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AP Chemistry Unit 3.4 Ideal Gas Laws Notes - New Syllabus 2024-2025

AP Chemistry Unit 3.4 Ideal Gas Laws Notes – New syllabus

AP Chemistry Unit 3.4 Ideal Gas Laws Notes – AP Chemistry –  per latest AP Chemistry Syllabus.

LEARNING OBJECTIVE

Explain the relationship between the macroscopic properties of a sample of gas or mixture of gases using the ideal gas law.

Key Concepts: 

  • The Ideal Gas Law
  • Partial Pressure & Total Pressure
  • Graphical Representations of the Gas Laws
  • Kinetic Molecular Theory
  • The Maxwell Boltzmann Distribution
  • Non-Ideal Behavior of Gases

AP Chemistry-Concise Summary Notes- All Topics

3.4.A.1 Ideal Gas Law: PV = nRT:

1. Macroscopic Properties of Gases:

PropertySymbolUnitDescriptionRelationship with Other Properties
PressurePatm, Pa, torr, mmHgThe force gas particles exert on the walls of their container.Pressure increases with more gas particles (n) or higher temperature (T).
VolumeVL, m³, cm³The space occupied by the gas.Volume increases with lower pressure (P) or higher temperature (T).
TemperatureTK (Kelvin)The measure of the average kinetic energy of gas particles.Temperature increases with more energy in the system, causing the gas to expand.
Number of MolesnmolThe quantity of gas particles (molecules or atoms).More moles (n) increase pressure (P) or volume (V) at constant temperature (T).
Ideal Gas ConstantR0.0821 L·atm/mol·K or 8.314 J/mol·KA constant used in the ideal gas law equation.Relates pressure, volume, and temperature for an ideal gas.

i. Ideal Gas Law

The relationships between these four properties are encapsulated in the Ideal Gas Law:

PV=nRTPV = nRT

Where:

  • P = pressure
  • V = volume
  • n = number of moles
  • R = the ideal gas constant (8.314 J/mol·K or 0.0821 L·atm/mol·K)
  • T = temperature in Kelvin

This equation shows that the pressure, volume, and temperature of a gas are all interdependent, and can be manipulated based on changes in the number of moles.

2. Gas Laws:

i. Boyle’s Law (P₁V₁ = P₂V₂) – At constant temperature, the volume of a gas is inversely proportional to its pressure.

ii. Charles’s Law (V₁/T₁ = V₂/T₂) – At constant pressure, the volume of a gas is directly proportional to its temperature.

iii. Avogadro’s Law (V₁/n₁ = V₂/n₂) – At constant temperature and pressure, the volume of a gas is directly proportional to the number of moles.

3. Ideal Gas Law:

i. Derivation of the Ideal Gas Law:

PV=nRTPV = nRT

The Ideal Gas Law relates pressure (P), volume (V), number of moles (n), and temperature (T) of an ideal gas through a constant

RR (the ideal gas constant). Here’s the step-by-step derivation and the assumptions that go into it:

a. Boyle’s Law (at constant temperature):

Boyle’s Law states that for a fixed amount of gas at constant temperature, the pressure (P) and volume (V) are inversely proportional:

P1VorPV=constantP \propto \frac{1}{V} \quad \text{or} \quad PV = \text{constant}

This relationship shows that when the volume of the gas decreases, the pressure increases, assuming the temperature is constant.

b. Charles’s Law (at constant pressure):

Charles’s Law states that for a fixed amount of gas at constant pressure, the volume (V) is directly proportional to its temperature (T) in Kelvin:

VTorVT=constantV \propto T \quad \text{or} \quad \frac{V}{T} = \text{constant}

This means that when the temperature increases, the volume also increases, as long as the pressure is kept constant.

c. Avogadro’s Law (at constant temperature and pressure):

Avogadro’s Law states that at constant temperature and pressure, the volume (V) of a gas is directly proportional to the number of moles (n):

VnorVn=constantV \propto n \quad \text{or} \quad \frac{V}{n} = \text{constant}

This implies that as more gas molecules are added to a fixed volume, the volume increases.

