Thermodynamics Exam 2

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39 Terms

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Intensive variables

do not depend on the size of the system

ex: pressure, temperature

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Extensive variables

directly proportional to the size of the system

ex: volume, energy, mass

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How do you make an intensive property from an extensive property?

extensive/n = intensive property

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When is the ideal gas law applicable?

  1. low pressure

  • gas is diluted enough that its molecules are far apart from each other on average that wen can ignore there intermediates (IMFs)

  1. High Temperature

  • at low temperature, gas becomes a liquid because the gases can fee the IMFs (the molecules slow down to interact


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Ideal gas equation of state

PV = RT

V= v bar, which equals V/n

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van der Waals equation (corrections/what it accounts for)

accounts for deviations from the ideal gas law

  1. low temperature

  2. high temperature


corrects:

  1. attractive forces

  2. molecular volume


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Figure 16.3

Shows that the ideal gas equation is not valid at high pressure

<p>Shows that the ideal gas equation is not valid at high pressure</p>
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Compressibility factor

Z > 1 : very high pressure

Vbar real > Vbar ideal

*If repulsive interactions are dominating


Z < 1 : intermediate pressure

Vbar real < Vbar ideal

*When attractive interactions are dominating

<p>Z &gt; 1 : very high pressure</p><p>Vbar real &gt; Vbar ideal</p><p>*If repulsive interactions are dominating</p><p></p><p>Z &lt; 1 : intermediate pressure</p><p>Vbar real &lt; Vbar ideal</p><p>*When attractive interactions are dominating </p>
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Figure 16.4

Shows that the effect of molecular attraction becomes less important at higher temperatures

<p>Shows that the effect of molecular attraction becomes less important at higher temperatures</p>
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Coexistence curve

Any point within this curve corresponds to liquid and gas coexisting in equilibrium with each other

  • At any point on or outside the curve, only one phase is present


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Law of Corresponding States

the properties of all gases are the same if we compare them under the same conditions relative to their critical point

  • predicted by Pc*V(bar)a/R*Tc which equals 3/8, indicating that this should be the same for all substances


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van der Waals equation (a and b)

a: corrects for attractive forces

  • Preal < Pideal

  • frequency and force of collisions with the walls are both reduced by attractive forces

  • Units: dm^6 * atm * mol^-2


b: corrects for the size of the molecules

  • Units: dm³ * mole^-1

  • Preal > Pideal


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van der Waals equation in terms of Z

(don’t need to memorize equation)

High pressure: first term dominates

  • volume of the molecules is not negligible

  • Zreal > Zideal

Low pressure: second term dominates

  • Zreal < Zideal


<p>(don’t need to memorize equation)</p><p>High pressure: first term dominates</p><ul><li><p>volume of the molecules is not negligible</p></li><li><p>Zreal &gt; Zideal</p></li></ul><p>Low pressure: second term dominates </p><ul><li><p>Zreal &lt; Zideal</p></li></ul><p></p>
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Isotherms

Holding temperature constant

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Figure 16.7

dashed line is a coexistence curve

Isotherm: temperature is held constant

  • at a higher and higher temperature, you get closer to the ideal gas law

  • dot = critical point

  • at a temperature greater than the critical point (T>Tc), the gas can’t be condensed

  • Experiment!!


<p>dashed line is a coexistence curve </p><p>Isotherm: temperature is held constant </p><ul><li><p>at a higher and higher temperature, you get closer to the ideal gas law</p></li><li><p>dot = critical point</p></li><li><p>at a temperature greater than the critical point (T&gt;Tc), the gas can’t be condensed </p></li><li><p>Experiment!!</p></li></ul><p></p>
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Figure 16.8

Pressure-volume isothenns of carbon dioxide around its critical temperature, as calculated from the van der Waals equation

  • Theory!!


<p>Pressure-volume isothenns of carbon dioxide around its critical temperature, as calculated from  the van der Waals equation</p><ul><li><p>Theory!!</p></li></ul><p></p>
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Second virial coefficient

B2v(T)

  • the second virial coefficient is the most important because it reflects the first deviation from ideality as the pressure of gas increases, or the volume decreases

  • can be determined experimentally from the slope of a Z against P plot ( Z-1 = B2P(T)*P)


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Boyle Temperature

B2v(T) = 0

  • the repulsive and attractive parts of the intermolecular interactions cancel each other, and the gas appears t behave ideally


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At the critical point…

knowt flashcard image
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Critical point

max temperature before the gas becomes a liquid

  • any T scale we use to describe a gas is necessarily arbitrary. A gas does ā€œknowā€ its critical temperature and is therefore aware of its temperature relative to its critical temperature (its reduced T, TR)


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Figure 16.10

Z = (VbarR)/(VbarR - 1/3) - 9/(8 * VbarR * TR)

<p>Z = (Vbar<sub>R</sub>)/(Vbar<sub>R</sub> - 1/3) - 9/(8 * Vbar<sub>R </sub>* T<sub>R</sub>)</p>
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Virial Coefficients Depend on..

the forces of interaction between the molecules of the gas

  • if no forces, the second and third virial coefficient = 0


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B2v(T) = Vbar - Vbarideal measures…

IMFs

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Consider 2 interacting molecules, their interactions depend on…

  1. orientation

  2. distance


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Perturbation theory with large values of r…

  • models intermolecular forces


<ul><li><p>models intermolecular forces </p></li></ul><p></p>
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Repulsive ad attractive part of perturbation theory…

u(r) = + C12/r12 - C6/r6

first term is repulsive part and the second term is the attractive part

  • usually written as the Lennard-Jones Potential


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Lennard Jones Parameters

ε = well depth

  • measure of how strongly molecules attract each other

σ = separation at which u(r) = 0

  • measure of the size of the molecules


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Order of magnitude of ε…

it will be way less than bond strength (100-1000 KJ/mol) because it correlates to breaking intermolecular forces rather than intramolecular forces

ε ~ 0.24 Kcal/mol

εimf « bond strength

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4 ways molecules can store energy

  1. Translational

  2. Rotational

  3. Vibrational

  4. Electronic


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Translational is approximately a…

continuum: the levels are so close and almost on top of each other

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Spectroscopy

interactions of matter with light

Ephoton = hv = hc/lamda

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Boltzmann factor

If a system has states with energies E1, E2, E3, etc, the probability Pj, that the system will be in the state Ej depends exponentially on the energy of that state

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Type of Energy + Model

Translational → particle in a box

Rotational → rigid rotator

Vibrational → harmonic oscillator

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beta =

1/KBT

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The system partition function, Q, tells us…

the number of available states

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We postulate that the average ensemble energy is equal to…

the observed energy of a system

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The partition function of a system of independent, distinhuishable molecules is…

the product of molecular partition functions

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Fundamental Postulate of Physical Chemistry

the average of any quantity, as calculated using the probability function, is the same as the experimentally observed value of that quantity

  • experimentally observed energy of the system = u (which equals the average of E/n or E bar), or the internal energy