Chapter 2: Atomic Theory
Chapter 2: Atomic Theory
Quantum Model
A History of the Atom: Theories and Models
Exploration of how ideas about atoms have evolved through history.
The development of various atomic models:
Solid Sphere Model (1803) by John Dalton
Plum Pudding Model (1897) by J.J. Thomson
Nuclear Model (1911) by Ernest Rutherford
Planetary Model (1913) by Niels Bohr
Quantum Mechanical Model (1926) by Erwin Schrödinger
Major Atomic Models
Solid Sphere Model (John Dalton):
Atoms are indivisible.
Atoms of a particular element are identical.
Compounds are combinations of different types of atoms.
Recognition that atoms of different elements are distinct.
Plum Pudding Model (J.J. Thomson):
Discovery of electrons (initially called 'corpuscles') in 1897.
Model depicts atoms as electrons scattered within a positive charge cloud.
Identified electrons as components of atoms but did not account for the nucleus nor later experimental observations.
Nuclear Model (Ernest Rutherford):
Based on the gold foil experiment where positively charged alpha particles were directed at gold foil.
Most alpha particles passed through with slight deflection; significant deflection indicated a small, dense nucleus.
Positively charged particles concentrated in the nucleus and most of the atom consists of empty space.
Failed to explain how electrons could remain in orbit around the nucleus.
Planetary Model (Niels Bohr):
Modified Rutherford's model by suggesting electrons orbit the nucleus at fixed distances.
Introduced quantization of electron energy levels; electrons could only occupy certain energy levels.
Explained some elements' emission spectra but struggled with heavier atoms due to energy emissions suggesting electron should spiral into the nucleus.
Quantum Mechanical Model (Erwin Schrödinger):
Electrons are not confined to orbits; instead, they exist in ‘clouds of probability’ (orbitals).
Probability distribution of finding an electron at any point around the nucleus.
Widely regarded as the most accurate atomic model throughout current scientific understanding.
Electromagnetic Waves
Wavelength ($ ext{λ}$), frequency ($ ext{ν}$), and speed of light ($c$) are interrelated:
A: Longer wavelength corresponds to lower frequency.
B: Shorter wavelength corresponds to higher frequency.
C: Wave amplitude may vary.
Light exhibits dual characteristics: behaves as both wave and particle.
Photon: Basic unit of light energy.
Planck’s constant (h): $h = 6.626 imes 10^{-34} ext{ J s}$.
Electromagnetic Spectrum
Complete spectrum includes various radiation types characterized by varying wavelength and frequency.
Gamma rays, X-rays, Ultraviolet, Visible (400-750 nm), Infrared, Microwave, Radio.
Interaction between matter and light results in absorption or emission of photons, with energy determined by photon frequency or wavelength:
$E = h
u$ (energy of a photon).
Hydrogen Spectra
Absorption Spectrum shows wavelengths absorbed by hydrogen; Emission Spectrum demonstrates wavelengths emitted.
The Balmer series specifies electron transitions within hydrogen, correlating with discrete wavelengths emitted upon electron excitation.
Bohr Model Development
Johann Balmer, Theodore Lyman, Friedrich Paschen, Johannes Rydberg:
Identified spectral lines related to electron transitions in hydrogen.
Rydberg formula: Relates energy level transitions to emitted wavelength.
Basic transitions provided defined energies corresponding to light.
Team Modules
Example Problem 2.1.2: Interpreting Balmer Series
Find principal quantum numbers $(n, m)$ for the red line in the Balmer series using the Rydberg formula and wavelengths.
Understanding Electron Behavior
Experimental evidence substantiates wave-particle duality of electrons:
The double-slit experiment confirms interference patterns demonstrating wave-like behavior.
De Broglie’s hypothesis about electron wave properties expanded understanding of quantum mechanics:
$ ext{λ} = rac{h}{mv}$ where $h$ is Planck's constant, $m$ is mass, and $v$ is velocity.
Electrons behave as standing waves confined in atomic orbitals, quantifying energy levels at which they oscillate.
Quantum Mechanical Model Parameters
Four quantum numbers specify each electron:
Principal quantum number (n): Determines energy and size (positive integer).
Azimuthal quantum number (l): Determines shape of orbital (s, p, d, f).
Magnetic quantum number (mᵡ): Orientation in space.
Spin quantum number (mₛ): Describes electron spin direction (+1/2 or -1/2).
Pauli Exclusion Principle dictates that no two electrons in an atom can have identical quantum numbers.
Shapes of Atomic Orbitals
n=1: Only one orbital type indicated as $ ext{Ψ}_{1s} $.
Wavefunctions shape probability density.
n=2: Includes s (spherical) and p (dumbbell) orbitals with distinct orientations.
n=3: Provides additional orbitals with higher complexity.
Electron Configuration Overview
Arrangement of electrons crucial for understanding chemistry and predicting bonding reactions.
Arranged by filling orbitals based on increasing energy levels according to the Aufbau principle.
Cations & Anions defined by electron gain/loss corresponding to charge changes in atoms.
Summary of Periodic Trends
Effective Nuclear Charge (Z*): Represents net positive charge experienced by electrons in an atom, affecting atomic and ionic sizes, ionization energies, and electron affinities.
Ionization Energy (IE): Energy necessary to remove an electron; higher for noble gases due to their full valence shells.
Electron Affinity (EA): Measures how likely an atom is to gain an electron.
Electronegativity (EN): Ability to attract electrons in a bond; varies across the periodic table.
Types of Bonds
Ionic Bonds: Formed by complete transfer of electrons due to large electronegativity difference (>1.9).
Covalent Bonds: Characterized by sharing electrons with smaller electronegativity differences.
Polar vs Nonpolar Bonds: Based on the unequal or equal sharing of electron density, respectively.
Examples of Chemical Reactions & Structures
Lewis Structures guide electron distribution in molecules but do not indicate 3D shape.
Formal Charges calculate electron ownership in bonds based on the defined rules for electron sharing.
Examine reactions and propose structures considering octets or expanded octets for appropriate examples in bonding scenarios.