Combining the Three Laws:

To combine these three relationships into one, we consider each of them individually:

  • Boyle’s Law tells us that
    P1VP \propto \frac{1}{V}

    or

    PV=constantPV = \text{constant}
  • Charles’s Law tells us that
    VTV \propto T

    or

    VT=constant\frac{V}{T} = \text{constant}
  • Avogadro’s Law tells us that
    VnV \propto n

    or

    Vn=constant\frac{V}{n} = \text{constant}

If we combine these proportionalities, we get the general form of the ideal gas law:

PVnT=constant\frac{PV}{nT} = \text{constant}

This constant is the ideal gas constant,

RR so we get the equation:

PV=nRTPV = nRT

where

RR is the ideal gas constant, whose value is:

  • R = 0.0821 L·atm/mol·K
  • R = 8.314 J/mol·K (this is the SI unit value)
  • R = 1.987 cal/mol·K

ii. Application of the Ideal Gas Law

The Ideal Gas Law

PV=nRTPV = nRT

is incredibly useful for calculating one of the four macroscopic properties (P, V, T, or n) of an ideal gas if the other three are known.

iii. Assumptions of the Ideal Gas Law

a. Ideal Gas Behavior: The gas must behave ideally, meaning the gas molecules have no volume and experience no intermolecular forces (except elastic collisions).

b. High Temperature & Low Pressure: Real gases approximate ideal behavior at high temperatures and low pressures, where interactions between gas molecules are minimal.

4. Kinetic Molecular Theory:

The Kinetic Molecular Theory (KMT) provides a molecular-level explanation for the behavior of gases. It helps explain why gases follow the gas laws (like the Ideal Gas Law) and describes the motion and interactions of gas molecules. Here’s a summary of the key postulates of KMT and how they explain gas behavior:

i. Key Postulates of the Kinetic Molecular Theory:

a. Gas molecules are in constant, random motion.

    • Gas molecules move in all directions and with various speeds, colliding with one another and with the walls of the container. These collisions are elastic, meaning that no energy is lost in the collisions.
    • The molecules’ kinetic energy (energy of motion) is directly related to the temperature of the gas.

b. The volume of the gas molecules is negligible.

    • Compared to the space between gas molecules, the size of the molecules themselves is very small. This assumption allows us to treat gases as if they have no volume.
    • The volume of the gas is determined primarily by the space between the molecules (not their individual sizes).

c. Gas molecules do not exert attractive or repulsive forces on each other.

    • In an ideal gas, molecules do not interact with each other except when they collide. There are no intermolecular forces (like van der Waals forces or hydrogen bonds) acting between them.
    • This assumption makes gases behave differently from liquids and solids, where intermolecular forces play a significant role in their behavior.

d. The average kinetic energy of gas molecules is proportional to the temperature.

  • The kinetic energy of gas molecules is directly related to the temperature in Kelvin. The higher the temperature, the faster the molecules move and the greater their kinetic energy.
  • The equation for the average kinetic energy of a gas molecule is:

KE=32kBT\text{KE} = \frac{3}{2} k_B T

where

kBk_B is Boltzmann’s constant (1.38×1023J/K ) and

TT is the temperature in Kelvin.

e. Gas molecules undergo perfectly elastic collisions.

    • When gas molecules collide with each other or with the walls of the container, they do so in a way that the total kinetic energy of the system is conserved.
    • In other words, the energy lost by one molecule during a collision is exactly gained by the other molecule(s) involved in the collision.

ii. Molecular Explanation of Gas Behavior:

Using the postulates of the Kinetic Molecular Theory, we can explain the following behaviors of gases:

a. Pressure:

  • Pressure arises from the collisions of gas molecules with the walls of the container. Each time a molecule hits the wall, it exerts a small force. The total pressure is the sum of the forces from all the collisions per unit area.
  • Since gas molecules are in constant motion, the more frequent and forceful the collisions, the higher the pressure.

b. Volume and Temperature Relationship (Charles’s Law):

  • As temperature increases, the kinetic energy of the gas molecules also increases. This results in the molecules moving faster and colliding with the walls of the container more forcefully, causing the gas to expand (increase in volume).
  • In a rigid container, if the temperature is increased, the molecules speed up, and their kinetic energy increases, which could lead to increased pressure if the volume is held constant.

c. Pressure and Volume Relationship (Boyle’s Law):

  • As the volume of a gas decreases, the gas molecules have less space to move. This means that the number of collisions with the container walls increases, and the pressure increases, assuming the temperature and number of molecules are constant.

d. Number of Moles and Volume Relationship (Avogadro’s Law):

  • If the number of gas molecules increases while the temperature and pressure remain constant, the volume increases because there are more molecules colliding with the container walls. This corresponds to an increase in the frequency of collisions and the overall volume the gas occupies.

e. Gas Distribution and Speed of Molecules:

  • Not all molecules in a gas travel at the same speed. The distribution of molecular speeds is described by the Maxwell-Boltzmann distribution.
  • At higher temperatures, the distribution shifts, meaning more molecules have higher speeds. The average kinetic energy of the molecules increases with temperature, as described earlier.

