330 Exam 2 Flashcards

1
Q

First Law of Thermodynamics

A

Energy of the universe is CONSTANT, it interconverts between the system and surroundings (change of energy of the system is equal to the (-) change of the energy in the surroundings)

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2
Q

DeltaG def

A

The Gibbs free energy tells us if a reaction is sponatneous under a set of condtions

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3
Q

What is a partition function? (q)

A

THe number of thermally accessible at a given temperature, it is a unitless quantity but it really has stealth units of states

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4
Q

Why must Delta G of a spontaneous process be negative

A

Bc it increases the entropy of the universe

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5
Q

KT»>E VS. E»>KT

A

KT> means that that energy levels can be seen as continuous energy spacings at high temperatures
But @ KT<, energy levels are discrete relative to thermal energy and you can get an integral in this case

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6
Q

4 ways to calculate entropy

A
  1. S(macrostate) =kln(W)
    per mol: **=Rln(W) **
  2. For a phase transition at constant pressure:** dS=dH/T**
  3. For heating:
    **S= Cpln (T2/T1) **
  4. Mixing of 2 gasses nk or nR * ln(v1+v2/v2) for each gas and then add them up
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7
Q

2nd law of thermodynamics

A

For any SPONTANEOUS process dS(of the universe)>0 as the universe is moving toward the most likely macrostate, to get to dS=0

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8
Q

Result of 2nd law of thermodynamics

A

dSuniverse= dSsys + dS surroundings
so that dSsys + dSsurr >0
dS surroundings = dHsurr/T
(can manipulate this from the first law and say dHsurr=-dHsys
THEN get dHsurroundings=-dHsys/T

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9
Q

2 ways to increase the internal energy of the system

A

Heat and work

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10
Q

Explain why heat capacity becomes “infinite” at a phase transition (and must approach zero as temperature approaches absolute zero)

A

Can think about it in terms of statistical mechanics- we are goiong from one collection states to a larger collection of states the temp is not going to heat a substance but to make this transition, hence the temperature does not increase the substance

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11
Q

Rotational partition function energy vs KT

A

For WIDE energy spacings, hv»>KT so q approaches 1
for small enrergy spacings hv«<KT means that all temps are thermally accessible

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12
Q

Define entropy statistically

A

How many microstates correspond to a macrostate

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13
Q

Law of large numbers

A

When we are dealing with very large number of molecules, certain macrostates are so overwhelimingly likely that they are the only thing that we observe

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14
Q

Define a state function
what it means to be either “path-independent” or “path-dependent?”

A

A state function is a function that obnly dependents on the starting and ending state of a system and NOT the path that it takes to get there
Energy is a state function
BUT the change in energy is not

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15
Q

Work is path dependent

A

The action of force over a distance, depends on how long the path is
example if you but a boot on a car, the change in energy is the same but if the boot means the car loses energy to friction and you need to increase work and push harder

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16
Q

When pressure is constant…

A

Isobaric conditions allow us to constrain a process to under constant pressure so that q transfer = change in enthalpy plus P(deltaV)
(where q=mcdT)

17
Q

Third law of therodynamics

A

The Third Law of Thermodynamics Says That the Entropy
of a Perfect Crystal Is Zero at 0 K is ZERO

18
Q

First law in math

A

dU=q+w

19
Q

Standard enthalpy of formation

A

dH that makes 1 mol of a substance from its elements

20
Q

Key for melting/vaporizing heating cooling problems

A

(-)heat out of a substance= heat into other substance
when you add heat to a substance, you can increase T (mcdT) OR break bonds @ constant temp

21
Q

Enthaply change depends

A

weakly on temp

22
Q

Standard enthalpy of a rxn

A

H products stnd- H reactants stnd
(Hess’ law)

23
Q

If specific heat is the same for reactants and products

A

Then enthalpy is temp dependent

24
Q

Specific heat

A

Cv=dU/dT or how much average energy changes with an increase in T

25
Q

Room temp partition function

A

Many states can be populated at room temp

26
Q

Comparing Q/K/dG

A

Q<K, dG<0 -rxn goes forward to reach equilibrium
Q>K, dG>0 - rxn goes backwards to get to equilibrium
Q=K, G=0 @ equilibrium, life is good

27
Q

Comparing dG and dS

A

dGsys<0, process is spontaneous
dGsys>0, reverse process is spontaneous
dGsys=0, system is at equilibrium

28
Q

Rotational partion function

A

=KT/B

29
Q

Average rotational energy

A

KT (or RT if PER MOL)

30
Q

When asked for probability of being at any J level

A

Multiply the probabilty times the degeneracy

31
Q

Theta rot (rotational temp)

A

=K/T

32
Q

Rotatational temp is directly proportional

A

=1/I