17: Temperature, Thermal Expansion, & Ideal Gas Law

17.1: Atomic Theory (pg 475) #

  • Atoms are the smallest unit of matter
  • Atomic unit: .$u = 1.66^{-27}$ kg
    • E.x. Hydrogen weighs .$1.0078 ua$
  • Molecular mass of a compound is the sum of the particles (atoms) in the compound

Terms #

  • Element: Substance that cannot be broken down into smaller substances (gold)
  • Molecule: Group of atoms held together by covalent bonds
  • Compound: Substance made from atoms combined in specific ratios

Brownian Motion #

  • Random movement seen in pollen/dust, as well as atoms
  • Using Brownian motion, Einstein found the size of an atom to be .$10^{-10}$ meters

Forces #

  • Atoms and molecules exert an (electric) attractive force on one another by default
  • If an atom/molecule gets too close to another, they exert a repelling force on one another
  • Matter states:
    • Solid:
      • Atoms held in matrix formation by strong attractive forces.
      • Atoms vibrate around their mean position
    • Liquid:
      • Force between atoms is weaker so atoms move more rapidly within
    • Gas:
      • Atom attractive forces are so weak compared to their kinetic energy that they move randomly
      • If two atoms collide, the attractive force is so weak that they may just bounce off one another

17.2: Temperature and Thermometers (pg 477) #

  • Matter property changes under different temperatures
    • Sidewalks expand under the sun
    • Electric resistance increases with heat
    • Lightbulb filament glows

Thermometers Types #

  • Originally used alcohol which expands linearly with heat (water doesn’t)
  • Bimetalic strips bend at slightly different rates under heat
  • Electronic thermometers measure resistance change and often have digital screens

Scales #

  • Fahrenheit: Water freezes at 32 and boils at 212 deg
  • Celsius: Water freezes at 0 and boils at 100 deg
  • Kelvin: Celsius + 273.15K. Written without degree sign. Absolute = 0K
  • Conversions: $$T(^\circ C) = \frac{5}{9}(T(^\circ F)-32)$$ $$T(^\circ F) = \frac{9}{5}(T(^\circ C)) + 32$$
  • Different materials expand at different rates ro we use constant-volume thermos because it’s pressure linearly relates to the temperature

17.3 0th Law of Thermodynamics (pg 480) #

  • If objects .$A$ and .$B$ are at equilibrium with object .$C$ , then .$A$ and .$B$ are also at equilibrium with one another
  • Systems naturally reach equilibrium over time

Thermal Expansion (pg 480) #

  • Most materials expand when heated

  • Expansion amount depends on the material

  • Equations (assuming a constant volume .$V$ )

    • Linear Expansion: $$\frac{dl}{dT} = \alpha(T)\cdot l$$ $$\Delta l \approxeq \alpha l_0 \cdot \Delta T$$ $$l_i + \Delta l = l_f = l_0 ( 1 + \alpha\Delta T)$$
      • .$\alpha$ is the coefficient of linear expansion and depends on the material
      • If .$\Delta T$ is too large such that the temperature dependence of .$\alpha$ is too large, we can do the following: $$\int_{l_i}^{l_f} \frac{1}{l}dl = \int_{T_i}^{T_f} \alpha(T) dT$$
    • Volume Expansion: $$\beta = \frac{1}{V} \frac{dV}{dT}$$ $$V_f \approxeq V_0 ( 1 + \beta\Delta T)$$
      • .$\beta \approx 3\cdot\alpha$ = coefficient of volume expansion.
    • Coefficient of expansion varies at extremely high heats so it only works with small .$\Delta T$ ’s
    • .$\alpha$ has the units of .$(^\circ C)^{-1}$
    • Materials must be isotropic (have same expansion properties in all directions) for us to say .$\alpha \approx 3\cdot\beta$
    • (Linear) expansion doesn’t exist for gas or liquids because they have no fixed space like solids.
  • Weird water property

    • .$0 - 4 ^\circ C$ : Water increases in density .$\rho^+\Longrightarrow$ decreases in volume .$V^-$
    • .$4^\circ C +$ : Water acts “normally”: increase in volume .$V$ proportional to temperature .$T$
    • This explains why pipes burt when frozen and why ice cubes float

17.5 Thermal Stresses (pg 484) #

  • When the ends a solid (rod) are fixed (such as in beams), temperature changes induce thermal stress due to the clamp limiting expansion/contraction
  • Process Steps:
    1. Beam tries to expand/contract by .$\Delta l$
    2. Mount reacts with an opposite reactive force, keeping it at it’s original length: $$\Delta l = \frac{1}{E} \cdot \frac{F}{A} \cdot l_0$$ where .$E$ is Young’s modulus for the material. We can also re-write for stress: $$\frac{F}{A} = \Delta l \cdot E \cdot \frac{l}{l_0} = (\alpha l_0 \Delta T) E \cdot \frac{l}{l_0} = \alpha E \Delta T$$

