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Lecture 7 CH131 Summer 1 2020 6/3/2020 12:46 PM Copyright © 2020 Dan Dill [email protected] 1 Lecture 7 CH131 Summer 1 Wednesday, June 3, 2020 Real gases Gas law for real gases: van der Waals equation Ch10: Solids, liquids and phase transitions Intermolecular forces IMF: H-bond, dipole-dipole, London IMFs determine relative boiling points Next lecture: Continue ch10 Real gases While the ideal gas law is the same for every gas, there are two effects in all real gases that are important at high gas densities due to temperatures close to condensation or very high pressures. Lecture 7 CH131 Summer 1 2020 8 Copyright © 2020 Dan Dill [email protected] Real gases The first effect is due to gas particles themselves taking up space. For example, we have seen that at 100, the density of H Oሺሻ is 0.0327 ୫୭୪ and the density of H O is 0.958 . Lecture 7 CH131 Summer 1 2020 9 Copyright © 2020 Dan Dill [email protected] TPThe density of H Oሺሻ is 0.0327 ୫୭୪ and the density of H O is 0.958 . Calculate how much space is taken up by the water molecules in 1 L of gaseous water at 100. 1. 0.0001 L 2. 0.0006 L 3. 0.001 L 4. 0.006 L 5. 0.01 L 6. 0.06 Copyright © 2020 Dan Dill [email protected] Lecture 7 CH131 Summer 1 2020 11 2 8 9 11

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Page 1: Lecture 7 CH131 Summer 1 2020 6/3/2020 12:46 PMgenchem.bu.edu/ch131-summer-1-2020/lectures/07-as-given.pdfLecture 7 CH131 Summer 1 2020 6/3/2020 12:46 PM Copyright © 2020 Dan Dill

Lecture 7 CH131 Summer 1 2020 6/3/2020 12:46 PM

Copyright © 2020 Dan Dill [email protected] 1

Lecture 7 CH131 Summer 1Wednesday, June 3, 2020

• Real gases• Gas law for real gases: van der Waals equation

Ch10: Solids, liquids and phase transitions• Intermolecular forces IMF : H-bond, dipole-dipole, London• IMFs determine relative boiling points

Next lecture: Continue ch10

Real gasesWhile the ideal gas law is the same for every gas, there are two effects in all real gases that are important at high gas densities due to temperatures close to condensation or very high pressures .

Lecture 7 CH131 Summer 1 2020

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Copyright © 2020 Dan Dill [email protected]

Real gasesThe first effect is due to gas particles themselves taking up space.

For example, we have seen that at 100℃, the density of H O 𝑔 is 0.0327and the density of H O 𝑙 is 0.958 .

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Copyright © 2020 Dan Dill [email protected]

TP The density of H O 𝑔 is 0.0327 and the density of H O 𝑙 is 0.958 .Calculate how much space is taken up by the water molecules in 1 L of gaseous water at 100℃.

1. 0.0001 L2. 0.0006 L3. 0.001 L4. 0.006 L5. 0.01 L6. 0.06

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Page 2: Lecture 7 CH131 Summer 1 2020 6/3/2020 12:46 PMgenchem.bu.edu/ch131-summer-1-2020/lectures/07-as-given.pdfLecture 7 CH131 Summer 1 2020 6/3/2020 12:46 PM Copyright © 2020 Dan Dill

Lecture 7 CH131 Summer 1 2020 6/3/2020 12:46 PM

Copyright © 2020 Dan Dill [email protected] 2

Real gasesThe density of H O 𝑔 is 0.0327 and the density of H O 𝑙 is 0.958 , so the volume taken up by the gaseous water as a liquid would be

𝑉 0.0327 mol . .

0.000614 L

This means that .

100% 0.06%

of the 1-L volume is taken up by the water molecules,

1 L 𝑉 𝑉 .

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Copyright © 2020 Dan Dill [email protected]

Real gasesMore generally, the volume of the container is expressed as empty space 𝑉 plus that taken up by the molecules themselves,

𝑉 𝑉 𝑏𝑛

Here the parameter van der Waals 𝑏 is the volume taken up by one mole of the molecules of the substance.