5. Real Gases vs. Ideal Gases:

While Ideal Gases are a theoretical concept based on the assumptions of the Kinetic Molecular Theory (KMT), Real Gases are actual gases that exhibit behaviors influenced by intermolecular forces and the finite volume of gas molecules. The Ideal Gas Law is a good approximation for many gases under standard conditions, but real gases often deviate from this behavior under certain circumstances.

i. Assumptions of Ideal Gases (KMT):

The Ideal Gas Law assumes:

  • Gas molecules have no volume: They are considered point particles with negligible size.
  • No intermolecular forces: Gas molecules are assumed to not attract or repel each other.
  • Elastic collisions: Molecules collide without loss of kinetic energy.
  • Constant motion: Molecules are in continuous, random motion, and their average kinetic energy is proportional to the temperature.

Under these idealized conditions, gases obey the Ideal Gas Law perfectly:

 

PV=nRTPV = nRT

 

However, these assumptions don’t hold perfectly in reality, especially under extreme conditions.

ii. Real Gases and Deviations:

Real gases deviate from ideal behavior mainly because of intermolecular forces and the finite size of the gas molecules. These deviations are most noticeable at high pressure and low temperature.

a) Deviations at High Pressure:

  • High Pressure means gas molecules are forced closer together, and the volume of the gas molecules themselves becomes significant (i.e., the volume of the molecules is no longer negligible compared to the container’s volume).

  • Intermolecular Forces also become more important at high pressure. At closer distances, the attractive forces (e.g., van der Waals forces) between gas molecules cause the gas to behave less ideally.

    Effect of High Pressure:

    • At high pressure, the volume of the gas is less than predicted by the Ideal Gas Law. This happens because the molecules are packed together, and the space they occupy is more significant.
    • Attractive forces between molecules cause a reduction in the overall pressure because the molecules don’t collide with the walls of the container as frequently (due to the attractive forces slowing them down).

b) Deviations at Low Temperature:

  • Low Temperature means gas molecules move more slowly, and intermolecular forces become more significant.

  • As molecules slow down, attractive forces (like van der Waals forces) cause the gas to condense, and the gas no longer behaves ideally.

    Effect of Low Temperature:

    • At low temperatures, real gases tend to condense into a liquid because intermolecular forces are more prominent. The Ideal Gas Law assumes that there’s no attraction between gas molecules, but in reality, attractive forces become stronger as the molecules move slower at lower temperatures.
    • The pressure of a real gas is lower than predicted by the Ideal Gas Law because the molecules are not moving as fast, and attractive forces decrease the frequency of collisions with the container walls.

iii. Van der Waals Equation: A Correction to the Ideal Gas Law:

To account for the deviations of real gases from ideal behavior, we use the Van der Waals equation, which includes two correction factors:

  • Correction for intermolecular attractions: Attracting forces between gas molecules reduce the pressure, so the pressure term is adjusted.
  • Correction for molecular volume: The finite volume of gas molecules is accounted for, as real gas molecules occupy space.

The Van der Waals equation is:

 

(P+aV2)(Vb)=nRT\left(P + \frac{a}{V^2}\right)(V – b) = nRT

 

Where:

P = Pressure

V = Volume of the gas n

n = Number of moles

T = Temperature

R = Ideal gas constant

a = A constant that accounts for the attractive forces between molecules

b = A constant that accounts for the finite volume of gas molecules

iv. Why Do Real Gases Deviate?

  • Intermolecular forces: Real gas molecules attract or repel each other. For example, gases like oxygen (O₂) or nitrogen (N₂) exhibit weak London dispersion forces, while water vapor (H₂O) experiences hydrogen bonding, which leads to more significant deviations from ideal gas behavior.

  • Molecular size: The molecules of real gases have a finite size, meaning that the volume occupied by the molecules themselves must be accounted for, especially at high pressures.

