Thermodynamics and Gas Laws Review

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Flashcards covering key concepts and formulas from lecture notes on gas laws and thermodynamics, presented in a vocabulary style.

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50 Terms

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Ideal Gas Law

pV = nRT

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Dalton’s Law of Partial Pressures

ptotal = Σ pi, with pi = yi p_total

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Molar volume at STP (1 bar, 273 K)

V_m ≈ 22.7 L mol⁻¹

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Average Molar Kinetic Energy

〈E_k〉 = (3/2)RT

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Root-mean-square speed (c_rms)

c_rms = √(3RT/M)

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Mean speed (c̄)

c̄ = √(8RT/πM)

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Most probable speed (c_mp)

c_mp = √(2RT/M)

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Compressibility Factor Z

Z = pV_m/(RT); ideal gas if Z=1

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van der Waals equation

(p + a n²/V²)(V − nb) = nRT

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van der Waals constants (a and b) from critical constants

b = RTc/(8pc), a = 27R²Tc²/(64pc)

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Virial expansion form

Z = 1 + B(T)/V_m + …

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First Law of Thermodynamics

∆U = q + w

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Work at constant external pressure

w = −p_ext ∆V

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Work reversible isothermal (ideal gas)

w = −nRT ln(V₂/V₁)

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Change in Internal Energy (∆U) for isothermal ideal gas

∆U = 0

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Change in Enthalpy (∆H) for isothermal ideal gas

∆H = 0

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Adiabatic reversible relation (pressure and volume)

pV^γ = const

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Adiabatic reversible relation (temperature and volume)

TV^(γ−1) = const

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Adiabatic work expression

w = ∆U = nC_V∆T

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Definition of Enthalpy H

H = U + pV

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Heat at constant pressure (q_p)

q_p = ∆H

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Heat at constant volume (q_V)

q_V = ∆U

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Mayer’s relation (ideal gas)

Cp − Cv = R

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Enthalpy change (∆H) for ideal gas formula

∆H = n ∫ C_p dT

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Internal energy change (∆U) for ideal gas formula

∆U = n ∫ C_v dT

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Standard enthalpy of reaction formula

rH° = Σν ∆fH°(products) − Σν ∆_fH°(reactants)

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Hess’s Law

Add reactions, add enthalpies

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Kirchhoff’s Law formula

rH(T₂) ≈ ∆rH(T₁) + ∆C_p ∆T

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Relation between ∆H and ∆U for ideal-gas reactions

∆H − ∆U = ∆n_g RT

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Internal pressure (π_T)

πT = (∂U/∂V)T

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Thermal expansion coefficient (α)

α = (1/V)(∂V/∂T)_p

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Isothermal compressibility (κ_T)

κT = −(1/V)(∂V/∂p)T

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Joule–Thomson coefficient (µ_JT)

µJT = (∂T/∂p)H = (V/C_p)(Tα − 1)

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Assumption defining an ideal gas

No intermolecular interactions; molecules occupy no volume; elastic collisions.

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Compressibility factor Z > 1

Indicates repulsions dominate (gas is less compressible).

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Compressibility factor Z < 1

Indicates attractions dominate (gas is more compressible).

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Origin of pressure in kinetic theory

From molecular collisions transferring momentum to container walls.

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Why average molar kinetic energy depends only on T

Because temperature measures average kinetic energy, independent of pressure or volume.

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First Law of Thermodynamics (in words)

Energy is conserved: the change in internal energy equals heat supplied plus work done on the system.

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Reason for maximum reversible work

External pressure is always infinitesimally less than system pressure, so the system does the most work possible without losing equilibrium.

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Distinction between isothermal and adiabatic expansion

Isothermal: T constant, ∆U=0, heat exchange balances work. Adiabatic: no heat exchange, T drops as system does work.

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Why ∆U is only a function of T for ideal gases

Because ideal gas internal energy depends only on kinetic energy, which is temperature dependent.

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Why ∆H ≈ ∆U for condensed phases

Because the pV term is negligible relative to the large energies of chemical bonds.

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Significance of Hess’s Law

Enthalpy is a state function, independent of path.

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Significance of Kirchhoff’s Law

Reflects the temperature dependence of reaction enthalpy due to differences in heat capacities of reactants and products.

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Meaning of ∆H − ∆U = ∆n_gRT

The difference between enthalpy and internal energy changes comes from expansion work of changing gas moles.

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Information conveyed by internal pressure (π_T)

How internal energy changes with volume at constant T; measures intermolecular interactions.

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Information conveyed by thermal expansion coefficient (α)

Fractional change in volume per degree rise at constant pressure.

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Information conveyed by isothermal compressibility (κ_T)

Fractional change in volume per unit pressure drop at constant T.

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Information conveyed by Joule–Thomson coefficient (µ_JT)

Whether a real gas cools or heats upon expansion at constant enthalpy.