * Gm(p) n is number of moles, Gm(p) is molar gibbs energy for partial pressure of a species
53
what is the chemical potential for ideal gases?
µ is the same as molar gibbs energy so that G = sum of nµ 
54
what is the chemical potential for solutions?
µ(c) = µ˚ + RT ln(c/c˚) same as molar gibbs energy eqn except using conc instead of pressure for ideal solutions
55
what is the chemical potential of a solid or liquid?
solids and pure liquids are always in standard state so = µ˚
56
definition of standard state
standard state of a substance =. in pure form at one bar and specified temp
57
∆rH˚ =
sum of standard enthalpies of formation * stoic coefficients
58