  • Temperature: At low temperatures, the attractive forces become more significant as the gas molecules move more slowly. This causes real gases to condense, deviating from ideal behavior.

v. Conditions Under Which Gases Behave Ideally:

Real gases behave more ideally when:

  • High temperature: Molecules move faster, and intermolecular forces have less impact.
  • Low pressure: Molecules are far apart, so their volume and intermolecular forces become negligible.
  • Nonpolar gases: Gases with weak intermolecular forces (e.g., noble gases like helium, neon) behave more ideally than those with strong intermolecular forces (e.g., hydrogen bonding in water vapor).

3.4.A.2 Dalton’s Law of Partial Pressures:

1. Partial Pressure:

i. Partial Pressure – Concept and Calculation in a Mixture:

The partial pressure of a gas in a mixture refers to the pressure that the gas would exert if it occupied the entire volume by itself at the same temperature. In other words, each gas in a mixture behaves as though it is the only gas present and exerts its own pressure independently of the others.

The concept of partial pressure comes from Dalton’s Law of Partial Pressures, which states that the total pressure exerted by a mixture of gases is the sum of the partial pressures of the individual gases in the mixture.

ii. Dalton’s Law of Partial Pressures:

Dalton’s Law states:

Ptotal=P1+P2+P3++PnP_{\text{total}} = P_1 + P_2 + P_3 + \cdots + P_n

Where:

  • Ptotalis the total pressure exerted by the gas mixture.
  • P1,P2,,PnP_1, P_2, \ldots, P_n

    are the partial pressures of the individual gases in the mixture.

a. Definition of Partial Pressure

The partial pressure of each gas in a mixture is directly proportional to its mole fraction in the mixture. The mole fraction of a gas

ii is the ratio of the number of moles of that gas (nin_i) to the total number of moles of all gases in the mixture (ntotaln_{\text{total}}):

Xi=nintotalX_i = \frac{n_i}{n_{\text{total}}}

Where:

  • XiX_i

    is the mole fraction of gas i.

  • nin_i

    is the number of moles of gas i.

  • ntotaln_{\text{total}}

    is the total number of moles of all gases in the mixture.

The partial pressure of gas ii can then be written as:

Pi=XiPtotalP_i = X_i \cdot P_{\text{total}}

or

Pi=nintotalPtotalP_i = \frac{n_i}{n_{\text{total}}} \cdot P_{\text{total}}

b. Calculation of Partial Pressures:

  1. Determine the total number of moles of gas in the mixture by adding up the moles of each individual gas.
    ntotal=n1+n2+n3++nnn_{\text{total}} = n_1 + n_2 + n_3 + \cdots + n_n
  2. Find the mole fraction of each gas:
    Xi=nintotalX_i = \frac{n_i}{n_{\text{total}}}
  3. Use Dalton’s Law to calculate the partial pressure of each gas:
    Pi=XiPtotal=nintotalPtotalP_i = X_i \cdot P_{\text{total}} = \frac{n_i}{n_{\text{total}}} \cdot P_{\text{total}}

c. Key Points to Remember:

  1. Partial pressures are directly proportional to the mole fractions of gases in a mixture.
  2. The total pressure is simply the sum of all the partial pressures.
  3. The mole fraction is a useful concept because it allows you to calculate the partial pressure of any gas in a mixture as a fraction of the total pressure.

iii. Applications of Dalton’s Law of Partial Pressures:

a. In breathing gases (like in scuba diving), knowing the partial pressure of gases like oxygen and nitrogen is important for calculating the risks of nitrogen narcosis or oxygen toxicity.

b. In chemical reactions that involve gaseous reactants, the partial pressures of the gases involved are often used to apply the ideal gas law to calculate quantities of substances or to use in Le Chatelier’s principle to predict how a reaction will shift in response to changes in pressure.

2. Mole Fraction (X):

The mole fraction of a component in a mixture is a way of expressing the proportion of moles of that component relative to the total number of moles in the mixture. Mole fraction is particularly useful when dealing with gas mixtures, as it directly relates to the partial pressure of each gas in the mixture.

i. Definition of Mole Fraction (X):

The mole fraction of a component ii in a mixture is defined as the ratio of the number of moles of that component (nin_i) to the total number of moles of all components (ntotaln_{\text{total}}) in the mixture:

Xi=nintotalX_i = \frac{n_i}{n_{\text{total}}}

Where:

  • XiX_i

    is the mole fraction of gas i

  • nin_i

    is the number of moles of gas i.

