Thermodynamics

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Last updated 8:09 AM on 4/15/26
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40 Terms

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1st law of thermodynamics

energy cannot be created or destroyed - only changed from one form to another

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how are system and surroundings related

delta Esystem = - delta Esurroundings

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internal energy U

energy associated with random disordered motion of molecules in a system

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how can U be changed

heat

work

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work

w = -P deltaV = -P(Vf-Vi)

transfer of energy from system to surroundings

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work = pos

surroundings are doing work on our system

i.e. system gains energy

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work = neg

system doing work on surrounding

i.e. system loses energy

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entropy S

a measure of how dispersed the energy is inside a closed or isolated system

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higher S

more energy dispersed

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lower S

energy less dispersed

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second law of thermodynamics

entropy S of an isolated system always increases

deltaS>0

ex: ice cube melting

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is the inital or final state of an isolated container more random

final state is less ordered and more random

system has become more disordered and entropy has increased

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can we revert back to original state

no unless we do work on the system

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reversible process

both system and surrounding can be reverted to original state after process has occured

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irreversible process

system and surrounding cannot be reverted to original state after process has occured

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how can we measure change of entropy delta S for a reversible process

delta S = qrev/T

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q rev

heat supplied reversible to the system

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microstate

when we look at a molecular system we want to know the number of diff ways molecules can be arranged

each individual arrangement = microstate

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how is microstate and entropy related

greater no. of microstates = greater entropy

S = kB ln(W)

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W

no. of microstates

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kB

boltzman constant

-> 1.38 x 10^-23

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how can we increase no. of microstates

increase volume

add heat

increase no. of molecules

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change in entropy of a system from one state to another

delta S = kB ln(W final) - kB ln(W initial)

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enthalpy H

heat content of a system at constant pressure

H = U + PV

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change in enthalpy delta H

amount of heat a system loses or gains

delta H = delta U + P delta V

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exothermic reaction

delta H is negative

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endothermic reaction

delta H is positive

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enthalpy vs internal energy

IE: sum of all molecular energies in a system

E: combo of internal energies + energy required to make space

so when heat is added enthalpy changes stays the same but if gas can expand some energy goes into work so internal energy increases less

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total entropy change of the universe

ΔSuniverse=ΔSsystem+ΔSsurroundings

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entropy change of surroundings

ΔSsurroundings = −ΔHsystem/T

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Gibbs free energy of a system

∆𝑮𝒔𝒚𝒔𝒕𝒆𝒎 = ∆𝑯𝒔𝒚𝒔𝒕𝒆𝒎 − 𝑻∆𝑺𝒔𝒚𝒔𝒕𝒆m

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neg delta G

spontaneous

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pos delta G

not spontaneous

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delta G = 0

equilibrium

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Clausius-Clapeyron equation

OR

P2 = P1e

<p>OR</p><p>P2 = P1e</p>
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equation for gibbs free energy under non-standard conditions

𝚫𝑮 = 𝚫𝑮 𝟎 + 𝑹𝑻𝒍𝒏 (Q)

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What is the relationship between ΔG° and K

𝚫𝑮 𝟎 = −𝑹𝑻𝒍𝒏 (K)

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If products are favoured at equilibrium

K>1

delta G0 < 0

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reactants are favoured at equilibrium

k < 1

delta G0 > 0

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neither reactants or products are favoured

K = 1

delta G0 = 0