Chemistry - Quantum-Mechanical Model of the Atom

Beginnings of Quantum Mechanics

  • Classical physics believed physical phenomena were deterministic. Quantum mechanics discovered that for subatomic particles, the present condition does not determine the future condition.
  • Quantum mechanics is the foundation of chemistry, explaining the periodic table, chemical bonding, and applications like lasers and computers.

Electron Behavior

  • Electrons are incredibly small; a dust speck has more electrons than the number of people who have lived on Earth.
  • Observing electrons changes their behavior, making direct observation impossible.
  • The quantum-mechanical model explains how electrons exist and behave in atoms, helping predict atomic properties.

Nature of Light

  • Light is electromagnetic radiation composed of perpendicular oscillating electric and magnetic waves.
  • All electromagnetic waves travel at the speed of light: 3.00 \times 10^8 m/s.

Characterizing Waves

  • Amplitude is the height of the wave, determining light intensity.
  • Wavelength (\lambda) is the distance covered by the wave.
  • Frequency (\nu) is the number of waves passing a point per time unit (Hz or s\text{^{-1}}).
  • c = \nu \lambda: Wavelength and frequency are inversely proportional for electromagnetic waves.

Electromagnetic Spectrum

  • Visible light is a small part of the electromagnetic spectrum.
  • Shorter wavelength (high-frequency) light has higher energy.
  • High-energy electromagnetic radiation can damage biological molecules (ionizing radiation).

Interference

  • Constructive interference: Waves add to make a larger wave (in phase).
  • Destructive interference: Waves cancel each other (out of phase).

Diffraction

  • Diffraction occurs when waves bend around obstacles or openings of comparable size to their wavelength.
  • Diffraction of light through two slits creates an interference pattern.

Photoelectric Effect

  • Metals emit electrons when light shines on them (photoelectric effect).
  • Einstein proposed light energy comes in packets called quanta or photons.
  • E = \frac{hc}{\lambda}: Energy of a photon is proportional to its frequency and inversely proportional to its wavelength.

Atomic Spectroscopy and Bohr Model

  • Atoms release energy as light when excited.
  • Emission spectrum: A unique pattern of wavelengths emitted by an element.
  • Rydberg's equation: \frac{1}{\lambda} = R \left( \frac{1}{m^2} - \frac{1}{n^2} \right), where R is the Rydberg constant (1.097 \times 10^7 m^{\text{-1}}), and m and n are integers.
  • Bohr's model: Electrons exist in quantized orbits at fixed distances from the nucleus.

Wave Behavior of Electrons

  • De Broglie proposed particles have wavelike character.
  • \lambda = \frac{h}{mv}: Wavelength of a particle is inversely proportional to its momentum.

Complementary Properties

  • Wave-particle duality: You cannot simultaneously observe the wave and particle nature of an electron.

Uncertainty Principle

  • Heisenberg's uncertainty principle: \Delta x \cdot \Delta (mv) \geq \frac{h}{4\pi}. The more accurately you know the position of a small particle, the less you know about its velocity, and vice versa.

Determinacy Versus Indeterminacy

  • Classical physics: Particles move in a path determined by velocity, position, and forces.
  • Quantum mechanics: We can only predict the probability of finding an electron in a region.

Schrödinger’s Equation

  • Schrödinger’s equation calculates the probability of finding an electron with a particular amount of energy at a location.
  • Solutions produce wave functions (\psi) describing the wavelike nature of the electron.
  • H \psi = E \psi

Quantum Numbers

  • Three integer terms in the wave function determine the size, shape, and orientation of an orbital:
    • Principal quantum number (n)
    • Angular momentum quantum number (l)
    • Magnetic quantum number (m_l)
    • Spin quantum number (m_s)

Principal Quantum Number (n)

  • Characterizes the size and energy of the electron; can be any integer \geq 1.
  • E_n = -2.18 \times 10^{\text{-18}} J \left( \frac{1}{n^2} \right)

Angular Momentum Quantum Number (l)

  • Determines the shape of the orbital; values from 0 to (n-1).
    • l = 0: s orbitals (spherical)
    • l = 1: p orbitals (dumbbell-shaped)
    • l = 2: d orbitals
    • l = 3: f orbitals

Magnetic Quantum Number (m_l)

  • Specifies the orientation of the orbital in space; integers from -l to +l, including zero.

Spin Quantum Number (m_s)

  • Specifies the orientation of the electron spin; either +1/2 (spin up) or -1/2 (spin down).

Orbitals and Energy Levels

  • Orbitals with the same n are in the same principal energy level (shell).
  • Orbitals with the same n and l are in the same sublevel (subshell).

Energy Levels and Sublevels

  • Number of sublevels in a level = n.
  • Number of orbitals in a sublevel = (2l + 1).
  • Number of orbitals in a level = n^2.

Atomic Spectroscopy

  • Each wavelength corresponds to an electron transition between quantum-mechanical orbitals.
  • Excitation: Electron transitions from lower to higher energy level.
  • Relaxation: Electron transitions from higher to lower energy level, releasing a photon.
  • E{\text{photon}} = \Delta E{\text{electron}}

Predicting the Spectrum of Hydrogen

  • Wavelengths can be predicted by calculating the energy difference between states.

Probability Density

  • Represents the probability of finding an electron at a point in space.

Radial Distribution Function

  • The total probability of finding an electron within a thin spherical shell at a distance r from the nucleus.

S Orbitals

  • Spherical shape; number of nodes = (n - 1).

P Orbitals

  • Two-lobed; one node at the nucleus, total of n nodes.

D Orbitals

  • Mainly four-lobed.

F Orbitals

  • Mainly eight-lobed.

Phase of an Orbital

  • Wave functions can have positive or negative values (phase).
  • Interacting orbitals can be in phase (same sign) or out of phase (opposite signs).