  • ntotaln_{\text{total}}

    is the total number of moles of all gases in the mixture.

ii. Mole Fraction and Partial Pressure:

Dalton’s Law of Partial Pressures states that the partial pressure of a gas in a mixture is proportional to its mole fraction. In fact, the mole fraction of a gas is equal to the ratio of its partial pressure to the total pressure of the gas mixture.

The relationship between mole fraction and partial pressure is given by:

Pi=XiPtotalP_i = X_i \cdot P_{\text{total}}

Where:

  • PiP_i

    is the partial pressure of gas i.

  • XiX_i

    is the mole fraction of gas i.

  • PtotalP_{\text{total}}

    is the total pressure of the gas mixture.

iii. Understanding the Relationship:

  • The mole fraction Xi tells you how much of the total mixture is made up of a particular gas.
  • Since the partial pressure of each gas is proportional to its mole fraction, a gas with a higher mole fraction will exert a higher partial pressure in the mixture.
  • If the mole fraction of a gas in the mixture increases, its partial pressure also increases proportionally, as long as the total pressure remains constant.

iv. Key Points:

  1. Mole fraction and partial pressure are proportional to each other.

    • If the mole fraction of a gas increases, its partial pressure increases.
    • If the mole fraction of a gas decreases, its partial pressure decreases.
  2. The mole fraction is dimensionless, as it is a ratio of the number of moles, and it ranges from 0 to 1.

  3. The total partial pressure is the sum of the individual partial pressures of all gases in the mixture, as per Dalton’s Law.

Ptotal=P1+P2++PnP_{\text{total}} = P_1 + P_2 + \cdots + P_n

v. Applications of Mole Fraction and Partial Pressure:

  • In chemical reactions involving gases, knowing the partial pressure of each reactant can help determine the rate of reaction using rate laws or calculate equilibrium concentrations using the law of mass action.
  • Mole fractions are often used in colligative properties like vapor pressure lowering, boiling point elevation, and freezing point depression in solutions.
  • In scuba diving and other fields involving gases under pressure, understanding partial pressures helps to prevent conditions like nitrogen narcosis or oxygen toxicity.

3. Dalton’s Law:

Dalton’s Law of Partial Pressures states that in a mixture of non-reacting gases, the total pressure exerted by the mixture is the sum of the partial pressures of the individual gases. Each gas in the mixture exerts a pressure independently of the others, and this pressure is directly proportional to the amount (moles) of gas present.

i. Formula for Total Pressure (Pₜₒₜₐₗ):

Dalton’s Law can be expressed as:

Ptotal=P1+P2+P3++PnP_{\text{total}} = P_1 + P_2 + P_3 + \cdots + P_n

Where:

  • PtotalP_{\text{total}}

    is the total pressure of the gas mixture.

  • P1,P2,,PnP_1, P_2, \dots, P_n

    are the partial pressures of the individual gases in the mixture.

ii. Partial Pressure of Each Gas:

The partial pressure of a gas is the pressure it would exert if it occupied the entire volume on its own at the same temperature. According to Dalton’s Law, the partial pressure of any gas in the mixture is proportional to its mole fraction in the mixture.

For a specific gas AA the partial pressure can be calculated using the formula:

PA=XAPtotalP_A = X_A \cdot P_{\text{total}}

Where:

  • PAP_A

    is the partial pressure of gas A.

    A
  • XAX_A

    is the mole fraction of gas A in the mixture.

  • PtotalP_{\text{total}}

    is the total pressure of the gas mixture.

iii. Mole Fraction (Xₐ) of a Gas:

The mole fraction

XAX_A is defined as the ratio of the moles of gas AA to the total number of moles in the mixture:

XA=nAntotalX_A = \frac{n_A}{n_{\text{total}}}

Where:

  • nAn_A

    is the number of moles of gas A.

  • ntotaln_{\text{total}}

    is the total number of moles of all gases in the mixture.

iv. Key Relationship:

  • The mole fraction
    XAX_A

    represents the fraction of the total moles that are gas A

  • The partial pressure
    PAP_A

    is therefore directly proportional to the mole fraction

    XAX_A

    and thus, the partial pressure of any gas in a mixture depends on both its mole fraction and the total pressure.