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Real gases𝑉 𝑉 𝑏𝑛

At high pressures, the volume of the molecules of a gas 𝑏𝑛 is no longer negligible relative to the volume of the container 𝑉 .

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Real gasesThe second effect is due to attraction of the gas particles for one another.

This attraction lessens the impact of each particle with the container walls and so reduces the pressure.

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Copyright © 2020 Dan Dill [email protected] 3

Real gasesThe reduction in pressure is proportional to the number of particles hitting the wall and the number of neighboring particles lessening each particle’s impact with the wall,

𝑃 𝑃 𝑎

The parameter van der Waals 𝑎 is a measure of the intermolecular attraction exerted between particles of the gas.

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Real gasesThe ideal gas law relates 𝑃 and 𝑉 , 𝑃 𝑉 𝑛𝑅𝑇.

Using the expressions 𝑉 𝑉 𝑏𝑛 and 𝑃 𝑃 𝑎 , we can rewrite the ideal gas law in terms of actual pressure and the actual container volume,

𝑃 𝑎 𝑉 𝑏𝑛 𝑛𝑅𝑇

This is known as the van der Waal equation.

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Real gasesComputations with the van der Waals equation are usually done by rearranging it for the observed pressure,

𝑃 𝑎

and using tabulated values of van der Waals 𝑎 and 𝑏.

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Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ K mol

For Cl2, 𝑎 6.58 bar L2/mol2 and 𝑏 0.0562 L/mol. What are the ideal and observed pressures of 3.00 mol of Cl2 confined in 4.00 L at 500. K?

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Copyright © 2020 Dan Dill [email protected] 4

Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ K mol

For Cl2, 𝑎 6.58 bar L2/mol2 and 𝑏 0.0562 L/mol. What are the ideal and observed pressures of 3.00 mol of Cl2 confined in 4.00 L at 500. K?

𝑃 31.3 bar confirm yourself

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Copyright © 2020 Dan Dill [email protected]

Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ K mol

For Cl2, 𝑎 6.58 bar L2/mol2 and 𝑏 0.0562 L/mol. What are the ideal and observed pressures of 3.00 mol of Cl2 confined in 4.00 L at 500. K?

𝑃 31.3 bar confirm yourself

𝑃 𝑎 32.5 bar 3.7 bar 28.8 bar confirm yourself

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Copyright © 2020 Dan Dill [email protected]

Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ K mol

For Cl2, 𝑎 6.58 bar L2/mol2 and 𝑏 0.0562 L/mol. What are the ideal and observed pressures of 3.00 mol of Cl2 confined in 4.00 L at 500. K?

𝑃 31.3 bar confirm yourself

𝑃 𝑎 32.5 bar 3.7 bar 28.8 bar confirm yourself

Since the observed pressure is smaller than the ideal pressure, the effect of 𝑎 is more important than 𝑏 at 500. K.

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Copyright © 2020 Dan Dill [email protected]

Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ K mol

For Cl2, 𝑎 6.58 bar L2/mol2 and 𝑏 0.0562 L/mol. What are the ideal and observed pressures of 3.00 mol of Cl2 confined in 4.00 L at 3000. K?

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Working with the van der Waals equation𝑝 𝑎 and 𝑅 0.08314 L bar/ K mol

For Cl2, 𝑎 6.58 bar L2/mol2 and 𝑏 0.0562 L/mol. What are the ideal and observed pressures of 3.00 mol of Cl2 confined in 4.00 L at 3000. K?

𝑃 187.1 bar confirm yourself

𝑃 𝑎 195.3 bar 3.7 bar 191.6 bar confirm yourself

Since the observed pressure is larger than the ideal pressure, the effect of 𝑏 is more important than 𝑎 at 3000. K.

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Copyright © 2020 Dan Dill [email protected]

Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ K mol

In general, the effect of 𝑏 is muted at low 𝑇 and so the effect of 𝑎 dominates there, while for high 𝑇 the effect of 𝑏 dominates.