17.6 Gas Laws and Absolute Temperature (pg 484) #

  • Equation at State describes how pressure varies with Temperature, Number of Particles (Molecules), and Volume
  • State is the physical condition of a system
  • Equilibrium State: .$T, N, \&\ V = \text{Constant}$

Laws #

Ideal Gas Law Relation Equation

  • Assume that gasses aren’t too dense (so .$P \sim \text{atmospheric pressure}$ ) and that they aren’t close to liquefaction (boiling) point either (for oxygen, this is .$~183^\circ C$ .
  • Boyle’s Law
    • .$V \propto P^{-1}\ \text{[Constant Temperature]}$
    • .$P$ should be absolute, not gauge, pressure
    • Alternatively, .$PV = \text{Constant}$ or .$P_1V_1 = P_2V_2$
  • Charles’s Law
    • .$V \propto T\ \text{[Constant Pressure]}$
    • Alternatively, .$\frac{V_1}{T_1} = \frac{V_2}{T_2}$
  • Gay Lussac’s Law
    • .$P \propto T\ \text{[Constant Volume]}$
    • Alternatively, .$\frac{P_1}{T_1} = \frac{P_2}{T_2}$

17.7 Ideal Gas Law (486) #

$$PV = nRT = n k_B N_a T$$

  • .$P$ is the pressure of the gas [Pascals]
  • .$V$ is the volume of the gas [Cubic Meters]
  • .$n$ is the amount of substance of gas (also known as number of moles) [Moles]
  • .$R$ is the ideal, or universal, gas constant, equal to .$k_B \cdot N_a = 8.314 \frac{J}{K\cdot \text{mol}} = 0.0821 \frac{L\cdot atm}{\text{mol}\cdot K}$
    • Using mass of a gas, different gasses have different proportionality constants
    • So we used number of moles, in which case .$R$ becomes the constant for all gasses
  • .$k_B $ is the Boltzmann constant
    • Relates the average relative kinetic energy of particles in a gas with the thermodynamic temperature of the gas
  • .$N_a$ is the Avogadro constant
    • The number of particles that are contained in one mole of gas
  • .$T$ is the absolute temperature of the gas [Kelvins]
  • Ideal in that the equation only works for gasses around atmospheric pressure and not excessive temperatures

Moles #

  • Mole is the SI unit for amount of substance
  • 1 mole = Number of particles in .$12g$ of Carbon
  • 1 mole = Number of grams of a substance numerically equal to the molar mass
  • $$n \text{(moles)} = \frac{\text{mass (grams)}}{\text{molecular mass (g/mol)}}$$

17.8 Problem Solving with .$PV=nRT$ (pg 487) #

STP: Standard Temperature and Pressure #

  • .$T = 273 \text{K}$
  • .$P = 1.00 \text{atm} = 1.013*10^5 \text{N/m}^2 = 101.3 \text{kPA}$
  • .$1 \text{mol of ideal gas} = 22.4\text{L}$ in volume
  • If P is in liters and V is in atm, then we can use .$R=0.0821 \frac{\text{L} \cdot \text{atm}}{\text{mol} \cdot \text{K}}$
  • Since .$n$ and .$R$ are constants, we can say: $$\frac{P_1 V_1}{T_1} = \frac{P_2 V_2}{T_2}$$

17.9 Ideal Gas with Avogadro’s Number (pg 489) #

  • Avogadro’s hypothesis:
    • Equal volume of gas with the same .$P$ and .$T$ have an equal .$n$ umber of particles (molecules)
    • .$N_a$ is avogadro’s number: the number of particles that are contained in one mole of gas (or one gram of hydrogen).
    • .$N_a = 6.022 \cdot 10^23 \text{particles/mole}$
    • Therefore, if .$N$ is the number of molecules of a gas sample and .$n$ is the number of moles, then $$N = n\cdot N_A \Longrightarrow n = \frac{N}{N_A} \Longrightarrow PV = \frac{N}{N_A}RT = Nk_B T$$ where .$k_B $ is Boltzmann’s constant .$\frac{R}{N_A} = 1.38 \cdot 10^{-23} \frac{\text{J}}{\text{K}}$

17.10 Ideal Gas Temperature (pg 490) #

Phase Diagram

A typical phase diagram. The solid green line applies to most substances; the dashed green line gives the anomalous behavior of water

  • Triple point: A precise temperature and pressure where the three phases (gas, liquid, and solid) of a substance can coexist in thermodynamic equilibrium.
  • .$P_3 = 4.88\ \text{torr}; T_3 = 0.01^\circ C$ for water $$T = (273.16 K)\bigg(\frac{P}{P_3}\bigg)\ \text{[Ideal Gas, constant volume]}$$ $$T = (273.16 K)\lim_{P_3 \Longrightarrow 0}\bigg(\frac{P}{P_3}\bigg)\ \text{[Constant volume]}$$