    P_{\text{N}_2} = 6.0 \, \text{atm}

3.4.A.3 Graphical Representations of Gas Behavior (P, V, T, n):

1. Ideal Gas Law:

VariableDescriptionRelationshipConstant
PPressureDirectly proportional to T and n, inversely proportional to Vn, T, and V constant
VVolumeDirectly proportional to T and n, inversely proportional to Pn, T, and P constant
TTemperatureDirectly proportional to P and V, inversely proportional to nP, V, and n constant
nNumber of molesDirectly proportional to P and V, inversely proportional to TP, V, and T constant

In the Ideal Gas Law

PV=nRTPV = nRT

, the behavior of these variables can be summarized:

  • If n (the number of moles) is constant, P increases as V decreases (Boyle’s Law), and P increases as T increases (Gay-Lussac’s Law).
  • If P (pressure) is constant, V increases as T increases (Charles’ Law).
  • If V (volume) is constant, P increases as T increases (Gay-Lussac’s Law).

2. Boyle’s Law:

VariableDescriptionRelationshipConstant
PPressure of the gasInversely proportional to VT and n constant
VVolume of the gasInversely proportional to PT and n constant
TTemperature of the gasConstant (does not change)
nNumber of moles of the gasConstant (does not change)

Boyle’s Law:

P×V=constant(at constant T and n)P \times V = \text{constant} \quad \text{(at constant T and n)}

So, as V increases, P decreases, and vice versa, as long as T and n are constant.

3. Charles’s Law:

VariableDescriptionRelationshipConstant
VVolume of the gasDirectly proportional to TP and n constant
TTemperature of the gasDirectly proportional to VP and n constant
PPressure of the gasConstant (does not change)
nNumber of moles of the gasConstant (does not change)

Charles’s Law Formula:

VT=constant(at constant P and n)\frac{V}{T} = \text{constant} \quad \text{(at constant P and n)}

This means if the temperature increases, the volume must increase as well, and vice versa, as long as pressure and the number of moles of gas remain constant.

4. Gay-Lussac’s Law:

VariableDescriptionRelationshipConstant
PPressure of the gasDirectly proportional to TV and n constant
TTemperature of the gasDirectly proportional to PV and n constant
VVolume of the gasConstant (does not change)
nNumber of moles of the gasConstant (does not change)

Gay-Lussac’s Law Formula:

PT=constant(at constant V and n)\frac{P}{T} = \text{constant} \quad \text{(at constant V and n)}

This means that as temperature increases, the pressure increases, and as temperature decreases, pressure decreases, assuming the volume and number of moles remain constant.

5. Avogadro’s Law:

VariableDescriptionRelationshipConstant
VVolume of the gasDirectly proportional to nT and P constant
nNumber of moles of the gasDirectly proportional to VT and P constant
TTemperature of the gasConstant (does not change)
PPressure of the gasConstant (does not change)

Avogadro’s Law Formula:

Vn=constant(at constant T and P)\frac{V}{n} = \text{constant} \quad \text{(at constant T and P)}

This means that increasing the number of gas molecules will result in a proportional increase in volume, and vice versa, as long as temperature and pressure stay constant.

6. Isothermal and Adiabatic Processes:

i. Isothermal Process:

An isothermal process occurs when the temperature of the gas remains constant throughout the process. In this case, the internal energy of an ideal gas does not change (since internal energy depends on temperature), and the gas does work on its surroundings or has work done on it, but the temperature stays the same.

Key Points:

  • Constant temperature (T=constant)
  • The internal energy of the gas does not change (for an ideal gas).
  • Heat Q is exchanged to maintain temperature, even as the volume or pressure changes.
  • The pressure-volume relationship follows Boyle’s Law: P×V=constant.P \times V = \text{constant}

Graph of Isothermal Process:
The graph of an isothermal process is a hyperbola on a P-V (Pressure-Volume) graph.

  • As volume increases, pressure decreases, and vice versa, while the temperature remains constant.

Equation:

P×V=constant(at constant T)P \times V = \text{constant} \quad (\text{at constant T})

This means the pressure is inversely proportional to the volume for an isothermal process.

ii. Adiabatic Process:

An adiabatic process occurs when there is no heat exchange with the surroundings (i.e.,Q=0Q = 0). In this case, any work done by the gas or on the gas results in a change in the internal energy, which leads to a change in temperature.

