CHEM1100 Study Guide: Quantum Theory and the Electronic Structure of Atoms

Chapter 3: Quantum Theory and the Electronic Structure of Atoms
3.1 Energy and Energy Changes
  • Definition of Energy: Capacity to do work or transfer heat.

  • Forms of Energy:

    • Kinetic Energy (EkE_k): Energy of motion.

    • Formula: Ek=12mu2E_k = \frac{1}{2} mu^2

    • Where:

      • mm = mass of the object

      • uu = velocity of the object

    • Special Note: Thermal energy is a specific form of kinetic energy, related to the random motion of atoms and molecules.

    • Potential Energy: Energy possessed by an object due to its position.

    • Two key forms for chemists:

      • Chemical Energy: Energy stored in the structural units of chemical substances.

      • Electrostatic Energy: Potential energy arising from the interactions between charged particles.

      • Formula: E<em>elE<em>{el} is proportional to Q</em>1Q2d\frac{Q</em>1 Q_2}{d}

      • Where Q<em>1Q<em>1 and Q</em>2Q</em>2 are charges and dd is the distance between them.

  • Interconvertibility of Energy: Kinetic and potential energy can be converted into one another. Total energy is constant (Law of Conservation of Energy).

3.2 Units of Energy
  • SI Unit for Energy: Joule (JJ)

    • Defined as the amount of energy possessed by a 2 kg2 \text{ kg} mass moving at 1 m/s1 \text{ m/s}.

    • Alternatively, it's the energy exerted when a force of 1 newton1 \text{ newton} is applied over a distance of 1 meter1 \text{ meter} (1 J=1 Nm1 \text{ J} = 1 \text{ N} \cdot \text{m}).

  • Kilojoule (kJkJ): A larger unit commonly used due to the small magnitude of a joule (1 kJ=1000 J1 \text{ kJ} = 1000 \text{ J}).

3.3 Worked Examples
Example 3.1: Calculate the kinetic energy of a helium atom moving at 125 m/s125 \text{ m/s}.
  • Given: Mass of helium atom = 4.003 amu4.003 \text{ amu} = 4.003×1.661×1024 g4.003 \times 1.661 \times 10^{-24} \text{ g}

  • Conversion:

    • Mass in kg = 4.003×1.661×1024 g×1 kg1000 g=6.649×1027 kg4.003 \times 1.661 \times 10^{-24} \text{ g} \times \frac{1 \text{ kg}}{1000 \text{ g}} = 6.649 \times 10^{-27} \text{ kg}

  • Calculation:

    • Ek=12(6.649×1027 kg)(125 m/s)2=5.19×1023 JE_k = \frac{1}{2}(6.649 \times 10^{-27} \text{ kg})(125 \text{ m/s})^2 = 5.19 \times 10^{-23} \text{ J}

Example 3.2: Attraction between different charges.
  • Comparison of Attractions:

    • Attraction between charges +2+2 and 2-2 is four times greater than between +1+1 and 1-1 (under the same distance).

3.2 The Nature of Light
  • Electromagnetic Spectrum: Range of all types of light, of which visible light is a small part.

  • Speed of Light in Vacuum:

    • Constant speed: c=2.99792458×108 m/sc = 2.99792458 \times 10^8 \text{ m/s} (commonly approximated as 3.00×108 m/s3.00 \times 10^8 \text{ m/s}).

  • Relationship among Speed, Frequency, and Wavelength:

    • Formula: c=ν×λc = \nu \times \lambda

    • Where:

    • ν\nu (nu) = frequency in hertz (HzHz)

    • λ\lambda (lambda) = wavelength in meters.

3.3 Properties of Waves
  • Characteristics of Electromagnetic Radiation:

    • Wavelength (λ\lambda): Distance between identical points on consecutive waves.

    • Frequency (ν\nu): Number of waves that pass a point per second.

    • Amplitude: Vertical distance from the midline of a wave to the peak or trough.

3.4 The Electromagnetic Spectrum
  • Components of Electromagnetic Wave: Contains both electric and magnetic components that share the same frequency and wavelength.

3.5 The Double-Slit Experiment
  • Interference Pattern: Occurs when light passes through two slits, demonstrating wave properties.

    • Constructive Interference: Occurs when waves are in phase.

    • Destructive Interference: Occurs with out-of-phase waves.

3.6 Worked Example 3.3
  • Laser Frequency Calculation: For a Neodymium-doped Yttrium Aluminum Garnet (Nd:YAG) laser at 532 nm532 \text{ nm} wavelength:

    • Convert to meters: 532 nm=5.32×107 m532 \text{ nm} = 5.32 \times 10^{-7} \text{ m}

  • Frequency Calculation:

    • Rearranged formula: ν=cλ\nu = \frac{c}{\lambda}

    • Result: ν=5.64×1014 s1\nu = 5.64 \times 10^{14} \text{ s}^{-1}

3.7 Quantum Theory
  • Historical Overview: Early physicists struggled to describe atoms with classical physics.

    • Classical laws do not apply to subatomic particles.

  • Quantization of Energy:

    • Hot solids emit electromagnetic radiation in discrete wavelengths.

  • Max Planck's Proposal: Energy is emitted/absorbed in packets called quanta.

  • Energy of a Quantum: E=hνE = h\nu where hh = Planck's constant, h=6.63×1034 Jsh = 6.63 \times 10^{-34} \text{ J} \cdot \text{s}.

    • Analogy: Like stepping on stairs (quantized) versus a ramp (continuous).

3.8 Photons and the Photoelectric Effect
  • Einstein's Explanation of the Photoelectric Effect: Light can eject electrons from metal surfaces when it meets a certain threshold frequency.

    • Below threshold frequency, no electron ejection occurs.

    • Each photon carries energy as Ephoton=hνE_{photon} = h\nu.

    • The kinetic energy (EkE_k) of the ejected electron relates to the equation:

    • Ek=hνWE_k = h\nu - W where WW is the binding energy of the electron.

3.9 Worked Example 3.4
  • Photon Energy Calculations:

    • (a) Photon with 50.0 nm50.0 \text{ nm} (infrared region): Use E=hνE = h\nu.

    • (b) 52 nm52 \text{ nm} (ultraviolet region): E calculation leads to number values via conversion to JJ.

    • (c) Max kinetic energy of an ejected electron from induced energy lesser than binding energy.

Conclusion: Summary of Key Points
  • Forms of Energy.

  • Law of Conservation of Energy.

  • Quantum Theory concepts, including energy quantization, photon behavior, and specific phenomena like the photoelectric effect and atomic line spectra.