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Copyright © 2020 Dan Dill [email protected]

Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ K mol

In general, the effect of 𝑏 is muted at low 𝑇 and so the effect of 𝑎 dominates there, while for high 𝑇 the effect of 𝑏 dominates.

For 3.00 mol of Cl2 confined in4.00 L, here is 1 versus 𝑇.

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Copyright © 2020 Dan Dill [email protected]

Working with the van der Waals equation𝑃 𝑎 and 𝑅 0.08314 L bar/ L mol

For Cl2, 𝑎 6.58 bar L2/mol2 and 𝑏 0.0562 L/mol. What is the observed and ideal pressures of 8.00 mol of Cl2 confined in 4.00 L at 27 ℃? Use

𝑃 49.9 bar

𝑃 𝑎 56.2 bar 26.3 bar 29.9 bar

Since the observed pressure is smaller than the ideal pressure, the effect of 𝑎 is more important than 𝑏 at 27 ℃

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Problem 7e:9.49 and 8e:9.51𝑎 3.640 L2bar/mol2

𝑏 0.04267 L/mol

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Why intermolecular forces (IMF)?We know from the van der Waals equation that gases attract one another.

Indeed, if they did not, they would not liquify.

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Intermolecular forces: electrical stickiness!Molecules attract one another, because of the attraction of opposite electrical charges.

The most specific and strongest IMF is “hydrogen bonding”: X—H ∙ ∙ ∙ Y

More common and of intermediate strength IMF is“dipole-dipole attraction”:

Always present and weakest IMF is “temporary dipole attraction” “London force” :

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Hydrogen bonding

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Ice and waterLecture 7 CH131 Summer 1 2020

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Ice and waterLecture 7 CH131 Summer 1 2020

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Hydrogen bond angle is 180°Copyright © 2020 Dan Dill [email protected]

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Lecture 7 CH131 Summer 1 2020

Hydrogen bonds are longer than typical bondsCopyright © 2020 Dan Dill [email protected]

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TP Which of the following cannot form H-bonds between themselves?

1. Ammonia, NH3

2. Methanol, CH3OH3. Ethanol, CH3CH2OH 4. Dimethyl ether, CH3OCH3

5. 1 and 36. 1 and 47. 2 and 48. All of the above can form hydrogen bonds with themselves

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Dipole-dipole attractionMolecules must be “polar”

What makes a molecule polar is unequal sharing of electron clouds.

Sharing tendency is proportional to electronegativity difference.

The greater the difference of electronegativities,the more unequal the sharing,

the more polar the shared electron cloud.

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TP Which of the following has dipole-dipole IMFs.

1. BFCl2, whose shape is trigonal-planar, like that of BF3

2. SCl2, which is a bent molecule, like H2O 3. NH2Cl, whose shape is trigonal-pyramidal, like that of NH3

4. OCS, which is a linear molecule, like CO2

5. All of the above6. None of the above

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Instantaneous dipoles → London forcesWhen one atom encounters another closely, the electrical repulsion between the electron clouds is similar to mismatched off-resonance interaction of light and matter.

The result is the electron clouds of all atoms always quiver slightly.

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Instantaneous dipoles → London forcesThis quivering means that electron clouds are momentarily lopsided, with the result that atom have momentary electrical dipoles.

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Instantaneous dipoles → London forcesShould another atom pass nearby, the momentary dipole will induce a dipole in the neighboring atom.

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Instantaneous dipoles → London forcesThe net result is that electron clouds on neighboring atoms and molecules attract one another, due to the London force.

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Relative boiling pointsBoiling means particles overcome attraction to their neighbors and depart the liquid.

Relative boiling points reflect relative strength of intermolecular forces …

London dispersion

Dipole-dipole interaction

Hydrogen bonding

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Why is SnH4 < SbH3 < TeH2?Copyright © 2020 Dan Dill [email protected] 7 CH131 Summer 1 2020

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Why is CH4 < SiH4 < GeH4 < SnH4?Copyright © 2020 Dan Dill [email protected] 7 CH131 Summer 1 2020

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