Key Points:

  • No heat exchange (Q=0).
  • The temperature of the gas changes as it expands or compresses.
  • The relationship between pressure and volume for an adiabatic process follows the equation:
    P×Vγ=constantP \times V^{\gamma} = \text{constant}

    where

    γ=CpCv\gamma = \frac{C_p}{C_v}

    is the adiabatic index (ratio of specific heats).

  • For an ideal gas undergoing an adiabatic expansion, the gas cools as it expands, and warms up as it is compressed.

Graph of Adiabatic Process:
The graph of an adiabatic process is a steeper curve than the isothermal curve on a P-V graph. The adiabatic curve is steeper because the temperature changes as the gas expands or compresses.

Equation:

P×Vγ=constant(for adiabatic process)P \times V^{\gamma} = \text{constant} \quad (\text{for adiabatic process})

This shows that pressure and volume are related by a power law, where the constant depends on the specific heat ratio of the gas.

iii. Comparison of Graphs:

ProcessType of ProcessGraph ShapeKey Feature
Isothermal

Constant temperature (

T=constantT = \text{constant}

)

Hyperbolic curve on a P-V graph.Temperature remains constant; Pressure and volume are inversely proportional.
Adiabatic

No heat exchange (

Q=0Q = 0

)

Steeper curve than isothermal on a P-V graph.No heat is exchanged; temperature changes with volume and pressure changes.

 

Example of Each Process:

  • Isothermal Expansion: If a gas expands slowly in a piston, it can absorb heat from the surroundings to maintain a constant temperature while doing work.
  • Adiabatic Expansion: If a gas expands rapidly (such as when a gas is released from a pressurized container), it does so without exchanging heat, leading to a temperature drop.

OLD CONTENT

A Gas (Review)

  • Uniformly fills any container (have variable volume)
  • Mixes spontaneously and completely with any other gas
  • Exerts pressure on its surroundings

 Pressure

  • Is equal to force/unit area
  • Pressure equals the number of collisions with the particles and its container
    • Collision = force; container = area → more collisions = higher pressure
  • Gasses have random motions and travel at high speeds → when they strike the side of the container they exert a force on that area = pressure
  • SI units = newton/meter² = 1 Pascal (Pa)

The Gas Laws

Boyle’s Law

  • Pressure and volume (and KE) are inversely related
    • Temperature must be constant
  • Units do not matter as long as they are the same on both sides
  • A gas that strictly obeys Boyle’s law is called an ideal gas

Charles Law

  • The volume of a gas is directly proportional to temperature
    • Pressure must be constant
  • In all gas laws, temperature must be in kelvin
  • Gas is heated to a higher temperature → avg KE & speed of gas increase → they hit the walls more often/with more
    • In order to keep the pressure constant, need to increase the volume of the container

Avogadro’s Law

  • The volume of a gas is directly proportional to the number of moles of gas
    • Temperature and pressure must be constant

Gay-Lussac’s Law

  • Pressure and temperature are directly related
    • Volume must be constant

Combined Gas Laws

  • Not that common on AP exam
  • If the moles of gas remains constant, use this formula and cancel out the other things that don’t change

 The Ideal Gas Laws

  • PV=nRT
    • P = pressure in atm, torr, kPa
    • V = volume in liters
    • n = moles
    • T = temperature in Kelvin
    • R = ideal/universal gas constant (on reference sheet)
      • = 0.08206 L atm K^-1 mol ^-1
      • = 62.4 L torr K^-1 mol^-1
      • = 8.314 L kPa K^-1 mol^-1
  • A gas that obeys this equation is said to behave ideally
  • Assumes that particles have no attraction

Gas Stoichiometry

  • Standard Temperature and Pressure (STP): The conditions 0 ℃ and 1 atm
    • The molar volume of an ideal gas is 22.42 L at STP

Gas Density and Molar Mass

Dalton’s Law of Partial Pressure

  • Dalton’s law of partial pressures: the pressure exerted by a mixture of gases in a container is the sum of the individual pressure exerted by each gas if it were alone
    • PTOTAL  = P1 + P2 + P3 + …..
    • P1 , P2 , P3 , represent each partial pressure: the pressure that a particular gas would exert if it were alone in the container.
  • Partial Pressure Formula:
    • Mole fraction() : Moles of gas / total gas moles (unitless)

Valve Questions

  • Have to use Boyle’s law to find P₂ and then add them up to calculate Ptotal
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